Dataset Preview
doc_ids sequence | abstracts sequence | index int64 | pearson_correlation float64 | reasoning string | label string | density float64 | f1 float64 |
|---|---|---|---|---|---|---|---|
["1607.01526","1607.03009","1607.06240","1607.07246","1607.07888","1607.08820","1607.06710","1607.08(...TRUNCATED) | ["'Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case'","'(...TRUNCATED) | null | null | null | null | null | null |
null | null | 2 | 0.66279 | "### Step 1: Identify Common Topics, Concepts, and Features in Max-Activating Examples\n\n1. **Stran(...TRUNCATED) | Strange quark matter and strange stars | 0.006939 | 0.75 |
null | null | 1 | 0.982008 | "### Step 1: Identify Potential Topics, Concepts, and Features\n\nBased on the max-activating exampl(...TRUNCATED) | Centaurs, TNOs, rings, satellites, characteristics | 0.002961 | 1 |
null | null | 4 | 0.510527 | "### Step 1: Identify Common Topics, Concepts, and Features in Max-Activating Examples\n\n1. **Impli(...TRUNCATED) | Implicit numerical methods | 0.001101 | 0.75 |
null | null | 0 | 0.724368 | "### Step 1: Identify Potential Topics, Concepts, and Features\n\nBased on the max-activating exampl(...TRUNCATED) | Triaxial models in astronomy | 0.003665 | 0.8 |
null | null | 3 | 0.967773 | "### Step 1: Identify Potential Topics, Concepts, and Features\n\nBased on the max-activating exampl(...TRUNCATED) | Cosmological observables in theoretical models | 0.006074 | 1 |
null | null | 8 | 0 | "### Step 1: Identify Potential Topics, Concepts, and Features\n\nBased on the max-activating exampl(...TRUNCATED) | Gravitational potential and energy | 0.003197 | 0.6 |
null | null | 7 | 0.186989 | "### Step 1: Identify Potential Topics, Concepts, and Features\n\nBased on the max-activating exampl(...TRUNCATED) | Barred galaxies and their dynamics | 0.004122 | 0.6 |
null | null | 6 | 0.683468 | "### Step 1: Identify Common Topics, Concepts, and Features in Max-Activating Examples\n\n1. **Comet(...TRUNCATED) | Comet C/1995 O1 (Hale-Bopp) | 0.001304 | 0.857143 |
null | null | 5 | 0.570447 | "### Step 1: Identify Potential Topics, Concepts, and Features\n\nBased on the max-activating exampl(...TRUNCATED) | Magnetic fields in β Cephei stars | 0.001042 | 0.75 |
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