PrismaX/SFE · Datasets at Hugging Face

id stringlengths 9 9	question stringclasses 284 values	options listlengths 0 15	answer stringlengths 1 1.49k	images listlengths 1 18	question_type stringclasses 3 values	field stringclasses 5 values	lang stringclasses 2 values
A009/0000	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.12627530097961426	[ "A009_dataset_0_ed03e981d759eec86cddd74b25587d14.png" ]	exact_match	astronomy	en
A009/0001	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	-0.003634300082921982	[ "A009_dataset_1_50826daea38941bbe699ac0bb3913148.png" ]	exact_match	astronomy	en
A009/0002	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.09097830206155777	[ "A009_dataset_2_a73c1adadbedc614c4f75a8d36d13014.png" ]	exact_match	astronomy	en
A009/0003	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.04309830069541931	[ "A009_dataset_3_75af86379235b439bbf4bc672d833e9a.png" ]	exact_match	astronomy	en
A009/0004	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.1657153069972992	[ "A009_dataset_4_87c27c010f2d30099c2049d0bb3422ed.png" ]	exact_match	astronomy	en
A009/0005	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.01240879949182272	[ "A009_dataset_5_6989de41d1fc4afb6057008cb9888947.png" ]	exact_match	astronomy	en
A009/0006	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	-0.019711699336767197	[ "A009_dataset_6_3b5de29489297138881515152422737a.png" ]	exact_match	astronomy	en
A009/0007	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.07547600567340851	[ "A009_dataset_7_cf4119bbf6760156370989c891bca499.png" ]	exact_match	astronomy	en
A009/0008	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	-0.05262269824743271	[ "A009_dataset_8_c94dbc12e17a10eece0ef1b3c5198f9e.png" ]	exact_match	astronomy	en
A009/0009	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	-0.04264570027589798	[ "A009_dataset_9_f66e52ce06c2c38376abdf5ec5cdb736.png" ]	exact_match	astronomy	en
A009/0010	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.09061399847269058	[ "A009_dataset_10_09692d1fe9cc96b02a9cf96dadc7ca52.png" ]	exact_match	astronomy	en
A009/0011	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.05570400133728981	[ "A009_dataset_11_5c9a6c649cdd21a3bc31c8c05ebd1ce4.png" ]	exact_match	astronomy	en
A009/0012	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.10715000331401825	[ "A009_dataset_12_e42b3e948d97d6c0ca9a62395ae8ddec.png" ]	exact_match	astronomy	en
A009/0013	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.03361229971051216	[ "A009_dataset_13_320ddaf07d4e769e3b0e61d147aa9a80.png" ]	exact_match	astronomy	en
A009/0014	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.08316600322723389	[ "A009_dataset_14_e8584fe473fcc39328f8313c3863ae6b.png" ]	exact_match	astronomy	en
A009/0015	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.08924499899148941	[ "A009_dataset_15_155143b17860a020a31e51491f5bec9e.png" ]	exact_match	astronomy	en
A009/0016	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.027879400178790092	[ "A009_dataset_16_524a660ec08db43ba46b734a79e3466a.png" ]	exact_match	astronomy	en
A009/0017	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.03957600146532059	[ "A009_dataset_17_9a889f7c8fc65fc3ea31dfe4076c519d.png" ]	exact_match	astronomy	en
A009/0018	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.08698400110006332	[ "A009_dataset_18_8795c19633fdf5d5d3a52900521a5626.png" ]	exact_match	astronomy	en
A009/0019	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.	[]	0.025318801403045654	[ "A009_dataset_19_ae6c1f66e68793b8a5a7b30fccdce2d4.png" ]	exact_match	astronomy	en
A006/0000	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5402.044921875	[ "A006_dataset_0_ed03e981d759eec86cddd74b25587d14.png" ]	exact_match	astronomy	en
A006/0001	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5645.55419921875	[ "A006_dataset_1_50826daea38941bbe699ac0bb3913148.png" ]	exact_match	astronomy	en
A006/0002	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5501.77294921875	[ "A006_dataset_2_a73c1adadbedc614c4f75a8d36d13014.png" ]	exact_match	astronomy	en
A006/0003	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5740.89892578125	[ "A006_dataset_3_75af86379235b439bbf4bc672d833e9a.png" ]	exact_match	astronomy	en
A006/0004	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5555.275390625	[ "A006_dataset_4_87c27c010f2d30099c2049d0bb3422ed.png" ]	exact_match	astronomy	en
A006/0005	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5945.7509765625	[ "A006_dataset_5_6989de41d1fc4afb6057008cb9888947.png" ]	exact_match	astronomy	en
A006/0006	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4784.11669921875	[ "A006_dataset_6_3b5de29489297138881515152422737a.png" ]	exact_match	astronomy	en
A006/0007	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4914.67529296875	[ "A006_dataset_7_cf4119bbf6760156370989c891bca499.png" ]	exact_match	astronomy	en
A006/0008	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	3767.69384765625	[ "A006_dataset_8_c94dbc12e17a10eece0ef1b3c5198f9e.png" ]	exact_match	astronomy	en
