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ce-61: a Tidal Dwarf Galaxy in the Hercules cluster?

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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W. van Driel, P.-A. Duc, P. Amram, F. Bournaud, C. Balkowski, V. Cayatte, J. Dickey, H. Hernandez
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J. Iglesias-Paramo, K. O'Neil, P. Papaderos, J.M. Vilchez

Astrophysics · Submitted 22 Oct 2003

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim The multi-wavelength data we obtained so far do not prove, however, that it is kinematically detached from the IC 1182 system and gravitationally bound.

how it is stated · asserted 0.75 read the record →

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arXiv IDastro-ph/0310631 (version 1)
Pith ID3K5WQJTY, Pith's permanent record of this paper and its review
CitationC. Balkowski, F. Bournaud, H. Hernandez, J. Dickey, J. Iglesias-Paramo, J.M. Vilchez, K. O'Neil, P.-A. Duc, P. Amram, P. Papaderos, V. Cayatte, W. van Driel. "ce-61: a Tidal Dwarf Galaxy in the Hercules cluster?." arXiv:astro-ph/0310631 (2003). https://pith.science/paper/3K5WQJTY
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,311 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.97 · human participants 0.02 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.08 · mentions code or data availability 0.03.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

A candidate Tidal Dwarf Galaxy, ce-61, was identified in the merger system IC 1182 in the Hercules supercluster. The multi-wavelength data we obtained so far do not prove, however, that it is kinematically detached from the IC 1182 system and gravitationally bound.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 A candidate Tidal Dwarf Galaxy, ce-61, was identified in the merger system IC 1182 in the Hercules supercluster. result 0.55 0.73 0.11 asserted 0.73
s1 The multi-wavelength data we obtained so far do not prove, however, that it is kinematically detached from the IC 1182 system and gravitationally bound. limitation 0.99 0.91 0.60 asserted 0.75

What kind of paper the classifier reports this is: empirical study 0.98 · evidence from observation or experiment 1.00.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

A candidate Tidal Dwarf Galaxy, ce-61, was identified in the merger system IC 1182 in the Hercules supercluster. The multi-wavelength data we obtained so far do not prove, however, that it is kinematically detached from the IC 1182 system and gravitationally bound.

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