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M003/0003 | Given a lattice‑diagram view of the material, infer the molecular formula based solely on the lattice composition and reply only with that formula (e.g., Ag₂O), without any additional text, explanation, or commentary.
Based on the provided lattice diagram <image>, determine the molecular formula of the material | []
| BaTe | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M003_mp-1000-lattice_22ca7af2a555dc7ff38b0450eff626ce.png"
]
| exact_match | material | en |
M003/0004 | Given a lattice‑diagram view of the material, infer the molecular formula based solely on the lattice composition and reply only with that formula (e.g., Ag₂O), without any additional text, explanation, or commentary.
Based on the provided lattice diagram <image>, determine the molecular formula of the material | []
| BP | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M003_mp-1479-lattice_f67c4c96d8ac8d427de225b514f0aa90.png"
]
| exact_match | material | en |
M003/0005 | Given a lattice‑diagram view of the material, infer the molecular formula based solely on the lattice composition and reply only with that formula (e.g., Ag₂O), without any additional text, explanation, or commentary.
Based on the provided lattice diagram <image>, determine the molecular formula of the material | []
| AgF₂ | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M003_mp-2284-lattice_4619b60520f5850d3a1d388de3137a36.png"
]
| exact_match | material | en |
M003/0006 | Given a lattice‑diagram view of the material, infer the molecular formula based solely on the lattice composition and reply only with that formula (e.g., Ag₂O), without any additional text, explanation, or commentary.
Based on the provided lattice diagram <image>, determine the molecular formula of the material | []
| Al₃Ir | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M003_mp-2294-lattice_b8bf8ca2d894259a634e8f6162558cba.png"
]
| exact_match | material | en |
M003/0007 | Given a lattice‑diagram view of the material, infer the molecular formula based solely on the lattice composition and reply only with that formula (e.g., Ag₂O), without any additional text, explanation, or commentary.
Based on the provided lattice diagram <image>, determine the molecular formula of the material | []
| BAs | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M003_mp-10044-lattice_b9bb0a27e9db926f840e96748c119d1f.png"
]
| exact_match | material | en |
M010/0000 | Given an electronic band structure plot, analyze the positions of the valence band maximum (VBM) and conduction band minimum (CBM) to decide if the material has a direct bandgap (VBM and CBM at the same high‑symmetry k‑point, which you must specify), an indirect bandgap (VBM and CBM at different high‑symmetry k‑points, which you must specify both), or if band crossings at the Fermi level indicate a metallic state with no bandgap. Reply with a single concise narrative paragraph stating your conclusion, including the relevant high‑symmetry k‑points for direct or indirect cases, or for a metallic case briefly explaining that band crossings preclude any bandgap, without bullet points, lists, or additional commentary.
Based on the provided band structure <image>, determine whether the material exhibits a direct or indirect bandgap | []
| The material is metallic, doesn't exhibit a direct or indirect bandgap | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M010_mp-353-eb-dos_d3b46e6f5f5ff5c47e19d880400a9950.png"
]
| open_ended | material | en |
M010/0001 | Given an electronic band structure plot, analyze the positions of the valence band maximum (VBM) and conduction band minimum (CBM) to decide if the material has a direct bandgap (VBM and CBM at the same high‑symmetry k‑point, which you must specify), an indirect bandgap (VBM and CBM at different high‑symmetry k‑points, which you must specify both), or if band crossings at the Fermi level indicate a metallic state with no bandgap. Reply with a single concise narrative paragraph stating your conclusion, including the relevant high‑symmetry k‑points for direct or indirect cases, or for a metallic case briefly explaining that band crossings preclude any bandgap, without bullet points, lists, or additional commentary.
