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Record W4396815201 · doi:10.3204/pubdb-2025-04848

Galactic transient sources with the Cherenkov Telescope Array Observatory

2024· preprint· en· W4396815201 on OpenAlexfundno aff
Cherenkov Telescope Array Consortium

Bibliographic record

VenuearXiv (Cornell University) · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersCanadian Space AgencyBundesministerium für Bildung, Wissenschaft und ForschungAgencia Nacional de Investigación y DesarrolloIstituto Nazionale di Fisica NucleareAustralian Research CouncilMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesRegione LombardiaState Committee of ScienceUniversitetet i OsloNatural Sciences and Engineering Research Council of CanadaIstituto Nazionale di AstrofisicaMinisterio de Ciencia e InnovaciónMinistère de l'Education Nationale, de l'Enseignement Superieur et de la RechercheFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroFundação AraucáriaWestern Sydney UniversityMax-Planck-GesellschaftInstitut National de Physique Nucléaire et de Physique des ParticulesHrvatska Zaklada za ZnanostEuropean Regional Development FundMinisterstvo Školství, Mládeže a TělovýchovyBundesministerium für Bildung und ForschungAgencia Estatal de InvestigaciónUniversity of New South WalesJavna Agencija za Raziskovalno Dejavnost RSMonash UniversityFundação de Amparo à Pesquisa do Estado de São PauloJapan Society for the Promotion of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoFondazione CariploUniversity of AdelaideUniversity of SydneyInstitute for Cosmic Ray Research, University of TokyoCentre National de la Recherche ScientifiqueMinistry of Education, Culture, Sports, Science and TechnologyNederlandse Organisatie voor Wetenschappelijk OnderzoekSveučilište u ZagrebuAgence Nationale de la RechercheDeutsche ForschungsgemeinschaftMinistero dell’Istruzione, dell’Università e della RicercaNational Research Foundation
KeywordsPhysicsPulsarAstrophysicsCherenkov radiationNeutron starAstronomyTelescopeMagnetarCherenkov Telescope ArrayMillisecond pulsarNebulaObservatoryCrab NebulaStarsDetectorOptics

Abstract

fetched live from OpenAlex

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exhibiting extreme variability as magnetars as well as pulsar-wind nebulae. Although most of them can show emission up to MeV and/or GeV energies, many have not yet been detected in the TeV domain by Imaging Atmospheric Cherenkov Telescopes. In this paper, we explore the feasibility of detecting new Galactic transients with the Cherenkov Telescope Array Observatory (CTAO) and the prospects for studying them with Target of Opportunity observations. We show that CTAO will likely detect new sources in the TeV regime, such as the massive microquasars in the Cygnus region, low-mass X-ray binaries with low-viewing angle, flaring emission from the Crab pulsar-wind nebula or other novae explosions, among others. Since some of these sources could also exhibit emission at larger time-scales, we additionally test their detectability at longer exposures. We finally discuss the multiwavelength synergies with other instruments and large astronomical facilities.

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)0.001
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: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.010

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.004
Science and technology studies0.0010.000
Scholarly communication0.0020.002
Open science0.0000.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0030.001

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 head0.033
GPT teacher head0.163
Teacher spread0.130 · 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 designNot applicable
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

Citations2
Published2024
Admission routes1
Has abstractyes

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