NIKA2 Cosmological Legacy Survey. First measurement of the confusion noise at the IRAM 30 m telescope

The NIKA2 Cosmological Legacy Survey (N2CLS) is a large programme using the NIKA2 dual-band camera on the IRAM 30 m telescope. Its goal is to improve our understanding of the physics of distant Dusty Star Forming Galaxies (DSFGs) by carrying out deep surveys of two fields, GOODS-North and COSMOS. This work is focussed on GOODS-North, which was observed for 78.2 hours, simultaneously at 1.2 and 2 mm, with a field of view of ∼240 arcmin 2 . With such a deep integration, we were able to measure, for the first time, the confusion noise limits at the 30 m telescope using the best sampled ∼62 arcmin 2 and masking sources with a flux greater than 0.54 or 0.17 mJy at 1.2 or 2 mm, respectively. We found a confusion noise of 139.1 −19.2 +15.9 ±11.9 μJy/beam at 1.2 mm and 38.6 −13.1 +9.6 ±3.7 μJy/beam at 2 mm (the first uncertainty is statistical, the second is the cosmic variance). In this region, this corresponds to half the instrumental noise. To derive these estimates, we devised a novel estimator, referred to as the cross variance, which also enabled us to estimate the correlated confusion noise between the two bands. Thus, we obtained a result of 49.6 −24.8 +15.9 ±6.4 μJy/beam. These values are consistent with the state of the art Simulated Infrared Dusty Extragalactic Sky (SIDES) model.

Authors

Institutions

Publication Details

Journal
Astronomy and Astrophysics
Published
2025-12-19
DOI
https://doi.org/10.1051/0004-6361/202554530
Citations
1
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
1.15

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

NIKA2 Cosmological Legacy Survey. First measurement of the confusion noise at the IRAM 30 m telescope

Á. Bongiovanni, Arlene Moore Sievers, F. Ruppin, F. Kéruzoré et al.
1 citations
Astronomy and Astrophysics
Galaxies: Formation, Evolution, Phenomena
1.15
article

NIKA2 Cosmological Legacy Survey. First measurement of the confusion noise at the IRAM 30 m telescope

Á. Bongiovanni, Arlene Moore Sievers, F. Ruppin, F. Kéruzoré, S. Leclercq, P. A. R. Ade, A. Maury, C. Hanser, Stergios Amarantidis, A. J. Rigby, N. Ponthieu, A. Gómez, K. Schuster, M. Muñoz-Echeverría, G. Lagache, I. Myserlis, G. Ejlali, E. F. C. Driessen, H. Ajeddig, V. Revéret, C. Tucker, S. Savorgnano, M. De Petris, M. Calvo Gomez, S. C. Madden, O. Bourrion, B. Ladjelate, M. Béthermin, S. Katsioli, C. Krämer, R. Adam, L. Bing, F. Mayet, R. Zylka, A. Beelen, F. -X. Désert, G. Pisano, J. Goupy, L. Perotto, A. Paliwal, A. Monfardini, A. Ferragamo, J. Bounmy, A. Moyer-Anin, H. Roussel, S. Berta, M. Sánchez-Portal, A. Ritacco, A. Benoît, A. Catalano, S. Doyle, J.F. Macías-Pérez, P. André, J. F. Lestrade, R. Neri, D. Chérouvrier
article en
1 citations

Abstract

The NIKA2 Cosmological Legacy Survey (N2CLS) is a large programme using the NIKA2 dual-band camera on the IRAM 30 m telescope. Its goal is to improve our understanding of the physics of distant Dusty Star Forming Galaxies (DSFGs) by carrying out deep surveys of two fields, GOODS-North and COSMOS. This work is focussed on GOODS-North, which was observed for 78.2 hours, simultaneously at 1.2 and 2 mm, with a field of view of ∼240 arcmin 2 . With such a deep integration, we were able to measure, for the first time, the confusion noise limits at the 30 m telescope using the best sampled ∼62 arcmin 2 and masking sources with a flux greater than 0.54 or 0.17 mJy at 1.2 or 2 mm, respectively. We found a confusion noise of 139.1 −19.2 +15.9 ±11.9 μJy/beam at 1.2 mm and 38.6 −13.1 +9.6 ±3.7 μJy/beam at 2 mm (the first uncertainty is statistical, the second is the cosmic variance). In this region, this corresponds to half the instrumental noise. To derive these estimates, we devised a novel estimator, referred to as the cross variance, which also enabled us to estimate the correlated confusion noise between the two bands. Thus, we obtained a result of 49.6 −24.8 +15.9 ±6.4 μJy/beam. These values are consistent with the state of the art Simulated Infrared Dusty Extragalactic Sky (SIDES) model.

Astronomy and AstrophysicsVol. 705
Université Claude Bernard Lyon 1 (FR), Institut polytechnique de Grenoble (FR), University of Rome Tor Vergata (IT), Institució Catalana de Recerca i Estudis Avançats (ES), Argonne National Laboratory (US), Centre National de la Recherche Scientifique (FR), University of Leeds (GB), Université Toulouse III - Paul Sabatier (FR), University of Sussex (GB), Université Fédérale de Toulouse Midi-Pyrénées (FR), Lyon College (US), National and Kapodistrian University of Athens (GR), Université Côte d'Azur (FR), Université Paris Cité (FR), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris Sciences et Lettres (FR), Université Paris-Saclay (FR), Institut d'Astrophysique de Paris (FR), Observatoire astronomique de Strasbourg (FR), Sorbonne Université (FR), Astrophysique, Instrumentation et Modélisation (FR), Institut de Radioastronomie Millimétrique (FR), Laboratoire d’Astrophysique de Marseille (FR), Institute of Space Sciences (ES), National Observatory of Athens (GR), Observatoire de la Côte d’Azur (FR), CEA Paris-Saclay (FR), Centro de Astrobiología (ES), Institut National de Physique Nucléaire et de Physique des Particules (FR), Institut Néel (FR), Institute for Research in Fundamental Sciences (IR), Cardiff University (GB), Sapienza University of Rome (IT), Université Grenoble Alpes (FR)
Aix-Marseille Université, European Commission, Agence Nationale de la Recherche, Centre National d’Etudes Spatiales, Max-Planck-Gesellschaft, Centre National de la Recherche Scientifique, Institut National de Physique Nucléaire et de Physique des Particules
Openalex Percentile: Top 14%
Galaxies: Formation, Evolution, Phenomena
1.15
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.