Details

BEACON: JWST NIRCam Pure-parallel imaging survey : I. survey design and initial results
ID Morishita, Takahiro (Author), ID Mason, Charlotte (Author), ID Kreilgaard, Kimi C. (Author), ID Bradač, Maruša (Author)

.pdfPDF - Presentation file, Download (2,09 MB)
MD5: 099CC7E17CB2DCF30C057E530DB1BD5F
URLURL - Source URL, Visit https://iopscience.iop.org/article/10.3847/1538-4357/adbbdc/pdf This link opens in a new window

Abstract
We introduce the Bias-free Extragalactic Analysis for Cosmic Origins with NIRCam (BEACON) survey, a JWST Cycle 2 program allocated up to 600 pure-parallel hours of observations. BEACON explores high-latitude areas of the sky with JWST/NIRCam over ∼100 independent sight lines, totaling ∼0.3 deg2, reaching a median F444W depth of ≈28.2 AB mag (5σ). Based on existing JWST observations in legacy fields, we estimate that BEACON will photometrically identify 25–150 galaxies at z > 10 and 500–1000 at z ∼ 7–10 uniquely enabled by an efficient multiple filter configuration spanning 0.9–5.0 μm. The expected sample size of z > 10 galaxies will allow us to obtain robust number density estimates and to discriminate between different models of early star formation. In this paper, we present an overview of the survey design and initial results using the first 19 fields. We present 129 galaxy candidates at z ≳7 identified in those fields, including 11 galaxies at z ≳10 and several UV-luminous (MUV < ‑21 mag) galaxies at z ∼ 8. The number densities of z < 13 galaxies inferred from the initial fields are overall consistent with those in the literature. Despite reaching a considerably large volume (∼105 Mpc3), however, we find no galaxy candidates at z > 13, providing us with a complimentary insight into early galaxy evolution with minimal cosmic variance. We publish imaging and catalog data products for these initial fields. Upon survey completion, all BEACON data will be coherently processed and distributed to the community along with catalogs for redshift and other physical quantities.

Language:English
Keywords:galaxies, high-redshift galaxies, reionization
Work type:Article
Typology:1.01 - Original Scientific Article
Organization:FMF - Faculty of Mathematics and Physics
Publication status:Published
Publication version:Version of Record
Publication date:01.04.2025
Year:2025
Number of pages:19 str.
Numbering:Vol. 983, id. 152
PID:20.500.12556/RUL-168991 This link opens in a new window
UDC:524.8
ISSN on article:1538-4357
DOI:10.3847/1538-4357/adbbdc This link opens in a new window
COBISS.SI-ID:234938883 This link opens in a new window
Publication date in RUL:06.05.2025
Views:679
Downloads:191
Metadata:XML DC-XML DC-RDF
:
Copy citation
Share:Bookmark and Share

Record is a part of a journal

Title:The Astrophysical journal
Shortened title:Astrophys. j.
Publisher:University of Chicago Press for the American Astronomical Society
ISSN:1538-4357
COBISS.SI-ID:515079705 This link opens in a new window

Licences

License:CC BY 4.0, Creative Commons Attribution 4.0 International
Link:http://creativecommons.org/licenses/by/4.0/
Description:This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.

Projects

Funder:EC - European Commission
Project number:101053208
Name:Exploring Cosmic Dawn with James Webb Space Telescope
Acronym:FIRSTLIGHT

Funder:ARIS - Slovenian Research and Innovation Agency
Project number:N1-0238-2022
Name:Raziskave kozmične zore z James Webb vesoljskim teleskopom

Funder:ARIS - Slovenian Research and Innovation Agency
Project number:P1-0188-2015
Name:Astrofizika in fizika atmosfere

Similar documents

Similar works from RUL:
Similar works from other Slovenian collections:

Back