Datasets:

etri-lirs
/

SFE

id stringlengths 9 9	question stringclasses 137 values	options listlengths 0 15	answer stringlengths 1 1.49k	question_type stringclasses 3 values	field stringclasses 5 values	lang stringclasses 1 value
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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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 val...	[]	5402.044921875	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 val...	[]	5645.55419921875	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 val...	[]	5501.77294921875	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 val...	[]	5740.89892578125	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 val...	[]	5555.275390625	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 val...	[]	5945.7509765625	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 val...	[]	4784.11669921875	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 val...	[]	4914.67529296875	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 val...	[]	3767.69384765625	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 val...	[]	6185.44384765625	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 val...	[]	4742.7451171875	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 val...	[]	5031.263671875	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 val...	[]	4974.60107421875	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 val...	[]	5049.7685546875	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 val...	[]	4975.68896484375	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 val...	[]	4918.45166015625	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 val...	[]	4892.9208984375	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 val...	[]	4659.77734375	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 val...	[]	5049.44482421875	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 val...	[]	3990.48583984375	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	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']	mcq	astronomy	en

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Repackaging Notice / 재패키징 안내 / 重新打包说明

English
This dataset is a repackaged version of the multimodal dataset InternScience/SFE, based on its 2025-06-11 release. The original content has been preserved, while all images have been embedded directly into the dataset files to simplify usage and distribution on the Hugging Face Hub.
For the original dataset description, license, and citation, please refer to the source dataset.

한국어 (Korean)
이 데이터셋은 멀티모달 데이터셋 InternScience/SFE의 2025-06-11 버전을 기반으로 재패키징한 것입니다. 원본 데이터 내용은 유지하면서, Hugging Face Hub에서의 사용 편의성을 위해 모든 이미지를 데이터셋 내부에 임베딩했습니다.
데이터셋 설명, 라이선스 및 인용 정보는 원본 데이터셋을 참고하시기 바랍니다.

中文 (Chinese)
本数据集基于多模态数据集 InternScience/SFE 的 2025-06-11 版本进行重新打包。在保持原始数据内容不变的前提下，我们将所有图像直接嵌入到数据文件中，以便在 Hugging Face Hub 上更方便地使用和分发。
有关原始数据集的描述、许可证和引用信息，请参考源数据集。

Scientists' First Exam: Probing Cognitive Abilities of MLLM via Perception, Understanding, and Reasoning

Evaluations

We use lmms-eval for evaluations. Please see here for more details.

License

SFE is released under the MIT License. See LICENSE for more details.

Reference

If you find SFE useful in your research, please consider citing the following paper:

@misc{zhou2025scientistsexamprobingcognitive,
      title={Scientists' First Exam: Probing Cognitive Abilities of MLLM via Perception, Understanding, and Reasoning}, 
      author={Yuhao Zhou and Yiheng Wang and Xuming He and Ruoyao Xiao and Zhiwei Li and Qiantai Feng and Zijie Guo and Yuejin Yang and Hao Wu and Wenxuan Huang and Jiaqi Wei and Dan Si and Xiuqi Yao and Jia Bu and Haiwen Huang and Tianfan Fu and Shixiang Tang and Ben Fei and Dongzhan Zhou and Fenghua Ling and Yan Lu and Siqi Sun and Chenhui Li and Guanjie Zheng and Jiancheng Lv and Wenlong Zhang and Lei Bai},
      year={2025},
      eprint={2506.10521},
      archivePrefix={arXiv},
      primaryClass={cs.AI},
      url={https://arxiv.org/abs/2506.10521}, 
}

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Paper for etri-lirs/SFE

Scientists' First Exam: Probing Cognitive Abilities of MLLM via Perception, Understanding, and Reasoning

Paper • 2506.10521 • Published Jun 12, 2025 • 73