The Arecibo Galaxy Environment Survey (AGES). XI. The expanded Abell 1367 field: Data catalogue and H I census over the surveyed volume

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00562598" target="_blank" >RIV/67985815:_____/22:00562598 - isvavai.cz</a>

Výsledek na webu

<a href="https://hdl.handle.net/11104/0335142" target="_blank" >https://hdl.handle.net/11104/0335142</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/202243103" target="_blank" >10.1051/0004-6361/202243103</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The Arecibo Galaxy Environment Survey (AGES). XI. The expanded Abell 1367 field: Data catalogue and H I census over the surveyed volume

Popis výsledku v původním jazyce

We present the results of the complete AGES survey of the A1367 field. In total, we detect 457 H I sources, 213 of which are detected for the first time by the AGES survey, and 134 of which are presented in this article for the first time. Of the 457 detections, 225 are in the cluster and 232 are in the remaining volume surveyed. Here we present the full catalogue of H I detections and their basic properties, including optical ones. We concentrate on the difference between the cluster and the foreground and background LSS, revealing a continuous correlation of H I-detected fraction (and H I deficiency) with local galaxy density, independent of global environment.

Název v anglickém jazyce

The Arecibo Galaxy Environment Survey (AGES). XI. The expanded Abell 1367 field: Data catalogue and H I census over the surveyed volume

Popis výsledku anglicky

We present the results of the complete AGES survey of the A1367 field. In total, we detect 457 H I sources, 213 of which are detected for the first time by the AGES survey, and 134 of which are presented in this article for the first time. Of the 457 detections, 225 are in the cluster and 232 are in the remaining volume surveyed. Here we present the full catalogue of H I detections and their basic properties, including optical ones. We concentrate on the difference between the cluster and the foreground and background LSS, revealing a continuous correlation of H I-detected fraction (and H I deficiency) with local galaxy density, independent of global environment.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/GA19-18647S" target="_blank" >GA19-18647S: Původ struktur temného neutrálního plynu kolem galaxií</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

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

Název periodika

Astronomy & Astrophysics

ISSN

0004-6361

e-ISSN

1432-0746

Svazek periodika

665

Číslo periodika v rámci svazku

September

Stát vydavatele periodika

FR - Francouzská republika

Počet stran výsledku

18

Strana od-do

A155

Kód UT WoS článku

000857191500010

EID výsledku v databázi Scopus

2-s2.0-85139830096