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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 |
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