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Record W4318071668 · doi:10.1038/s41550-022-01874-x

Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries

2023· article· en· W4318071668 on OpenAlexfundno aff
C. J. Clark, M. Kerr, E D Barr, Bhaswati Bhattacharyya, R. P. Breton, P. Bruel, F. Camilo, W Chen, I. Cognard, H. Thankful Cromartie, J. S. Deneva, V. S. Dhillon, L. Guillemot, Mark Kennedy, A. G. Lyne, D. Mata Sánchez, L. Nieder, Camryn L. Phillips, S. M. Ransom, Paul S. Ray, M. S. Roberts, Jayanta Roy, D. A. Smith, R. Spiewak, B. W. Stappers, S. Tabassum, G. Theureau, Guillaume Voisin

Bibliographic record

VenueNature Astronomy · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersU.S. Naval Research LaboratoryIstituto Nazionale di Fisica NucleareNational Research FoundationHigh Energy Accelerator Research OrganizationIstituto Nazionale di AstrofisicaScience and Technology Facilities CouncilInstitut National de Physique Nucléaire et de Physique des ParticulesNational Radio Astronomy ObservatoryU.S. Department of EnergyVetenskapsrådetMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueMinistry of Education, Culture, Sports, Science and TechnologyDepartment of Atomic Energy, Government of IndiaEuropean Regional Development FundJapan Aerospace Exploration AgencyEuropean CommissionCanadian Institute for Advanced ResearchNational Aeronautics and Space AdministrationOffice of Naval ResearchIrish Research CouncilAssociated UniversitiesSpace Telescope Science InstituteAgenzia Spaziale ItalianaNational Science Foundation
KeywordsMillisecond pulsarPhysicsPulsarAstrophysicsNeutron starPulsar planetLight curveAstronomyFermi Gamma-ray Space TelescopeEclipseBinary pulsarX-ray pulsar

Abstract

fetched live from OpenAlex

Reliable neutron star mass measurements are key to determining the equation of state of cold nuclear matter, but such measurements are rare. Black widows and redbacks are compact binaries consisting of millisecond pulsars and semi-degenerate companion stars. Spectroscopy of the optically bright companions can determine their radial velocities, providing inclination-dependent pulsar mass estimates. Although inclinations can be inferred from subtle features in optical light curves, such estimates may be systematically biased due to incomplete heating models and poorly understood variability. Using data from the Fermi Large Area Telescope, we have searched for gamma-ray eclipses from 49 spider systems, discovering significant eclipses in 7 systems, including the prototypical black widow PSR B1957+20. Gamma-ray eclipses require direct occultation of the pulsar by the companion, and so the detection, or significant exclusion, of a gamma-ray eclipse strictly limits the binary inclination angle, providing new robust, model-independent pulsar mass constraints. For PSR B1957+20, the eclipse implies a much lighter pulsar (1.81 ± 0.07 solar masses) than inferred from optical light curve modelling.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.002
Threshold uncertainty score0.003

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.010
GPT teacher head0.311
Teacher spread0.301 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations36
Published2023
Admission routes1
Has abstractyes

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