Based on the provided band structure <image>, determine whether the material exhibits a direct or indirect bandgap | []
| VBM and CBM are located at same k-points, the material exhibits direct bandgap | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M010_mp-661-eb-dos_c365e50f098b63e2b525c4ec418979ee.png"
]
| open_ended | material | en |
M010/0002 | Given an electronic band structure plot, analyze the positions of the valence band maximum (VBM) and conduction band minimum (CBM) to decide if the material has a direct bandgap (VBM and CBM at the same high‑symmetry k‑point, which you must specify), an indirect bandgap (VBM and CBM at different high‑symmetry k‑points, which you must specify both), or if band crossings at the Fermi level indicate a metallic state with no bandgap. Reply with a single concise narrative paragraph stating your conclusion, including the relevant high‑symmetry k‑points for direct or indirect cases, or for a metallic case briefly explaining that band crossings preclude any bandgap, without bullet points, lists, or additional commentary.
Based on the provided band structure <image>, determine whether the material exhibits a direct or indirect bandgap | []
| VBM and CBM are located at same k-points, the material exhibits direct bandgap | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M010_mp-856-eb-dos_2e41504acab43542fe6f99032876ec60.png"
]
| open_ended | material | en |
M010/0003 | Given an electronic band structure plot, analyze the positions of the valence band maximum (VBM) and conduction band minimum (CBM) to decide if the material has a direct bandgap (VBM and CBM at the same high‑symmetry k‑point, which you must specify), an indirect bandgap (VBM and CBM at different high‑symmetry k‑points, which you must specify both), or if band crossings at the Fermi level indicate a metallic state with no bandgap. Reply with a single concise narrative paragraph stating your conclusion, including the relevant high‑symmetry k‑points for direct or indirect cases, or for a metallic case briefly explaining that band crossings preclude any bandgap, without bullet points, lists, or additional commentary.
Based on the provided band structure <image>, determine whether the material exhibits a direct or indirect bandgap | []
| VBM (Γ) and CBM (X) are located at different k-points, the material exhibits indirect bandgap | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M010_mp-1000-eb-dos_78a6f549803f8501ccb6da02ef6c0003.png"
]
| open_ended | material | en |
M021/0000 | Given an XRD pattern of a single‑phase material, identify the crystalline phase, assign the obvious primary diffraction peaks to their Miller indices (hkl), calculate the lattice parameters from those peak positions, and reply with a single concise narrative paragraph integrating these findings and calculations, without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please identify the crystalline phase(s) present, assign Miller indices (hkl) to the distinct primary diffraction peaks (note that, you only need to specify the obvious peaks), and use those peak positions to estimate the lattice parameters. | []
| The main diffraction peaks at 2θ = 26.5°, 32.6°, 37.8°, 54.6°, 65.1°, 68.4°, 80.9° and 90.0° correspond exactly to the (110), (111), (200), (220), (311), (222), (400) and (331) reflections of Ag₂O (Space group Pn3̅m). No impurity phase is found in the XRD pattern. The calculated lattice parameters are: a = b = c = 4.75Å, α = β = γ = 90°. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M021_mp-353-xrd_d5b5f4f9302869ae0b1d65b0eac06311.png"
]
| open_ended | material | en |
M021/0001 | Given an XRD pattern of a single‑phase material, identify the crystalline phase, assign the obvious primary diffraction peaks to their Miller indices (hkl), calculate the lattice parameters from those peak positions, and reply with a single concise narrative paragraph integrating these findings and calculations, without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please identify the crystalline phase(s) present, assign Miller indices (hkl) to the distinct primary diffraction peaks (note that, you only need to specify the obvious peaks), and use those peak positions to estimate the lattice parameters. | []
| The main diffraction peaks at 2θ = 26.5°, 33.7°, 38.8°, 51.5°, 54.5°, 62.2°, 65.6°, 70.8°, 78.2° and 89.2° correspond exactly to the (110), (101), (111), (211), (220), (221), (301), (202), (321) and (312) reflections of SnO₂ (Space group P4₂/mnm). No impurity phase is found in the XRD pattern. The calculated lattice parameters are: a = b = 4.76Å, c = 3.21Å, α = β = γ = 90°. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M021_mp-856-xrd_740c7f3fb5b2e5b34fb129235364accc.png"
]
| open_ended | material | en |