A006/0009	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	6185.44384765625	[ "A006_dataset_9_f66e52ce06c2c38376abdf5ec5cdb736.png" ]	exact_match	astronomy	en
A006/0010	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4742.7451171875	[ "A006_dataset_10_09692d1fe9cc96b02a9cf96dadc7ca52.png" ]	exact_match	astronomy	en
A006/0011	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5031.263671875	[ "A006_dataset_11_5c9a6c649cdd21a3bc31c8c05ebd1ce4.png" ]	exact_match	astronomy	en
A006/0012	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4974.60107421875	[ "A006_dataset_12_e42b3e948d97d6c0ca9a62395ae8ddec.png" ]	exact_match	astronomy	en
A006/0013	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5049.7685546875	[ "A006_dataset_13_320ddaf07d4e769e3b0e61d147aa9a80.png" ]	exact_match	astronomy	en
A006/0014	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4975.68896484375	[ "A006_dataset_14_e8584fe473fcc39328f8313c3863ae6b.png" ]	exact_match	astronomy	en
A006/0015	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4918.45166015625	[ "A006_dataset_15_155143b17860a020a31e51491f5bec9e.png" ]	exact_match	astronomy	en
A006/0016	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4892.9208984375	[ "A006_dataset_16_524a660ec08db43ba46b734a79e3466a.png" ]	exact_match	astronomy	en
A006/0017	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	4659.77734375	[ "A006_dataset_17_9a889f7c8fc65fc3ea31dfe4076c519d.png" ]	exact_match	astronomy	en
A006/0018	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	5049.44482421875	[ "A006_dataset_18_8795c19633fdf5d5d3a52900521a5626.png" ]	exact_match	astronomy	en
A006/0019	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.	[]	3990.48583984375	[ "A006_dataset_19_ae6c1f66e68793b8a5a7b30fccdce2d4.png" ]	exact_match	astronomy	en
A007/0000	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.417627334594727	[ "A007_dataset_0_ed03e981d759eec86cddd74b25587d14.png" ]	exact_match	astronomy	en
A007/0001	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.1094794273376465	[ "A007_dataset_1_50826daea38941bbe699ac0bb3913148.png" ]	exact_match	astronomy	en
A007/0002	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.304114818572998	[ "A007_dataset_2_a73c1adadbedc614c4f75a8d36d13014.png" ]	exact_match	astronomy	en
A007/0003	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.4836273193359375	[ "A007_dataset_3_75af86379235b439bbf4bc672d833e9a.png" ]	exact_match	astronomy	en
A007/0004	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.271500110626221	[ "A007_dataset_4_87c27c010f2d30099c2049d0bb3422ed.png" ]	exact_match	astronomy	en
A007/0005	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.123192310333252	[ "A007_dataset_5_6989de41d1fc4afb6057008cb9888947.png" ]	exact_match	astronomy	en
A007/0006	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.536657333374023	[ "A007_dataset_6_3b5de29489297138881515152422737a.png" ]	exact_match	astronomy	en
A007/0007	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	3.3005595207214355	[ "A007_dataset_7_cf4119bbf6760156370989c891bca499.png" ]	exact_match	astronomy	en
A007/0008	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.6511921882629395	[ "A007_dataset_8_c94dbc12e17a10eece0ef1b3c5198f9e.png" ]	exact_match	astronomy	en
A007/0009	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	4.346240997314453	[ "A007_dataset_9_f66e52ce06c2c38376abdf5ec5cdb736.png" ]	exact_match	astronomy	en
A007/0010	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	3.25662899017334	[ "A007_dataset_10_09692d1fe9cc96b02a9cf96dadc7ca52.png" ]	exact_match	astronomy	en
A007/0011	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	3.456131935119629	[ "A007_dataset_11_5c9a6c649cdd21a3bc31c8c05ebd1ce4.png" ]	exact_match	astronomy	en
A007/0012	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	2.3882505893707275	[ "A007_dataset_12_e42b3e948d97d6c0ca9a62395ae8ddec.png" ]	exact_match	astronomy	en
A007/0013	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	3.2916665077209473	[ "A007_dataset_13_320ddaf07d4e769e3b0e61d147aa9a80.png" ]	exact_match	astronomy	en
A007/0014	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	2.4835898876190186	[ "A007_dataset_14_e8584fe473fcc39328f8313c3863ae6b.png" ]	exact_match	astronomy	en
A007/0015	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	2.4800865650177	[ "A007_dataset_15_155143b17860a020a31e51491f5bec9e.png" ]	exact_match	astronomy	en
A007/0016	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	2.6240267753601074	[ "A007_dataset_16_524a660ec08db43ba46b734a79e3466a.png" ]	exact_match	astronomy	en
A007/0017	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	2.384700059890747	[ "A007_dataset_17_9a889f7c8fc65fc3ea31dfe4076c519d.png" ]	exact_match	astronomy	en
A007/0018	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	2.447835922241211	[ "A007_dataset_18_8795c19633fdf5d5d3a52900521a5626.png" ]	exact_match	astronomy	en
A007/0019	<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.	[]	1.1980178356170654	[ "A007_dataset_19_ae6c1f66e68793b8a5a7b30fccdce2d4.png" ]	exact_match	astronomy	en
