Detecting and characterizing pulsar haloes with the Cherenkov telescope array

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90247%2F23%3A00604384" target="_blank" >RIV/68378271:90247/23:00604384 - isvavai.cz</a>

Výsledek na webu

<a href="https://hdl.handle.net/11104/0361780" target="_blank" >https://hdl.handle.net/11104/0361780</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1093/mnras/stad715" target="_blank" >10.1093/mnras/stad715</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Detecting and characterizing pulsar haloes with the Cherenkov telescope array

Popis výsledku v původním jazyce

The recently identified source class of pulsar haloes may be numerous and bright enough in the TeV energy range to constitute a large fraction of the sources that will be observed with the Cherenkov Telescope Array (CTA). In this work, we quantify the prospects for detecting and characterizing pulsar haloes in observations of the projected Galactic Plane Survey (GPS), using a simple phenomenological diffusion model for individual pulsar haloes and their population in the Milky Way. Our ability to uncover pulsar haloes and constrain their main physical parameters in the CTA GPS is assessed in the framework of a full spatial-spectral likelihood analysis of simulated survey observations, using the most recent estimates for the instrument response function and prototypes for the science tools.

Název v anglickém jazyce

Detecting and characterizing pulsar haloes with the Cherenkov telescope array

Popis výsledku anglicky

The recently identified source class of pulsar haloes may be numerous and bright enough in the TeV energy range to constitute a large fraction of the sources that will be observed with the Cherenkov Telescope Array (CTA). In this work, we quantify the prospects for detecting and characterizing pulsar haloes in observations of the projected Galactic Plane Survey (GPS), using a simple phenomenological diffusion model for individual pulsar haloes and their population in the Milky Way. Our ability to uncover pulsar haloes and constrain their main physical parameters in the CTA GPS is assessed in the framework of a full spatial-spectral likelihood analysis of simulated survey observations, using the most recent estimates for the instrument response function and prototypes for the science tools.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2023

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

e-ISSN

1365-2966

Svazek periodika

521

Číslo periodika v rámci svazku

3

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

17

Strana od-do

3793-3809

Kód UT WoS článku

000961016300029

EID výsledku v databázi Scopus

2-s2.0-85160329445