M021/0002 | Given an XRD pattern of a single‑phase material, identify the crystalline phase, assign the obvious primary diffraction peaks to their Miller indices (hkl), calculate the lattice parameters from those peak positions, and reply with a single concise narrative paragraph integrating these findings and calculations, without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please identify the crystalline phase(s) present, assign Miller indices (hkl) to the distinct primary diffraction peaks (note that, you only need to specify the obvious peaks), and use those peak positions to estimate the lattice parameters. | []
| The main diffraction peaks at 2θ = 25.1°, 35.8°, 44.3°, 51.6°, 58.2°, 64.4°, 75.9°, 81.4° and 86.9° correspond exactly to the (200), (220), (222), (400), (420), (422), (440), (600) and (620) reflections of BaTe (Space group Fm3̅m). No impurity phase is found in the XRD pattern. The calculated lattice parameters are: a = b = c = 7.09Å, α = β = γ = 90°. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M021_mp-1000-xrd_edffd3779425795e159be6498f6c76f7.png"
]
| open_ended | material | en |
M021/0003 | Given an XRD pattern of a single‑phase material, identify the crystalline phase, assign the obvious primary diffraction peaks to their Miller indices (hkl), calculate the lattice parameters from those peak positions, and reply with a single concise narrative paragraph integrating these findings and calculations, without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please identify the crystalline phase(s) present, assign Miller indices (hkl) to the distinct primary diffraction peaks (note that, you only need to specify the obvious peaks), and use those peak positions to estimate the lattice parameters. | []
| The main diffraction peaks at 2θ = 34.3°, 39.8°, 57.5°, 68.7°, 72.2° and 85.8° correspond exactly to the (111), (200), (220), (311), (222) and (400) reflections of BP (Space group F4̅3m). No impurity phase is found in the XRD pattern. The calculated lattice parameters are: a = b = c = 4.53Å, α = β = γ = 90°. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M021_mp-1479-xrd_760b62663aba060337dada1fa4c1183e.png"
]
| open_ended | material | en |
M022/0000 | Given an XRD pattern of a material with a clearly defined most intense peak, apply the Scherrer equation to that peak to calculate the average crystallite size and reply with a single concise narrative paragraph stating the result and key parameters used (e.g., peak position, peak intensity), without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please estimate the average crystallite size of the sample by applying the Scherrer equation to the most intense XRD peak. | []
| Applying the Scherrer formula to the most intense (111) peak, the calculated average crystallite size is 0.1nm | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M022_mp-353-xrd_d5b5f4f9302869ae0b1d65b0eac06311.png"
]
| open_ended | material | en |
M022/0001 | Given an XRD pattern of a material with a clearly defined most intense peak, apply the Scherrer equation to that peak to calculate the average crystallite size and reply with a single concise narrative paragraph stating the result and key parameters used (e.g., peak position, peak intensity), without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please estimate the average crystallite size of the sample by applying the Scherrer equation to the most intense XRD peak. | []
| Applying the Scherrer formula to the most intense (110) peak, the calculated average crystallite size is 0.1nm | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M022_mp-856-xrd_740c7f3fb5b2e5b34fb129235364accc.png"
]
| open_ended | material | en |
M022/0002 | Given an XRD pattern of a material with a clearly defined most intense peak, apply the Scherrer equation to that peak to calculate the average crystallite size and reply with a single concise narrative paragraph stating the result and key parameters used (e.g., peak position, peak intensity), without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please estimate the average crystallite size of the sample by applying the Scherrer equation to the most intense XRD peak. | []
| Applying the Scherrer formula to the most intense (200) peak, the calculated average crystallite size is 0.1nm | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M022_mp-1000-xrd_edffd3779425795e159be6498f6c76f7.png"
]
| open_ended | material | en |
M022/0003 | Given an XRD pattern of a material with a clearly defined most intense peak, apply the Scherrer equation to that peak to calculate the average crystallite size and reply with a single concise narrative paragraph stating the result and key parameters used (e.g., peak position, peak intensity), without bullet points, lists, or additional commentary.
