Datasets:
Dataset Viewer
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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_3e0e51d486cb924a24d49b9bc0b17ea1.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_1a0c79dc8ee01a32a0812bdfdffe7443.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_4e93ee8d72d0d5fb01cde0e9f6985e3f.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_4c612fecd3acc4f8e04fa250bccd7b6b.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_511b7c3662a627cbb3ec9da36ee2cb5d.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_10cc995c6c739e56408fb8dcf1068803.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_edd450e0bcf2cb8b36865ae8725cafbc.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_fd48716e37fe2669496a83e1a03d755b.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_0b8ecf873222111f0d5b51116fa5752a.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_bef333b0797fed49685fa5e702243d5d.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_a21b52f8e32a38ba6eb426fe4eac1c84.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_0cba02b03c9eee02fdd2c99d52453dd6.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_2d3fc49ae82c059f43b9e4fb1ffa8ca3.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_13e34fe8f2a2776a00a98949d92e803d.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_e865409928830710946cf9ef7fd9eb5f.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_1fe3df89c0826f64dc0a0f64ac994c4d.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_7df9f93822b18d494f5071065cd5e521.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_b4068e6e2b67451b2ef7d11872dff56a.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_0a254185f1fb901f98c31fc59c3345dc.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_35c76a094de12be4ef74ba229f4d2d58.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_3e0e51d486cb924a24d49b9bc0b17ea1.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_1a0c79dc8ee01a32a0812bdfdffe7443.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_4e93ee8d72d0d5fb01cde0e9f6985e3f.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_4c612fecd3acc4f8e04fa250bccd7b6b.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_511b7c3662a627cbb3ec9da36ee2cb5d.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_10cc995c6c739e56408fb8dcf1068803.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_edd450e0bcf2cb8b36865ae8725cafbc.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_fd48716e37fe2669496a83e1a03d755b.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_0b8ecf873222111f0d5b51116fa5752a.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_bef333b0797fed49685fa5e702243d5d.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_a21b52f8e32a38ba6eb426fe4eac1c84.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_0cba02b03c9eee02fdd2c99d52453dd6.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_2d3fc49ae82c059f43b9e4fb1ffa8ca3.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_13e34fe8f2a2776a00a98949d92e803d.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_e865409928830710946cf9ef7fd9eb5f.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_1fe3df89c0826f64dc0a0f64ac994c4d.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_7df9f93822b18d494f5071065cd5e521.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_b4068e6e2b67451b2ef7d11872dff56a.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_0a254185f1fb901f98c31fc59c3345dc.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_35c76a094de12be4ef74ba229f4d2d58.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_3e0e51d486cb924a24d49b9bc0b17ea1.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_1a0c79dc8ee01a32a0812bdfdffe7443.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_4e93ee8d72d0d5fb01cde0e9f6985e3f.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_4c612fecd3acc4f8e04fa250bccd7b6b.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_511b7c3662a627cbb3ec9da36ee2cb5d.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_10cc995c6c739e56408fb8dcf1068803.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_edd450e0bcf2cb8b36865ae8725cafbc.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_fd48716e37fe2669496a83e1a03d755b.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_0b8ecf873222111f0d5b51116fa5752a.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_bef333b0797fed49685fa5e702243d5d.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_a21b52f8e32a38ba6eb426fe4eac1c84.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_0cba02b03c9eee02fdd2c99d52453dd6.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_2d3fc49ae82c059f43b9e4fb1ffa8ca3.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_13e34fe8f2a2776a00a98949d92e803d.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_e865409928830710946cf9ef7fd9eb5f.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_1fe3df89c0826f64dc0a0f64ac994c4d.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_7df9f93822b18d494f5071065cd5e521.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_b4068e6e2b67451b2ef7d11872dff56a.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_0a254185f1fb901f98c31fc59c3345dc.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_35c76a094de12be4ef74ba229f4d2d58.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 |
End of preview. Expand
in Data Studio
Scientists' First Exam
Scientific discoveries are driven by complex multimodal reasoning based on information-intensive scientific data and domain-specific expertise. With supervision from expert-level scientific benchmarks, scientific multimodal Large Language Models (MLLMs) could significantly enhance this discovery process in realistic workflows. However, current scientific benchmarks current scientific benchmarks inadequately assess MLLMs’ perception, understanding, and reasoning skills necessary for scientific breakthroughs across multiple disciplines. To address this gap, we present the Scientists’ First Example (SFE) benchmark, designed to comprehensively evaluate the scientific cognitive capacities of MLLMs through three interconnected levels: \textit{scientific signal perception}, \textit{scientific attribute understanding}, \textit{scientific comparative reasoning}. Specifically, SFE comprises 839 expert-verified MQA/VQA pairs spanning 66 multimodal tasks across five high-value disciplines. Extensive experimental results reveal that current \textit{state-of-the-art} GPT-4.1 and InternVL-2.5 achieve only 30.8% and 24.43% on SFE, highlighting a significant room for MLLMs to improve in scientific realms. We hope insights obtained in SFE could facilitate further developments in AI-enhanced scientific discoveries.
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