id stringlengths 9 9 | question stringclasses 137
values | options listlengths 0 15 | answer stringlengths 1 1.49k | images images listlengths 1 18 | 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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