Based on the provided XRD pattern <image>, please estimate the average crystallite size of the sample by applying the Scherrer equation to the most intense XRD peak. | []
| Applying the Scherrer formula to the most intense (111) peak, the calculated average crystallite size is 0.1nm | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M022_mp-1479-xrd_760b62663aba060337dada1fa4c1183e.png"
]
| open_ended | material | en |
M008/0000 | Based on the given band structure and DOS <image>, is the material metallic or semiconducting? What could be concluded more from the graph? | []
| The material is metallic (bands cross the Fermi level). Electronic states near the Fermi level dominated by Ag atoms. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M008_mp-353-eb-dos_d3b46e6f5f5ff5c47e19d880400a9950.png"
]
| open_ended | material | en |
M008/0001 | Given an electronic band structure plot alongside its DOS, assess whether band crossings at the Fermi level indicate a metallic state or a semiconducting gap; then inspect the DOS near the Fermi level to identify which atomic or orbital contributions dominate and mention any other notable features. Reply with a single concise narrative paragraph stating your conclusions—no bullet points, lists, or additional commentary.
Based on the given band structure and DOS <image>, is the material metallic or semiconducting? What could be concluded more from the graph? | []
| The material is wide bandgap semiconductor (with bandgap about 4 meV). N-2p domimated the valence band states, while N and Al atoms together dominate the conduction band states. VBM and CBM located at the same high-symmetry points, indicating AlN a direct bandgap materials. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M008_mp-661-eb-dos_c365e50f098b63e2b525c4ec418979ee.png"
]
| open_ended | material | en |
M008/0002 | Based on the given band structure and DOS <image>, is the material metallic or semiconducting? What could be concluded more from the graph? | []
| The material has a bandgap of 0.65 meV, exhibiting direct bandgap (VBM and CBM located at same high symmetry point) | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M008_mp-856-eb-dos_2e41504acab43542fe6f99032876ec60.png"
]
| open_ended | material | en |
M008/0003 | Based on the given band structure and DOS <image>, is the material metallic or semiconducting? What could be concluded more from the graph? | []
| The material is semicondutor, with a bandgap of about 1.59eV. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M008_mp-1000-eb-dos_78a6f549803f8501ccb6da02ef6c0003.png"
]
| open_ended | material | en |
M020/0000 | Given a combined XRD pattern and several materials' individual XRD patterns, analyze the set of diffraction peaks to determine which crystalline phases are present and provide a concise narrative explanation of your reasoning in a single paragraph, avoiding bullet points, lists, or any additional commentary.
Based on the XRD pattern of the composite material made from a mixture of three materials <image> and five XRD patterns of Ag₂O <image>, SnO₂ <image>, BaTe <image>, BAs <image> and Ac₂CuIr <image> (orderly), identify all three phases/materials present in the composite material. | []
| This graph contains three distinct materials: Ag₂O, BaTe, and Ac₂CuIr. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000_mp-353_mp-861883-xrd_5c6fc7e1c24c1308cec88760f725173c.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-353-xrd_d5b5f4f9302869ae0b1d65b0eac06311.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-856-xrd_740c7f3fb5b2e5b34fb129235364accc.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000-xrd_edffd3779425795e159be6498f6c76f7.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-10044-xrd_58e3f5f29cd97b0f4353b05be40fc20b.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-861883-xrd_f3c095b7ddb13ea75c0648e2fbf4e5cf.png"
]
| exact_match | material | en |
M020/0001 | Given a combined XRD pattern and several materials' individual XRD patterns, analyze the set of diffraction peaks to determine which crystalline phases are present and provide a concise narrative explanation of your reasoning in a single paragraph, avoiding bullet points, lists, or any additional commentary.
Based on the XRD pattern of the composite material made from a mixture of three materials <image> and five XRD patterns of AlN <image>, SnO₂ <image>, BaTe <image>, BP <image> and Ac₂CuGe <image> (orderly), identify all three phases/materials present in the composite material. | []
| This graph contains three distinct materials: AlN, BaTe and Ac₂CuGe. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000_mp-661_mp-862786-xrd_cde7995f078c81c9eb82d6a1c4990c5d.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-661-xrd_334bdf3d5484d6511fb76db6d9250b14.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-856-xrd_740c7f3fb5b2e5b34fb129235364accc.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000-xrd_edffd3779425795e159be6498f6c76f7.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1479-xrd_760b62663aba060337dada1fa4c1183e.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-862786-xrd_869dde84a5b0cab5b7cbdf72bc6121e4.png"
]
| exact_match | material | en |
M020/0002 | Given a combined XRD pattern and several materials' individual XRD patterns, analyze the set of diffraction peaks to determine which crystalline phases are present and provide a concise narrative explanation of your reasoning in a single paragraph, avoiding bullet points, lists, or any additional commentary.
