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Record W7082099986

Combined dark matter search towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS

2025· article· en· W7082099986 on OpenAlexfundno aff

Bibliographic record

VenueDesy Publications Database (Deutsches Elektronen-Synchrotron DESY) · 2025
Typearticle
Languageen
FieldComputer Science
TopicGeochemistry and Geologic Mapping
Canadian institutionsnot available
FundersLos Alamos National LaboratoryLaboratory Directed Research and DevelopmentInstitute for Cosmic Ray Research, University of TokyoInstituto de Astrofísica de CanariasOffice of ScienceOffice of National Higher Education Science Research and Innovation Policy CouncilDeutsche ForschungsgemeinschaftBundesministerium für Bildung, Wissenschaft und ForschungNational Commission on Research, Science and TechnologyJapan Society for the Promotion of ScienceJapan Aerospace Exploration AgencyBenemérita Universidad Autónoma de PueblaMinistry of Education, Culture, Sports, Science and TechnologyBundesministerium für Bildung und ForschungNatural Sciences and Engineering Research Council of CanadaIstituto Nazionale di AstrofisicaEuropean Regional Development FundMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroInstitut National de Physique Nucléaire et de Physique des ParticulesSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungScience and Technology Facilities CouncilHigh Energy Accelerator Research OrganizationHrvatska Zaklada za ZnanostCoordinación de la Investigación CientíficaNational Research Foundation of KoreaConselho Nacional de Desenvolvimento Científico e TecnológicoDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoConsejo Nacional de Ciencia y TecnologíaNational Research FoundationAustrian Science FundIstituto Nazionale di Fisica NucleareGeneralitat de CatalunyaIrish Research CouncilUniversiteit van AmsterdamAgencia Estatal de InvestigaciónUniversity of NamibiaCentres de Recerca de CatalunyaVetenskapsrådetSmithsonian InstitutionEuropean CommissionNational Science FoundationScience Foundation IrelandAgenzia Spaziale ItalianaNational Energy Research Scientific Computing CenterKnut och Alice Wallenbergs StiftelseAlexander von Humboldt-StiftungNational Aeronautics and Space Administration
KeywordsCherenkov radiationDark matterGalaxyDwarf spheroidal galaxyDwarf galaxyAnnihilation
DOInot available

Abstract

fetched live from OpenAlex

Dwarf spheroidal galaxies (dSphs) are excellent targets for indirect dark matter (DM) searches using gamma-ray telescopes because they are thought to have high DM content and a low astrophysical background. The sensitivity of these searches is improved by combining the observations of dSphs made by different gamma-ray telescopes. We present the results of a combined search by the most sensitive currently operating gamma-ray telescopes, namely: the satellite-borne Fermi-LAT telescope; the ground-based imaging atmospheric Cherenkov telescope arrays H.E.S.S., MAGIC, and VERITAS; and the HAWC water Cherenkov detector. Individual datasets were analyzed using a common statistical approach. Results were subsequently combined via a global joint likelihood analysis. We obtain constraints on the velocity-weighted cross section 〈σv〉 for DM self-annihilation as a function of the DM particle mass. This five-instrument combination allows the derivation of up to 2-3 times more constraining upper limits on 〈σv〉 than the individual results over a wide mass range spanning from 5 GeV to 100 TeV. Depending on the DM content modeling, the 95% confidence level observed limits reach 1.5×10<sup>-24</sup> cm<sup>3</sup>s<sup>-1</sup> and 3.2×10<sup>-25</sup> cm<sup>3</sup>s<sup>-1</sup>, respectively, in the τ<sup>+</sup>τ<sup>-</sup> annihilation channel for a DM mass of 2 TeV.

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)0.001
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: none
Teacher disagreement score0.641
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.002
Science and technology studies0.0010.001
Scholarly communication0.0010.002
Open science0.0020.001
Research integrity0.0000.001
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 head0.017
GPT teacher head0.247
Teacher spread0.229 · 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
Published2025
Admission routes1
Has abstractyes

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