| Issue |
A&A
Volume 710, June 2026
|
|
|---|---|---|
| Article Number | A73 | |
| Number of page(s) | 25 | |
| Section | Catalogs and data | |
| DOI | https://doi.org/10.1051/0004-6361/202348390 | |
| Published online | 01 June 2026 | |
The Atacama Cosmology Telescope: Extragalactic Point Sources in the Southern Surveys at 150, 220, and 280 GHz observed between 2008 and 2010
1
Instituto de Astrofísica and Centro de Astro-Ingeniería, Facultad de Física, Pontificia Universidad Católica de Chile,
Av. Vicuña Mackenna 4860,
7820436
Macul,
Santiago,
Chile
2
Instituto de Astrofísica de Canarias,
38200
La Laguna,
Tenerife,
Spain
3
Departamento de Astrofísica, Universidad de La Laguna,
38206
La Laguna,
Tenerife,
Spain
4
Sapienza – University of Rome - Physics department,
Piazzale Aldo Moro 5
00185
Rome,
Italy
5
DAMTP, Centre for Mathematical Sciences, University of Cambridge,
Wilberforce Road,
Cambridge
CB3 OWA,
UK
6
Kavli Institute for Cosmology Cambridge,
Madingley Road,
Cambridge
CB3 0HA,
UK
7
Department of Astronomy/Steward Observatory, University of Arizona,
933 N. Cherry Ave.,
Tucson,
AZ
85721,
USA
8
Center for Astrophysics | Harvard & Smithsonian,
60 Garden St.,
Cambridge,
MA
02138,
USA
9
Wits Centre for Astrophysics, School of Physics, University of the Witwatersrand,
Private Bag 3,
2050
Johannesburg,
South Africa
10
Astrophysics Research Centre, School of Mathematics, Statistics, and Computer Science, University of KwaZulu-Natal,
Westville Campus,
Durban
4041,
South Africa
11
David A. Dunlap Department of Astronomy & Astrophysics, University of Toronto,
50 St. George St.,
Toronto
ON
M5S 3H4,
Canada
12
Specola Vaticana (Vatican Observatory),
V-00120
Vatican City State,
Italy
13
Department of Physics, Florida State University,
Tallahassee
FL
32306,
USA
14
The William H. Miller III Department of Physics and Astronomy, Johns Hopkins University,
3701 San Martin Drive,
Baltimore,
MD
21220,
USA
15
European Southern Observatory,
Karl-Schwarzschild-Str. 2,
85748
Garching,
Germany
16
Department of Physics, Cornell University,
Ithaca,
NY
14853,
USA
17
Department of Astronomy, Cornell University,
Ithaca,
NY
14853,
USA
18
Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University,
Princeton,
NJ
08544,
USA
19
Department of Physics and Astronomy, Haverford College,
Haverford,
PA
19041,
USA
20
Cosmic Dawn Center, Denmark
21
Niels Bohr Institute, University of Copenhagen,
Jagtvej 128,
2200
Copenhagen N,
Denmark
22
Instituto de Física, Pontificia Universidad Católica de Valparaíso,
Casilla
4059,
Valparaíso,
Chile
23
NASA/Goddard Space Flight Center,
Greenbelt,
MD
20771,
USA
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
25
October
2023
Accepted:
21
May
2024
Abstract
We present a multi-frequency, multi-epoch catalog of extragalactic sources. The catalog is based on 150, 220, and 280 GHz observations carried out in 2008, 2009, and 2010 using the Millimeter Bolometric Array Camera on the Atacama Cosmology Telescope. We also present and release 280 GHz maps from 2008 and 2010. The catalog contains 483 sources found in a sky area of ∼600 square degrees. It was obtained by cross-matching sources found in 11 sub-catalogs, one for each season and frequency band. We also include coadded data from ∼150 and ∼160 square degrees using two and three years of overlapping observations. We divide the sources into two populations, synchrotron and dusty emitters, based on their spectral behavior in the 150-280 GHz frequency range. We find 284 synchrotron sources and 183 dusty source candidates. Our cross-matching with catalogs from radio to X-ray results in 251 synchrotron sources (88%) and 92 dusty sources (51%) with counterparts and suggests that 91 dusty candidates are not in existing catalogs. We study the variability and number counts of each population. In the case of synchrotron sources, we find year-to-year variability, with a mean value around 35%. As expected, we find no evidence of dusty source variability. Our number counts generally agree with previous measurements and models, except for dusty sources at 280 GHz, where some models overestimate our results.
Key words: catalogs / surveys / galaxies: active / galaxies: high-redshift / galaxies: starburst / submillimeter: galaxies
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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