A001/0000	<image> What is the structure of galaxy in the image?	[ "(A) Disturbed Galaxies", "(B) Merging Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Edge-on Galaxies with out Bulge" ]	['A']	[ "A001_dataset_0_c48e56e5a0a10c36c26fd9237ce84d99.png" ]	mcq	astronomy	en
A001/0001	<image> What is the structure of galaxy in the image?	[ "(A) Edge-on Galaxies with Bulge", "(B) In-between Round Smooth Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Merging Galaxies" ]	['D']	[ "A001_dataset_1_2a6880a64e11c8a34108c9bbcc91477b.png" ]	mcq	astronomy	en
A001/0002	<image> What is the structure of galaxy in the image?	[ "(A) Edge-on Galaxies with out Bulge", "(B) Round Smooth Galaxies", "(C) In-between Round Smooth Galaxies", "(D) Merging Galaxies" ]	['D']	[ "A001_dataset_2_9837b67d5b6bb6d165d965fb5730dee9.png" ]	mcq	astronomy	en
A001/0003	<image> What is the structure of galaxy in the image?	[ "(A) Round Smooth Galaxies", "(B) Edge-on Galaxies with Bulge", "(C) Barred Spiral Galaxies", "(D) Unbarred Loose Spiral Galaxies" ]	['A']	[ "A001_dataset_3_ccd11fee72e431318f758b1c8756ef4e.png" ]	mcq	astronomy	en
A001/0004	<image> What is the structure of galaxy in the image?	[ "(A) Unbarred Tight Spiral Galaxies", "(B) Barred Spiral Galaxies", "(C) Round Smooth Galaxies", "(D) Cigar Shaped Smooth Galaxies" ]	['D']	[ "A001_dataset_4_ea3d15a6fc3e7dd6fabbe4f60f841127.png" ]	mcq	astronomy	en
A001/0005	<image> What is the structure of galaxy in the image?	[ "(A) Unbarred Tight Spiral Galaxies", "(B) Unbarred Loose Spiral Galaxies", "(C) Cigar Shaped Smooth Galaxies", "(D) Edge-on Galaxies with out Bulge" ]	['D']	[ "A001_dataset_5_163427ca59b676014e89eaa9c64f684f.png" ]	mcq	astronomy	en
A001/0006	<image> What is the structure of galaxy in the image?	[ "(A) Unbarred Tight Spiral Galaxies", "(B) Barred Spiral Galaxies", "(C) Disturbed Galaxies", "(D) Edge-on Galaxies with out Bulge" ]	['D']	[ "A001_dataset_6_6885419d4ef7e86f47091b6a79afb1dd.png" ]	mcq	astronomy	en
A001/0007	<image> What is the structure of galaxy in the image?	[ "(A) Unbarred Loose Spiral Galaxies", "(B) Round Smooth Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Edge-on Galaxies with out Bulge" ]	['D']	[ "A001_dataset_7_d258afa725d591c6edd843fb6b834278.png" ]	mcq	astronomy	en
A001/0008	<image> What is the structure of galaxy in the image?	[ "(A) Edge-on Galaxies with out Bulge", "(B) Cigar Shaped Smooth Galaxies", "(C) Round Smooth Galaxies", "(D) Edge-on Galaxies with Bulge" ]	['D']	[ "A001_dataset_8_0dcdb9b5a1352059499015dfcb90afb8.png" ]	mcq	astronomy	en
A001/0009	<image> What is the structure of galaxy in the image?	[ "(A) Unbarred Loose Spiral Galaxies", "(B) Barred Spiral Galaxies", "(C) In-between Round Smooth Galaxies", "(D) Edge-on Galaxies with Bulge" ]	['D']	[ "A001_dataset_9_ee8f21d5a03b3b0b5cfc019866e5e7c0.png" ]	mcq	astronomy	en
A001/0010	<image> What is the structure of galaxy in the image?	[ "(A) Merging Galaxies", "(B) Unbarred Loose Spiral Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Disturbed Galaxies" ]	['C']	[ "A001_dataset_10_3adebc477c62c8560bf5eb605b9e5037.png" ]	mcq	astronomy	en
A001/0011	<image> What is the structure of galaxy in the image?	[ "(A) In-between Round Smooth Galaxies", "(B) Merging Galaxies", "(C) Disturbed Galaxies", "(D) Unbarred Tight Spiral Galaxies" ]	['B']	[ "A001_dataset_11_67cab37114278d28ad9492ccff2775e0.png" ]	mcq	astronomy	en
A001/0012	<image> What is the structure of galaxy in the image?	[ "(A) Unbarred Loose Spiral Galaxies", "(B) Disturbed Galaxies", "(C) Cigar Shaped Smooth Galaxies", "(D) Merging Galaxies" ]	['C']	[ "A001_dataset_12_ece6b6179264cc800415b682f8419653.png" ]	mcq	astronomy	en
A001/0013	<image> What is the structure of galaxy in the image?	[ "(A) Barred Spiral Galaxies", "(B) In-between Round Smooth Galaxies", "(C) Merging Galaxies", "(D) Unbarred Tight Spiral Galaxies" ]	['A']	[ "A001_dataset_13_00f351ae2845d64ac4f6596a0505bb2f.png" ]	mcq	astronomy	en
A001/0014	<image> What is the structure of galaxy in the image?	[ "(A) Merging Galaxies", "(B) Edge-on Galaxies with out Bulge", "(C) Round Smooth Galaxies", "(D) Unbarred Loose Spiral Galaxies" ]	['D']	[ "A001_dataset_14_e07436726b00a785d097a0279817b4b0.png" ]	mcq	astronomy	en
A001/0015	<image> What is the structure of galaxy in the image?	[ "(A) Edge-on Galaxies with Bulge", "(B) Unbarred Loose Spiral Galaxies", "(C) Cigar Shaped Smooth Galaxies", "(D) Barred Spiral Galaxies" ]	['A']	[ "A001_dataset_15_ccfd326230ce1b1e9abebf703d2522c9.png" ]	mcq	astronomy	en
A001/0016	<image> What is the structure of galaxy in the image?	[ "(A) Disturbed Galaxies", "(B) Edge-on Galaxies with out Bulge", "(C) Cigar Shaped Smooth Galaxies", "(D) Barred Spiral Galaxies" ]	['D']	[ "A001_dataset_16_3bc1dd666997645a61a917f8dbda3017.png" ]	mcq	astronomy	en
A001/0017	<image> What is the structure of galaxy in the image?	[ "(A) Disturbed Galaxies", "(B) Barred Spiral Galaxies", "(C) Edge-on Galaxies with out Bulge", "(D) Merging Galaxies" ]	['A']	[ "A001_dataset_17_1911656e88f98c86713b510605242c92.png" ]	mcq	astronomy	en
A001/0018	<image> What is the structure of galaxy in the image?	[ "(A) In-between Round Smooth Galaxies", "(B) Edge-on Galaxies with out Bulge", "(C) Round Smooth Galaxies", "(D) Unbarred Loose Spiral Galaxies" ]	['C']	[ "A001_dataset_18_2786217b2e038ed9414ba5fa93b7bf23.png" ]	mcq	astronomy	en