Based on the XRD pattern of the composite material made from a mixture of three materials <image> and five XRD patterns of BaTe <image>, YSF <image>, Al₂Ru <image>, FeO <image>, AgBr <image> (orderly), identify all three phases/materials present in the composite material. | []
| This graph contains three distinct materials: YSF, BaTe and AgBr. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000_mp-10086_mp-23231-xrd_9a151dbecfe7e3bb3b9ebc54a4b0ec07.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000-xrd_edffd3779425795e159be6498f6c76f7.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-10086-xrd_40963c9a5cbf6178e739ef3c03390698.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-10910-xrd_7e9e6a2ef2ffcc8314a135a692980021.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-18905-xrd_ddc80c9ef19ba31424611c5d89e4acec.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-23231-xrd_d99310c8259bac533325a8eb29c0d378.png"
]
| exact_match | material | en |
M020/0003 | Given a combined XRD pattern and several materials' individual XRD patterns, analyze the set of diffraction peaks to determine which crystalline phases are present and provide a concise narrative explanation of your reasoning in a single paragraph, avoiding bullet points, lists, or any additional commentary.
Based on the XRD pattern of the composite material made from a mixture of three materials <image> and five XRD patterns of AlN <image>, BaTe <image>, Al₃Ir <image>, AcOF <image>, Ac₂CuIr <image> (orderly), identify all three phases/materials present in the composite material. | []
| This graph contains three distinct materials: Al₃Ir, AcOF and Ac₂CuIr. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-2294_mp-36526_mp-861883-xrd_68fee02439b291163b7c4e0671bc9acc.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-661-xrd_334bdf3d5484d6511fb76db6d9250b14.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-1000-xrd_edffd3779425795e159be6498f6c76f7.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-2294-xrd_cac10131ae8adfb0e22f1f129287ee38.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-36526-xrd_9abc52260e67a99194d670f94513ef26.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-861883-xrd_f3c095b7ddb13ea75c0648e2fbf4e5cf.png"
]
| exact_match | material | en |
M020/0004 | Given a combined XRD pattern and several materials' individual XRD patterns, analyze the set of diffraction peaks to determine which crystalline phases are present and provide a concise narrative explanation of your reasoning in a single paragraph, avoiding bullet points, lists, or any additional commentary.
Based on the XRD pattern of the composite material made from a mixture of three materials <image> and five XRD patterns of Ag₂O <image>, AlN <image>, BAs <image>, YSF <image> and AcOF <image>, identify all three phases/materials present in the composite material. | []
| This graph contains three distinct materials: Ag₂O, BAs and YSF. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-10044_mp-10086_mp-353-xrd_e63a8e6798424b68ecffecf681d53ff2.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-353-xrd_d5b5f4f9302869ae0b1d65b0eac06311.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-661-xrd_334bdf3d5484d6511fb76db6d9250b14.png",
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"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-10086-xrd_40963c9a5cbf6178e739ef3c03390698.png",
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M020_mp-36526-xrd_9abc52260e67a99194d670f94513ef26.png"
]
| exact_match | material | en |
M018/0000 | Given the XPS spectrum of the sample, analyze the spectral features to determine which elements and compounds are present and assign their core‑level peaks (including any satellite or oxidation‑state‑specific signatures), and reply with a single descriptive paragraph that mirrors the example style—no bullet points, lists, or additional commentary.
Based on the provided XPS spectra <image>, please specify all the element species and identify the characteristic peaks. If multiple materials are present, analyze and assign the peaks for each materials. | []
| Co metal shows sharp 2p₃/₂ and 2p₁/₂ peaks at 778.1 eV and 793.1 eV, without noticeable satellites.
