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Record W6903676610 · doi:10.13016/m274p4-w4fw

Multiwavelength Investigation of ?-ray Source MGRO J1908+06 Emission Using Fermi--LAT, VERITAS, and HAWC

2024· article· en· W6903676610 on OpenAlexfundno aff

Bibliographic record

VenueMaryland Shared Open Access Repository (USMAI Consortium) · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesCoordinación de la Investigación CientíficaLos Alamos National LaboratoryGoddard Space Flight CenterOffice of ScienceOffice of National Higher Education Science Research and Innovation Policy CouncilIstituto Nazionale di Fisica NucleareHigh Energy Accelerator Research OrganizationJapan Aerospace Exploration AgencyBenemérita Universidad Autónoma de PueblaInstitute for Cosmic Ray Research, University of TokyoCentre National de la Recherche ScientifiqueU.S. Department of EnergySmithsonian InstitutionVetenskapsrådetAgenzia Spaziale ItalianaGeneralitat ValencianaNational Energy Research Scientific Computing CenterLaboratory Directed Research and DevelopmentNational Science FoundationDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoIstituto Nazionale di AstrofisicaNatural Sciences and Engineering Research Council of CanadaBarnard CollegeMinistry of Education, Culture, Sports, Science and TechnologyNational Aeronautics and Space AdministrationUniversities Space Research AssociationConsejo Nacional de Ciencia y Tecnología
KeywordsPulsarBroadbandMagnetic fieldEmission spectrumNebulaSpectral shape analysisSpectral lineSpectral properties

Abstract

fetched live from OpenAlex

This paper investigates the origin of the ?-ray emission from MGRO J1908+06 in the GeV-TeV energy band. By analyzing the data collected by {\it Fermi}--LAT, VERITAS, and HAWC, with the addition of spectral data previously reported by LHAASO, a multiwavelength (MW) study of the morphological and spectral features of MGRO J1908+06 provides insight into the origin of the ?-ray emission. The mechanism behind the bright TeV emission is studied by constraining the magnetic field strength, the source age, and the distance through detailed broadband modeling. Both spectral shape and energy-dependent morphology support the scenario that inverse-Compton (IC) emission of an evolved pulsar wind nebula (PWN) associated with PSR J1907+0602 is responsible for the MGRO J1908+06 ?-ray emission with a best-fit true age of T=22±9 kyr and a magnetic field of B=5.4±0.8 ?G, assuming the distance to the pulsar dPSR=3.2 kpc.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow), Scholarly communication
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.377
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0020.001
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.033
GPT teacher head0.304
Teacher spread0.271 · 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 teacher head, not a consensus.

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

Citations0
Published2024
Admission routes1
Has abstractyes

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