A001/0019	<image> What is the structure of galaxy in the image?	[ "(A) Merging Galaxies", "(B) Round Smooth Galaxies", "(C) Disturbed Galaxies", "(D) Barred Spiral Galaxies" ]	['B']	[ "A001_dataset_19_10f64a65d627c8da0e0bedd9af5d23ef.png" ]	mcq	astronomy	en
A003/0000	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) M-dwarf", "(B) AGN", "(C) TDE", "(D) Microlens-Single" ]	['B']	[ "A003_dataset_4_48f5e42b2d682027b578388f1b536a25.png" ]	mcq	astronomy	en
A003/0001	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) EB", "(B) KN", "(C) SNII", "(D) SNIbc" ]	['C']	[ "A003_dataset_5_dc0bc08678fa8a6d5a7d6002c234f8e8.png" ]	mcq	astronomy	en
A003/0002	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) Microlens-Single", "(B) SLSN-I", "(C) SNIa", "(D) TDE" ]	['C']	[ "A003_dataset_6_fc969a40835cc54fef619132416d5dcc.png" ]	mcq	astronomy	en
A003/0003	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) Microlens-Single", "(B) AGN", "(C) SNIa-91bg", "(D) M-dwarf" ]	['B']	[ "A003_dataset_9_5d1fdc06aba98ff1c92be0a8584dbebc.png" ]	mcq	astronomy	en
A003/0004	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) EB", "(B) SNIax", "(C) KN", "(D) SLSN-I" ]	['D']	[ "A003_dataset_10_27c59fda5c97c5a9e5bb0e1eca759ea7.png" ]	mcq	astronomy	en
A003/0005	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) EB", "(B) AGN", "(C) KN", "(D) SNIa" ]	['B']	[ "A003_dataset_11_67493d72167d98e037d041242542e1e3.png" ]	mcq	astronomy	en
A003/0006	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) RRL", "(B) Mira", "(C) AGN", "(D) SNII" ]	['D']	[ "A003_dataset_12_cfa9dfda2b9520989508a5112aa89967.png" ]	mcq	astronomy	en
A003/0007	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) Microlens-Single", "(B) KN", "(C) SNIax", "(D) SNIbc" ]	['D']	[ "A003_dataset_13_a0a646bb1ca52dfb0ee1c6be86b73a9b.png" ]	mcq	astronomy	en
A003/0008	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SNIa", "(B) AGN", "(C) M-dwarf", "(D) SNII" ]	['D']	[ "A003_dataset_14_0646f136a69567b40d873cc72f7b2f7a.png" ]	mcq	astronomy	en
A003/0009	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SNIbc", "(B) RRL", "(C) KN", "(D) SNIa" ]	['A']	[ "A003_dataset_15_0b8b7eee862b6a64dc2f657733ce89fc.png" ]	mcq	astronomy	en
A003/0010	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) TDE", "(B) RRL", "(C) AGN", "(D) KN" ]	['A']	[ "A003_dataset_16_25191be39a03d9e6994e1ac6c29a12de.png" ]	mcq	astronomy	en
A003/0011	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SNIax", "(B) Mira", "(C) SNIa", "(D) KN" ]	['A']	[ "A003_dataset_18_f92f09a3e9c25cabd575ea929a930e41.png" ]	mcq	astronomy	en
A003/0012	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SNIa", "(B) TDE", "(C) Mira", "(D) SLSN-I" ]	['A']	[ "A003_dataset_20_706fbede16d7d82b3f08c6b1b9fd92da.png" ]	mcq	astronomy	en
A003/0013	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SLSN-I", "(B) SNIa", "(C) AGN", "(D) SNIbc" ]	['B']	[ "A003_dataset_24_5f095bba037123a27bf978f250b1c9e9.png" ]	mcq	astronomy	en
A003/0014	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SNIax", "(B) TDE", "(C) M-dwarf", "(D) SNIa" ]	['D']	[ "A003_dataset_26_6273ea7a1fbdac5d242f4cd99add4a1e.png" ]	mcq	astronomy	en
A003/0015	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) SNIbc", "(B) SLSN-I", "(C) SNII", "(D) TDE" ]	['C']	[ "A003_dataset_27_5f335328169496c62bfedd363ced78d7.png" ]	mcq	astronomy	en
A003/0016	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) Mira", "(B) EB", "(C) SNII", "(D) TDE" ]	['D']	[ "A003_dataset_28_e448bee4885b5ceb60dcaef7b8ad5c54.png" ]	mcq	astronomy	en
A003/0017	<image> Based on the provided images of different bands, what type of light curve is it?	[ "(A) TDE", "(B) SLSN-I", "(C) SNIax", "(D) SNIbc" ]	['D']	[ "A003_dataset_29_f1b04b2b89676432e7ea572aba3da44f.png" ]	mcq	astronomy	en
A011/0000	<image> <image> <image> The first image is the latest reference image, the second image is the historical reference image, and the third image shows the difference between the two. Please determine whether a transient event has occurred based on these three images.	[ "(A) Yes, a transient event has occurred.", "(B) No, a transient event has not occurred.", "(C) I don't know." ]	['B']	[ "A011_dataset_science_0_a00218cf037507137ade01427a689a47.png", "A011_dataset_reference_0_5d0b2c5a3ecc2abeecdd07ebab1a6634.png", "A011_dataset_difference_0_65552eb33dc2908a7f519c8cd08c6c50.png" ]	mcq	astronomy	en
A011/0001	<image> <image> <image> The first image is the latest reference image, the second image is the historical reference image, and the third image shows the difference between the two. Please determine whether a transient event has occurred based on these three images.	[ "(A) Yes, a transient event has occurred.", "(B) No, a transient event has not occurred.", "(C) I don't know." ]	['B']	[ "A011_dataset_science_1_511e2ad823af07454a5665d75405bd84.png", "A011_dataset_reference_1_898bc5caf6b38992d43ae5ca79d41e33.png", "A011_dataset_difference_1_81bdb299628d386c2196c6944b16021b.png" ]	mcq	astronomy	en

