TY - JOUR
T1 - Erratum
T2 - The ALMA Frontier Fields Survey: IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACS J0416.1-2403, and MACS J1149.5+2223 (A&A (2018) 620 A125 DOI: 10.1051/0004-6361/201732442)
AU - Muñoz Arancibia, A. M.
AU - González-López, J.
AU - Ibar, E.
AU - Bauer, F. E.
AU - Carrasco, M.
AU - Laporte, N.
AU - Anguita, T.
AU - Aravena, M.
AU - Barrientos, F.
AU - Bouwens, R. J.
AU - Demarco, R.
AU - Infante, L.
AU - Kneissl, R.
AU - Nagar, N.
AU - Padilla, N.
AU - Romero-Cañizales, C.
AU - Troncoso, P.
AU - Zitrin, A.
N1 - Publisher Copyright:
© 2019 EDP Sciences. All rights reserved.
PY - 2019/11/1
Y1 - 2019/11/1
N2 - We noticed an error in the code that conducts the source injection simulations used in our article Muñoz Arancibia et al. (2018). This error led the source scale radii in the image plane to be 1=2:35 times smaller that what it should be. Wrongly computed scale radii primarily a ect the calculation of first, completeness as a function of image-plane integrated flux density curves for di erent image-plane scale radii; and second, image-plane integrated flux densities estimated for low-significance ALMA detections. These in turn a ect the calculation of deboosting correction factors, demagnified integrated flux densities (for low-significance ALMA detections), di erential and cumulative number counts, and the contribution to the extragalactic background light.
AB - We noticed an error in the code that conducts the source injection simulations used in our article Muñoz Arancibia et al. (2018). This error led the source scale radii in the image plane to be 1=2:35 times smaller that what it should be. Wrongly computed scale radii primarily a ect the calculation of first, completeness as a function of image-plane integrated flux density curves for di erent image-plane scale radii; and second, image-plane integrated flux densities estimated for low-significance ALMA detections. These in turn a ect the calculation of deboosting correction factors, demagnified integrated flux densities (for low-significance ALMA detections), di erential and cumulative number counts, and the contribution to the extragalactic background light.
UR - http://www.scopus.com/inward/record.url?scp=85103737966&partnerID=8YFLogxK
U2 - 10.1051/0004-6361/201732442e
DO - 10.1051/0004-6361/201732442e
M3 - Comment/debate
AN - SCOPUS:85103737966
SN - 0004-6361
VL - 631
JO - Astronomy and Astrophysics
JF - Astronomy and Astrophysics
M1 - C2
ER -