CoO (Co²⁺) features its 2p₃/₂ main peak at ~780.0 eV and a shake-up satellite at ~786.5 eV; the 2p₁/₂ appears at ~795.0 eV with a satellite near 802.5 eV.
Co(OH)₂ shifts the Co²⁺ 2p₃/₂ to ~781.0 eV, but retains a similar satellite structure.
Co₃O₄ contains both Co³⁺ and Co²⁺ : Co³⁺ 2p₃/₂ at ~779.6 eV, Co²⁺ 2p₃/₂ at ~780.0 eV, and corresponding satellites around 786 eV, with 2p₁/₂ features near 794.5–795.0 eV. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M018_Cobalt_figure_ae409f50f55be1bcca7da9f109fc239d.jpg"
]
| open_ended | material | en |
M018/0001 | Given the XPS spectrum of the sample, analyze the spectral features to determine which elements and compounds are present and assign their core‑level peaks (including any satellite or oxidation‑state‑specific signatures), and reply with a single descriptive paragraph that mirrors the example style—no bullet points, lists, or additional commentary.
Based on the provided XPS spectra <image>, please specify the element species and identify the characteristic peaks. If multiple materials are present, analyze and assign the peaks for each materials. | []
| The depicted XPS spectrum showed Ir 4f₇/₂ and 4f₅/₂ peaks, with a binding energy of 60.59 eV and 63.59 eV respectively. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M018_Iridium_figure2_141c5926956aedd822af39aac779c318.jpg"
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| open_ended | material | en |
M018/0002 | Given the XPS spectrum of the sample, analyze the spectral features to determine which elements and compounds are present and assign their core‑level peaks (including any satellite or oxidation‑state‑specific signatures), and reply with a single descriptive paragraph that mirrors the example style—no bullet points, lists, or additional commentary.
Based on the provided XPS spectra <image>, please specify the element species and identify the characteristic peaks. If multiple materials are present, analyze and assign the peaks for each materials. | []
| The depicted XPS spectrum showed Au 4f₇/₂ and 4f₅/₂ peaks, with a binding energy of 83.96 eV and 87.63 eV respectively. | [
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]
| open_ended | material | en |
M018/0003 | Given the XPS spectrum of the sample, analyze the spectral features to determine which elements and compounds are present and assign their core‑level peaks (including any satellite or oxidation‑state‑specific signatures), and reply with a single descriptive paragraph that mirrors the example style—no bullet points, lists, or additional commentary.
Based on the provided XPS spectra <image>, please specify the element species and identify the characteristic peaks. If multiple materials are present, analyze and assign the peaks for each materials. | []
| The depicted XPS spectrum showed Ca 2p₃/₂ and 2p₁/₂ peaks, with a binding energy of 348.29 eV and 351.83 eV respectively. | [
"/fs-computility/ai4sData/earth-shared/SFE/sfe_dataset/v0/images/M018_Calcium_figure2_bb1e74b2054dba79635f2af06ee32ad3.jpg"
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| open_ended | material | en |
A009/0000 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0001 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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A009/0002 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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A009/0003 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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A009/0004 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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A009/0005 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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A009/0006 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0007 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0008 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0009 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0010 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0011 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0012 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0013 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0014 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0015 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0016 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0017 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0018 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A009/0019 | <image> 提供的图像是恒星光谱。X轴表示波长（以埃为单位），Y轴表示光通量。红点表示线扩散函数（Line Spread Function）的西格玛（Sigma）。根据光谱，估计的恒星整体α丰度（[alpha/M]）是多少？你只需要回复一个浮点值。 | []
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| exact_match | astronomy | zh |
A006/0000 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0001 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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| exact_match | astronomy | zh |
A006/0002 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0003 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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| exact_match | astronomy | zh |