A009/0000

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.12627530097961426

[ "A009_dataset_0_ed03e981d759eec86cddd74b25587d14.png" ]

exact_match

astronomy

en

A009/0001

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

-0.003634300082921982

[ "A009_dataset_1_50826daea38941bbe699ac0bb3913148.png" ]

exact_match

astronomy

en

A009/0002

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.09097830206155777

[ "A009_dataset_2_a73c1adadbedc614c4f75a8d36d13014.png" ]

exact_match

astronomy

en

A009/0003

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.04309830069541931

[ "A009_dataset_3_75af86379235b439bbf4bc672d833e9a.png" ]

exact_match

astronomy

en

A009/0004

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.1657153069972992

[ "A009_dataset_4_87c27c010f2d30099c2049d0bb3422ed.png" ]

exact_match

astronomy

en

A009/0005

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.01240879949182272

[ "A009_dataset_5_6989de41d1fc4afb6057008cb9888947.png" ]

exact_match

astronomy

en

A009/0006

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

-0.019711699336767197

[ "A009_dataset_6_3b5de29489297138881515152422737a.png" ]

exact_match

astronomy

en

A009/0007

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.07547600567340851

[ "A009_dataset_7_cf4119bbf6760156370989c891bca499.png" ]

exact_match

astronomy

en

A009/0008

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

-0.05262269824743271

[ "A009_dataset_8_c94dbc12e17a10eece0ef1b3c5198f9e.png" ]

exact_match

astronomy

en

A009/0009

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

-0.04264570027589798

[ "A009_dataset_9_f66e52ce06c2c38376abdf5ec5cdb736.png" ]

exact_match

astronomy

en

A009/0010

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.09061399847269058

[ "A009_dataset_10_09692d1fe9cc96b02a9cf96dadc7ca52.png" ]

exact_match

astronomy

en

A009/0011

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.05570400133728981

[ "A009_dataset_11_5c9a6c649cdd21a3bc31c8c05ebd1ce4.png" ]

exact_match

astronomy

en

A009/0012

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.10715000331401825

[ "A009_dataset_12_e42b3e948d97d6c0ca9a62395ae8ddec.png" ]

exact_match

astronomy

en

A009/0013

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.03361229971051216

[ "A009_dataset_13_320ddaf07d4e769e3b0e61d147aa9a80.png" ]

exact_match

astronomy

en

A009/0014

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.08316600322723389

[ "A009_dataset_14_e8584fe473fcc39328f8313c3863ae6b.png" ]

exact_match

astronomy

en

A009/0015

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.08924499899148941

[ "A009_dataset_15_155143b17860a020a31e51491f5bec9e.png" ]

exact_match

astronomy

en

A009/0016

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.027879400178790092

[ "A009_dataset_16_524a660ec08db43ba46b734a79e3466a.png" ]

exact_match

astronomy

en

A009/0017

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.03957600146532059

[ "A009_dataset_17_9a889f7c8fc65fc3ea31dfe4076c519d.png" ]

exact_match

astronomy

en

A009/0018

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.08698400110006332

[ "A009_dataset_18_8795c19633fdf5d5d3a52900521a5626.png" ]

exact_match

astronomy

en

A009/0019

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated overall alpha abundance ([alpha/M]) of the stellar based on the spectrum?You only need to response a float value.

[]

0.025318801403045654

[ "A009_dataset_19_ae6c1f66e68793b8a5a7b30fccdce2d4.png" ]

exact_match

astronomy

en

A006/0000

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5402.044921875

[ "A006_dataset_0_ed03e981d759eec86cddd74b25587d14.png" ]

exact_match

astronomy

en

A006/0001

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5645.55419921875

[ "A006_dataset_1_50826daea38941bbe699ac0bb3913148.png" ]

exact_match

astronomy

en

A006/0002

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5501.77294921875

[ "A006_dataset_2_a73c1adadbedc614c4f75a8d36d13014.png" ]

exact_match

astronomy

en

A006/0003

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5740.89892578125

[ "A006_dataset_3_75af86379235b439bbf4bc672d833e9a.png" ]

exact_match

astronomy

en

A006/0004

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5555.275390625

[ "A006_dataset_4_87c27c010f2d30099c2049d0bb3422ed.png" ]

exact_match

astronomy

en

A006/0005

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5945.7509765625

[ "A006_dataset_5_6989de41d1fc4afb6057008cb9888947.png" ]

exact_match

astronomy

en

A006/0006

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4784.11669921875

[ "A006_dataset_6_3b5de29489297138881515152422737a.png" ]

exact_match

astronomy

en

A006/0007

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4914.67529296875

[ "A006_dataset_7_cf4119bbf6760156370989c891bca499.png" ]

exact_match

astronomy

en

A006/0008

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

3767.69384765625

[ "A006_dataset_8_c94dbc12e17a10eece0ef1b3c5198f9e.png" ]

exact_match

astronomy

en

A006/0009

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

6185.44384765625

[ "A006_dataset_9_f66e52ce06c2c38376abdf5ec5cdb736.png" ]

exact_match

astronomy

en

A006/0010

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4742.7451171875

[ "A006_dataset_10_09692d1fe9cc96b02a9cf96dadc7ca52.png" ]

exact_match

astronomy

en

A006/0011

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5031.263671875

[ "A006_dataset_11_5c9a6c649cdd21a3bc31c8c05ebd1ce4.png" ]

exact_match

astronomy

en

A006/0012

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4974.60107421875

[ "A006_dataset_12_e42b3e948d97d6c0ca9a62395ae8ddec.png" ]

exact_match

astronomy

en

A006/0013

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5049.7685546875

[ "A006_dataset_13_320ddaf07d4e769e3b0e61d147aa9a80.png" ]

exact_match

astronomy

en

A006/0014

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4975.68896484375

[ "A006_dataset_14_e8584fe473fcc39328f8313c3863ae6b.png" ]

exact_match

astronomy

en

A006/0015

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4918.45166015625

[ "A006_dataset_15_155143b17860a020a31e51491f5bec9e.png" ]

exact_match

astronomy

en

A006/0016

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4892.9208984375

[ "A006_dataset_16_524a660ec08db43ba46b734a79e3466a.png" ]

exact_match

astronomy

en

A006/0017

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

4659.77734375

[ "A006_dataset_17_9a889f7c8fc65fc3ea31dfe4076c519d.png" ]

exact_match

astronomy

en

A006/0018

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

5049.44482421875

[ "A006_dataset_18_8795c19633fdf5d5d3a52900521a5626.png" ]

exact_match

astronomy

en

A006/0019

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated effective temperature(Teff, in Kelvin) of the stellar based on the spectrum?You only need to response a float value.

