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Soft gamma-ray polarimetry with COSI using maximum likelihood analysis

Soft gamma-ray polarimetry with COSI using maximum likelihood analysis

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2646838405

Soft gamma-ray polarimetry with COSI using maximum likelihood analysis

About this item

Full title

Soft gamma-ray polarimetry with COSI using maximum likelihood analysis

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2022-03

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Measurements of the linear polarization of high-energy emission from pulsars, accreting black holes, and gamma-ray bursts (GRBs) provide an opportunity for constraining the emission mechanisms and geometries (e.g., of the accretion disk, jet, magnetic field, etc.) in the sources. For photons in the soft (MeV) gamma-ray band, Compton scattering is t...

Alternative Titles

Full title

Soft gamma-ray polarimetry with COSI using maximum likelihood analysis

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2646838405

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2646838405

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2204.00027

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