A006/0004 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0005 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0006 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0007 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0008 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0009 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0010 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0011 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0012 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0013 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0014 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0015 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0016 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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A006/0017 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
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| exact_match | astronomy | zh |
A006/0018 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
| 5049.44482421875 | [
"A006_dataset_18_0a254185f1fb901f98c31fc59c3345dc.png"
]
| exact_match | astronomy | zh |
A006/0019 | <image> 所提供的图像是恒星的光谱。X轴代表波长，以埃（Å）为单位，Y轴代表光通量。红点表示线扩展函数西格玛。基于光谱，恒星的估计有效温度（Teff，以开尔文为单位）是多少？您只需提供一个浮点值。 | []
| 3990.48583984375 | [
"A006_dataset_19_35c76a094de12be4ef74ba229f4d2d58.png"
]
| exact_match | astronomy | zh |
A007/0000 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.417627334594727 | [
"A007_dataset_0_3e0e51d486cb924a24d49b9bc0b17ea1.png"
]
| exact_match | astronomy | zh |
A007/0001 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.1094794273376465 | [
"A007_dataset_1_1a0c79dc8ee01a32a0812bdfdffe7443.png"
]
| exact_match | astronomy | zh |
A007/0002 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.304114818572998 | [
"A007_dataset_2_4e93ee8d72d0d5fb01cde0e9f6985e3f.png"
]
| exact_match | astronomy | zh |
A007/0003 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.4836273193359375 | [
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]
| exact_match | astronomy | zh |
A007/0004 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.271500110626221 | [
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]
| exact_match | astronomy | zh |
A007/0005 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.123192310333252 | [
"A007_dataset_5_10cc995c6c739e56408fb8dcf1068803.png"
]
| exact_match | astronomy | zh |
A007/0006 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.536657333374023 | [
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]
| exact_match | astronomy | zh |
A007/0007 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 3.3005595207214355 | [
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]
| exact_match | astronomy | zh |
A007/0008 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.6511921882629395 | [
"A007_dataset_8_0b8ecf873222111f0d5b51116fa5752a.png"
]
| exact_match | astronomy | zh |
A007/0009 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 4.346240997314453 | [
"A007_dataset_9_bef333b0797fed49685fa5e702243d5d.png"
]
| exact_match | astronomy | zh |
A007/0010 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 3.25662899017334 | [
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]
| exact_match | astronomy | zh |
A007/0011 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 3.456131935119629 | [
"A007_dataset_11_0cba02b03c9eee02fdd2c99d52453dd6.png"
]
| exact_match | astronomy | zh |
A007/0012 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 2.3882505893707275 | [
"A007_dataset_12_2d3fc49ae82c059f43b9e4fb1ffa8ca3.png"
]
| exact_match | astronomy | zh |
A007/0013 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 3.2916665077209473 | [
"A007_dataset_13_13e34fe8f2a2776a00a98949d92e803d.png"
]
| exact_match | astronomy | zh |
A007/0014 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 2.4835898876190186 | [
"A007_dataset_14_e865409928830710946cf9ef7fd9eb5f.png"
]
| exact_match | astronomy | zh |
A007/0015 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 2.4800865650177 | [
"A007_dataset_15_1fe3df89c0826f64dc0a0f64ac994c4d.png"
]
| exact_match | astronomy | zh |
A007/0016 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 2.6240267753601074 | [
"A007_dataset_16_7df9f93822b18d494f5071065cd5e521.png"
]
| exact_match | astronomy | zh |
A007/0017 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 2.384700059890747 | [
"A007_dataset_17_b4068e6e2b67451b2ef7d11872dff56a.png"
]
| exact_match | astronomy | zh |
A007/0018 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 2.447835922241211 | [
"A007_dataset_18_0a254185f1fb901f98c31fc59c3345dc.png"
]
| exact_match | astronomy | zh |
A007/0019 | <image> 提供的图像是恒星的光谱。X轴表示波长，单位为埃（Å），Y轴表示辐射通量。红点表示线扩展函数 Sigma。基于光谱，恒星的估计表面重力（log g）是多少？您只需回复一个浮点值。 | []
| 1.1980178356170654 | [
"A007_dataset_19_35c76a094de12be4ef74ba229f4d2d58.png"
]
| exact_match | astronomy | zh |
A001/0000 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0001 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0002 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0003 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0004 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0005 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0006 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0007 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0008 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
A001/0009 | <image> 图像中的星系结构是什么？ | [
"(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 | zh |
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