[]

3990.48583984375

[ "A006_dataset_19_ae6c1f66e68793b8a5a7b30fccdce2d4.png" ]

exact_match

astronomy

en

A007/0000

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.417627334594727

[ "A007_dataset_0_ed03e981d759eec86cddd74b25587d14.png" ]

exact_match

astronomy

en

A007/0001

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.1094794273376465

[ "A007_dataset_1_50826daea38941bbe699ac0bb3913148.png" ]

exact_match

astronomy

en

A007/0002

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.304114818572998

[ "A007_dataset_2_a73c1adadbedc614c4f75a8d36d13014.png" ]

exact_match

astronomy

en

A007/0003

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.4836273193359375

[ "A007_dataset_3_75af86379235b439bbf4bc672d833e9a.png" ]

exact_match

astronomy

en

A007/0004

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.271500110626221

[ "A007_dataset_4_87c27c010f2d30099c2049d0bb3422ed.png" ]

exact_match

astronomy

en

A007/0005

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.123192310333252

[ "A007_dataset_5_6989de41d1fc4afb6057008cb9888947.png" ]

exact_match

astronomy

en

A007/0006

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.536657333374023

[ "A007_dataset_6_3b5de29489297138881515152422737a.png" ]

exact_match

astronomy

en

A007/0007

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

3.3005595207214355

[ "A007_dataset_7_cf4119bbf6760156370989c891bca499.png" ]

exact_match

astronomy

en

A007/0008

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.6511921882629395

[ "A007_dataset_8_c94dbc12e17a10eece0ef1b3c5198f9e.png" ]

exact_match

astronomy

en

A007/0009

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

4.346240997314453

[ "A007_dataset_9_f66e52ce06c2c38376abdf5ec5cdb736.png" ]

exact_match

astronomy

en

A007/0010

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

3.25662899017334

[ "A007_dataset_10_09692d1fe9cc96b02a9cf96dadc7ca52.png" ]

exact_match

astronomy

en

A007/0011

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

3.456131935119629

[ "A007_dataset_11_5c9a6c649cdd21a3bc31c8c05ebd1ce4.png" ]

exact_match

astronomy

en

A007/0012

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

2.3882505893707275

[ "A007_dataset_12_e42b3e948d97d6c0ca9a62395ae8ddec.png" ]

exact_match

astronomy

en

A007/0013

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

3.2916665077209473

[ "A007_dataset_13_320ddaf07d4e769e3b0e61d147aa9a80.png" ]

exact_match

astronomy

en

A007/0014

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

2.4835898876190186

[ "A007_dataset_14_e8584fe473fcc39328f8313c3863ae6b.png" ]

exact_match

astronomy

en

A007/0015

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

2.4800865650177

[ "A007_dataset_15_155143b17860a020a31e51491f5bec9e.png" ]

exact_match

astronomy

en

A007/0016

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

2.6240267753601074

[ "A007_dataset_16_524a660ec08db43ba46b734a79e3466a.png" ]

exact_match

astronomy

en

A007/0017

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

2.384700059890747

[ "A007_dataset_17_9a889f7c8fc65fc3ea31dfe4076c519d.png" ]

exact_match

astronomy

en

A007/0018

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

2.447835922241211

[ "A007_dataset_18_8795c19633fdf5d5d3a52900521a5626.png" ]

exact_match

astronomy

en

A007/0019

<image> The image provided is a spectrum of a stellarX-axis represents wavelength in Angstroms (Å), and the Y-axis represents flux. The red spots indicate the Line Spread Function SigmaWhat is the estimated surface gravity (log g) of the stellar based on the spectrum?You only need to response a float value.

[]

1.1980178356170654

[ "A007_dataset_19_ae6c1f66e68793b8a5a7b30fccdce2d4.png" ]

exact_match

astronomy

en

A001/0000

<image> What is the structure of galaxy in the image?

[ "(A) Disturbed Galaxies", "(B) Merging Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Edge-on Galaxies with out Bulge" ]

['A']

[ "A001_dataset_0_c48e56e5a0a10c36c26fd9237ce84d99.png" ]

mcq

astronomy

en

A001/0001

<image> What is the structure of galaxy in the image?

[ "(A) Edge-on Galaxies with Bulge", "(B) In-between Round Smooth Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Merging Galaxies" ]

['D']

[ "A001_dataset_1_2a6880a64e11c8a34108c9bbcc91477b.png" ]

mcq

astronomy

en

A001/0002

<image> What is the structure of galaxy in the image?

[ "(A) Edge-on Galaxies with out Bulge", "(B) Round Smooth Galaxies", "(C) In-between Round Smooth Galaxies", "(D) Merging Galaxies" ]

['D']

[ "A001_dataset_2_9837b67d5b6bb6d165d965fb5730dee9.png" ]

mcq

astronomy

en

A001/0003

<image> What is the structure of galaxy in the image?

[ "(A) Round Smooth Galaxies", "(B) Edge-on Galaxies with Bulge", "(C) Barred Spiral Galaxies", "(D) Unbarred Loose Spiral Galaxies" ]

['A']

[ "A001_dataset_3_ccd11fee72e431318f758b1c8756ef4e.png" ]

mcq

astronomy

en

A001/0004

<image> What is the structure of galaxy in the image?

