CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 deg2 field and the impact of field-to-field variance
Artikel i vetenskaplig tidskrift, 2023
In the submillimeter regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time. However, both of these two measurements suffer from field-to-field variance. We study the effect of field-to-field variance on the predicted CO and [CII] power spectra from future LIM experiments such as CONCERTO, as well as on the line luminosity functions (LFs) and the cosmic molecular gas mass density that are currently derived from spectral line scans. We combined a 117 deg2 dark matter lightcone from the Uchuu cosmological simulation with the simulated infrared dusty extragalactic sky (SIDES) approach. The clustering of the dusty galaxies in the SIDES-Uchuu product is validated by reproducing the cosmic infrared background anisotropies measured by Herschel and Planck. We find that in order to constrain the CO LF with an uncertainty below 20%, we need survey sizes of at least 0.1 deg2. Furthermore, accounting for the field-to-field variance using only the Poisson variance can underestimate the total variance by up to 80%. The lower the luminosity is and the larger the survey size is, the higher the level of underestimate. At z < 3, the impact of field-to-field variance on the cosmic molecular gas density can be as high as 40% for the 4.6 arcmin2 field, but drops below 10% for areas larger than 0.2 deg2. However, at z > 3 the variance decreases more slowly with survey size and for example drops below 10% for 1 deg2 fields. Finally, we find that the CO and [CII] LIM power spectra can vary by up to 50% in 1 deg2 fields. This limits the accuracy of the constraints provided by the first 1 deg2 surveys. In addition the level of the shot noise power is always dominated by the sources that are just below the detection thresholds, which limits its potential for deriving number densities of faint [CII] emitters. We provide an analytical formula to estimate the field-to-field variance of current or future LIM experiments given their observed frequency and survey size. The underlying code to derive the field-to-field variance and the full SIDES-Uchuu products (catalogs, cubes, and maps) are publicly available.
Galaxies: star formation
Cosmic background radiation
Galaxies: luminosity function
Large-scale structure of Universe
Mass function
Galaxies: high-redshift
Galaxies: ISM
Författare
A. Gkogkou
Laboratoire d'Astrophysique de Marseille
Matthieu Béthermin
Laboratoire d'Astrophysique de Marseille
Observatoire Astronomique de Strasbourg
G. Lagache
Laboratoire d'Astrophysique de Marseille
M. Van Cuyck
Laboratoire d'Astrophysique de Marseille
E. Jullo
Laboratoire d'Astrophysique de Marseille
Manuel Aravena
Universidad Diego Portales
A. Beelen
Laboratoire d'Astrophysique de Marseille
A. Benoit
Université Grenoble Alpes
Groupement d'Interet Scientifique KID
J. Bounmy
Groupement d'Interet Scientifique KID
Université Grenoble Alpes
M. Calvo
Université Grenoble Alpes
Groupement d'Interet Scientifique KID
A. Catalano
Université Grenoble Alpes
Groupement d'Interet Scientifique KID
S. Cora
Universidad Nacional de La Plata
D. Croton
Swinburne University of Technology
ARC Centre of Excellence for All-sky Astrophysics
S. De La Torre
Laboratoire d'Astrophysique de Marseille
A. Fasano
Laboratoire d'Astrophysique de Marseille
A. Ferrara
Scuola Normale Superiore di Pisa
J. Goupy
Université Grenoble Alpes
Groupement d'Interet Scientifique KID
C. Hoarau
Groupement d'Interet Scientifique KID
Université Grenoble Alpes
W. Hu
Laboratoire d'Astrophysique de Marseille
T. Ishiyama
Chiba University
Kirsten Knudsen
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
J. C. Lambert
Laboratoire d'Astrophysique de Marseille
J. F. Maciás-Pérez
Groupement d'Interet Scientifique KID
Université Grenoble Alpes
J. Marpaud
Université Grenoble Alpes
Groupement d'Interet Scientifique KID
G. Mellema
Oskar Klein Centre
A. Monfardini
Université Grenoble Alpes
Groupement d'Interet Scientifique KID
Andrea Pallottini
Scuola Normale Superiore di Pisa
N. Ponthieu
Groupement d'Interet Scientifique KID
Université Grenoble Alpes
F. Prada
Instituto de Astrofisica de Andalucía (IAA)
Y. Roehlly
Laboratoire d'Astrophysique de Marseille
L. Vallini
Scuola Normale Superiore di Pisa
F. Walter
Max-Planck-Gesellschaft
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 670 A16Ämneskategorier
Astronomi, astrofysik och kosmologi
Atom- och molekylfysik och optik
Signalbehandling
DOI
10.1051/0004-6361/202245151