General Relativity and Quantum Cosmology · arXiv:1105.5843 v1 · submitted 30 May 2011
Multimessenger Astronomy
The paper says
“Presented here is a summary of the status of LIGO-Virgo multimessenger detection efforts, along with a discussion of questions that might be resolved using the data from advanced or third generation gravitational wave detector networks.”
from the abstract · picked out as the main claim by a classifier
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The paper
Abstract
Multimessenger astronomy incorporating gravitational radiation is a new and exciting field that will potentially provide significant results and exciting challenges in the near future. With advanced interferometric gravitational wave detectors (LCGT, LIGO, Virgo) we will have the opportunity to investigate sources of gravitational waves that are also expected to be observable through other messengers, such as electromagnetic (gamma-rays, x-rays, optical, radio) and/or neutrino emission. The LIGO-Virgo interferometer network has already been used for multimessenger searches for gravitational radiation that have produced insights on cosmic events. The simultaneous observation of electromagnetic and/or neutrino emission could be important evidence in the first direct detection of gravitational radiation. Knowledge of event time, source sky location, and the expected frequency range of the signal enhances our ability to search for the gravitational radiation signatures with an amplitude closer to the noise floor of the detector. Presented here is a summary of the status of LIGO-Virgo multimessenger detection efforts, along with a discussion of questions that might be resolved using the data from advanced or third generation gravitational wave detector networks.
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. No sentence in this record was written by a model.
abstract compiled · 2026-09-23 · no language-model review
How the main claim is stated: asserted 0.78
What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.11 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.10 · mentions code or data availability 0.02
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v1). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| Multimessenger astronomy incorporating gravitational radiation is a new and exciting field that will potentially provide significant results and exciting challenges in the near future. | background 0.99 | 0.04 | 0.12 | hedged possibility 0.64 |
| With advanced interferometric gravitational wave detectors (LCGT, LIGO, Virgo) we will have the opportunity to investigate sources of gravitational waves that are also expected to be observable through other messengers, such as electromagnetic (gamma-rays, x-rays, optical, radio) and/or neutrino emission. | background 0.84 | 0.05 | 0.05 | hedged possibility 0.85 |
| The LIGO-Virgo interferometer network has already been used for multimessenger searches for gravitational radiation that have produced insights on cosmic events. | background 0.92 | 0.22 | 0.09 | asserted 1.00 |
| The simultaneous observation of electromagnetic and/or neutrino emission could be important evidence in the first direct detection of gravitational radiation. | background 0.91 | 0.06 | 0.10 | hedged possibility 1.00 |
| Knowledge of event time, source sky location, and the expected frequency range of the signal enhances our ability to search for the gravitational radiation signatures with an amplitude closer to the noise floor of the detector. | background 0.83 | 0.08 | 0.06 | asserted 0.97 |
| Presented here is a summary of the status of LIGO-Virgo multimessenger detection efforts, along with a discussion of questions that might be resolved using the data from advanced or third generation gravitational wave detector networks. | contribution 1.00 | 0.45 | 0.18 | asserted 0.78 |
What kind of paper the classifier reports this is: review 1.00 · evidence from literature 0.79
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
Levels run
- P abstract
Not run
- S sections
- T body sentences
- C citations
- R cross-paper relations
How the labels were made
Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,058 input tokens, $0.0002 reported.
Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON
Cited by 1 Pith paper
Reviewed papers on Pith that cite this one. The full citation record
- Exploring gravity with the MIGA large scale atom interferometer physics.atom-ph · Mar 2017
How the literature uses it
6 arXiv papers cite this in 6 sentences
Papers citing it · 3 sentences without a confident label
Cites it as background 3 papers
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With the imminent direct detection of gravitational waves (GWs) by second generation detectors ( [ref] ), the pursuit of an understanding of the electromagnetic (EM) counterparts to GWs becomes urgent, as a joint observation in both channels will provide irreplaceable means to diagnose properties of the astrophysical sources ( [ref] ).
Plasma-wave generation in a dynamic spacetime · Introduction · 0.82
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The third pillar is almost ready with near future gravitational-wave observations by interferometric detectors like LIGO, Virgo, GEO600 and LCGT [ref] .
Gravitationally Driven Electromagnetic Perturbations of Neutron Stars and Black Holes · Introduction · 0.96
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Now, the worldwide projects are going on to detect gravitational waves associated with the astrophysical phenomena involving compact objects [ref] .
Shear oscillations in the hadron-quark mixed phase · Introduction · 0.98
Challenges and discussion
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