[ "(A) Unbarred Tight Spiral Galaxies", "(B) Barred Spiral Galaxies", "(C) Round Smooth Galaxies", "(D) Cigar Shaped Smooth Galaxies" ]

['D']

[ "A001_dataset_4_ea3d15a6fc3e7dd6fabbe4f60f841127.png" ]

mcq

astronomy

en

A001/0005

<image> What is the structure of galaxy in the image?

[ "(A) Unbarred Tight Spiral Galaxies", "(B) Unbarred Loose Spiral Galaxies", "(C) Cigar Shaped Smooth Galaxies", "(D) Edge-on Galaxies with out Bulge" ]

['D']

[ "A001_dataset_5_163427ca59b676014e89eaa9c64f684f.png" ]

mcq

astronomy

en

A001/0006

<image> What is the structure of galaxy in the image?

[ "(A) Unbarred Tight Spiral Galaxies", "(B) Barred Spiral Galaxies", "(C) Disturbed Galaxies", "(D) Edge-on Galaxies with out Bulge" ]

['D']

[ "A001_dataset_6_6885419d4ef7e86f47091b6a79afb1dd.png" ]

mcq

astronomy

en

A001/0007

<image> What is the structure of galaxy in the image?

[ "(A) Unbarred Loose Spiral Galaxies", "(B) Round Smooth Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Edge-on Galaxies with out Bulge" ]

['D']

[ "A001_dataset_7_d258afa725d591c6edd843fb6b834278.png" ]

mcq

astronomy

en

A001/0008

<image> What is the structure of galaxy in the image?

[ "(A) Edge-on Galaxies with out Bulge", "(B) Cigar Shaped Smooth Galaxies", "(C) Round Smooth Galaxies", "(D) Edge-on Galaxies with Bulge" ]

['D']

[ "A001_dataset_8_0dcdb9b5a1352059499015dfcb90afb8.png" ]

mcq

astronomy

en

A001/0009

<image> What is the structure of galaxy in the image?

[ "(A) Unbarred Loose Spiral Galaxies", "(B) Barred Spiral Galaxies", "(C) In-between Round Smooth Galaxies", "(D) Edge-on Galaxies with Bulge" ]

['D']

[ "A001_dataset_9_ee8f21d5a03b3b0b5cfc019866e5e7c0.png" ]

mcq

astronomy

en

A001/0010

<image> What is the structure of galaxy in the image?

[ "(A) Merging Galaxies", "(B) Unbarred Loose Spiral Galaxies", "(C) Unbarred Tight Spiral Galaxies", "(D) Disturbed Galaxies" ]

['C']

[ "A001_dataset_10_3adebc477c62c8560bf5eb605b9e5037.png" ]

mcq

astronomy

en

A001/0011

<image> What is the structure of galaxy in the image?

[ "(A) In-between Round Smooth Galaxies", "(B) Merging Galaxies", "(C) Disturbed Galaxies", "(D) Unbarred Tight Spiral Galaxies" ]

['B']

[ "A001_dataset_11_67cab37114278d28ad9492ccff2775e0.png" ]

mcq

astronomy

en

A001/0012

<image> What is the structure of galaxy in the image?

[ "(A) Unbarred Loose Spiral Galaxies", "(B) Disturbed Galaxies", "(C) Cigar Shaped Smooth Galaxies", "(D) Merging Galaxies" ]

['C']

[ "A001_dataset_12_ece6b6179264cc800415b682f8419653.png" ]

mcq

astronomy

en

A001/0013

<image> What is the structure of galaxy in the image?

[ "(A) Barred Spiral Galaxies", "(B) In-between Round Smooth Galaxies", "(C) Merging Galaxies", "(D) Unbarred Tight Spiral Galaxies" ]

['A']

[ "A001_dataset_13_00f351ae2845d64ac4f6596a0505bb2f.png" ]

mcq

astronomy

en

A001/0014

<image> What is the structure of galaxy in the image?

[ "(A) Merging Galaxies", "(B) Edge-on Galaxies with out Bulge", "(C) Round Smooth Galaxies", "(D) Unbarred Loose Spiral Galaxies" ]

['D']

[ "A001_dataset_14_e07436726b00a785d097a0279817b4b0.png" ]

mcq

astronomy

en

A001/0015

<image> What is the structure of galaxy in the image?

[ "(A) Edge-on Galaxies with Bulge", "(B) Unbarred Loose Spiral Galaxies", "(C) Cigar Shaped Smooth Galaxies", "(D) Barred Spiral Galaxies" ]

['A']

[ "A001_dataset_15_ccfd326230ce1b1e9abebf703d2522c9.png" ]

mcq

astronomy

en

A001/0016

<image> What is the structure of galaxy in the image?

[ "(A) Disturbed Galaxies", "(B) Edge-on Galaxies with out Bulge", "(C) Cigar Shaped Smooth Galaxies", "(D) Barred Spiral Galaxies" ]

['D']

[ "A001_dataset_16_3bc1dd666997645a61a917f8dbda3017.png" ]

mcq

astronomy

en

A001/0017

<image> What is the structure of galaxy in the image?

[ "(A) Disturbed Galaxies", "(B) Barred Spiral Galaxies", "(C) Edge-on Galaxies with out Bulge", "(D) Merging Galaxies" ]

['A']

[ "A001_dataset_17_1911656e88f98c86713b510605242c92.png" ]

mcq

astronomy

en

A001/0018

<image> What is the structure of galaxy in the image?

[ "(A) In-between Round Smooth Galaxies", "(B) Edge-on Galaxies with out Bulge", "(C) Round Smooth Galaxies", "(D) Unbarred Loose Spiral Galaxies" ]

['C']

[ "A001_dataset_18_2786217b2e038ed9414ba5fa93b7bf23.png" ]

mcq

astronomy

en

A001/0019

<image> What is the structure of galaxy in the image?

[ "(A) Merging Galaxies", "(B) Round Smooth Galaxies", "(C) Disturbed Galaxies", "(D) Barred Spiral Galaxies" ]

['B']

[ "A001_dataset_19_10f64a65d627c8da0e0bedd9af5d23ef.png" ]

mcq

astronomy

en

A003/0000

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) M-dwarf", "(B) AGN", "(C) TDE", "(D) Microlens-Single" ]

['B']

[ "A003_dataset_4_48f5e42b2d682027b578388f1b536a25.png" ]

mcq

astronomy

en

A003/0001

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) EB", "(B) KN", "(C) SNII", "(D) SNIbc" ]

['C']

[ "A003_dataset_5_dc0bc08678fa8a6d5a7d6002c234f8e8.png" ]

mcq

astronomy

en

A003/0002

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) Microlens-Single", "(B) SLSN-I", "(C) SNIa", "(D) TDE" ]

['C']

[ "A003_dataset_6_fc969a40835cc54fef619132416d5dcc.png" ]

mcq

astronomy

en

A003/0003

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) Microlens-Single", "(B) AGN", "(C) SNIa-91bg", "(D) M-dwarf" ]

['B']

[ "A003_dataset_9_5d1fdc06aba98ff1c92be0a8584dbebc.png" ]

mcq

astronomy

en

A003/0004

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) EB", "(B) SNIax", "(C) KN", "(D) SLSN-I" ]

['D']

[ "A003_dataset_10_27c59fda5c97c5a9e5bb0e1eca759ea7.png" ]

mcq

astronomy

en

A003/0005

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) EB", "(B) AGN", "(C) KN", "(D) SNIa" ]

['B']

[ "A003_dataset_11_67493d72167d98e037d041242542e1e3.png" ]

mcq

astronomy

en

A003/0006

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) RRL", "(B) Mira", "(C) AGN", "(D) SNII" ]

['D']

[ "A003_dataset_12_cfa9dfda2b9520989508a5112aa89967.png" ]

mcq

astronomy

en

A003/0007

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) Microlens-Single", "(B) KN", "(C) SNIax", "(D) SNIbc" ]

['D']

[ "A003_dataset_13_a0a646bb1ca52dfb0ee1c6be86b73a9b.png" ]

mcq

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A003/0008

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SNIa", "(B) AGN", "(C) M-dwarf", "(D) SNII" ]

['D']

[ "A003_dataset_14_0646f136a69567b40d873cc72f7b2f7a.png" ]

mcq

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A003/0009

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SNIbc", "(B) RRL", "(C) KN", "(D) SNIa" ]

['A']

[ "A003_dataset_15_0b8b7eee862b6a64dc2f657733ce89fc.png" ]

mcq

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A003/0010

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) TDE", "(B) RRL", "(C) AGN", "(D) KN" ]

['A']

[ "A003_dataset_16_25191be39a03d9e6994e1ac6c29a12de.png" ]

mcq

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A003/0011

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SNIax", "(B) Mira", "(C) SNIa", "(D) KN" ]

['A']

[ "A003_dataset_18_f92f09a3e9c25cabd575ea929a930e41.png" ]

mcq

astronomy

en

A003/0012

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SNIa", "(B) TDE", "(C) Mira", "(D) SLSN-I" ]

['A']

[ "A003_dataset_20_706fbede16d7d82b3f08c6b1b9fd92da.png" ]

mcq

astronomy

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A003/0013

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SLSN-I", "(B) SNIa", "(C) AGN", "(D) SNIbc" ]

['B']

[ "A003_dataset_24_5f095bba037123a27bf978f250b1c9e9.png" ]

mcq

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A003/0014

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SNIax", "(B) TDE", "(C) M-dwarf", "(D) SNIa" ]

['D']

[ "A003_dataset_26_6273ea7a1fbdac5d242f4cd99add4a1e.png" ]

mcq

astronomy

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A003/0015

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) SNIbc", "(B) SLSN-I", "(C) SNII", "(D) TDE" ]

['C']

[ "A003_dataset_27_5f335328169496c62bfedd363ced78d7.png" ]

mcq

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A003/0016

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) Mira", "(B) EB", "(C) SNII", "(D) TDE" ]

['D']

[ "A003_dataset_28_e448bee4885b5ceb60dcaef7b8ad5c54.png" ]

mcq

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A003/0017

<image> Based on the provided images of different bands, what type of light curve is it?

[ "(A) TDE", "(B) SLSN-I", "(C) SNIax", "(D) SNIbc" ]

['D']

[ "A003_dataset_29_f1b04b2b89676432e7ea572aba3da44f.png" ]

mcq

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A011/0000

<image> <image> <image> The first image is the latest reference image, the second image is the historical reference image, and the third image shows the difference between the two. Please determine whether a transient event has occurred based on these three images.

[ "(A) Yes, a transient event has occurred.", "(B) No, a transient event has not occurred.", "(C) I don't know." ]

['B']

[ "A011_dataset_science_0_a00218cf037507137ade01427a689a47.png", "A011_dataset_reference_0_5d0b2c5a3ecc2abeecdd07ebab1a6634.png", "A011_dataset_difference_0_65552eb33dc2908a7f519c8cd08c6c50.png" ]

mcq

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A011/0001

<image> <image> <image> The first image is the latest reference image, the second image is the historical reference image, and the third image shows the difference between the two. Please determine whether a transient event has occurred based on these three images.

[ "(A) Yes, a transient event has occurred.", "(B) No, a transient event has not occurred.", "(C) I don't know." ]

['B']

[ "A011_dataset_science_1_511e2ad823af07454a5665d75405bd84.png", "A011_dataset_reference_1_898bc5caf6b38992d43ae5ca79d41e33.png", "A011_dataset_difference_1_81bdb299628d386c2196c6944b16021b.png" ]

mcq

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en