2019A&A...632A..79B


Query : 2019A&A...632A..79B

2019A&A...632A..79B - Astronomy and Astrophysics, volume 632A, 79-79 (2019/12-0)

Cold dust and stellar emissions in dust-rich galaxies observed with ALMA: a challenge for SED-fitting techniques.

BUAT V., CIESLA L., BOQUIEN M., MALEK K. and BURGARELLA D.

Abstract (from CDS):


Context. Over the past few years the Atacama Large Millimeter Array (ALMA) has detected dust-rich galaxies whose cold dust emission is spatially disconnected from the ultraviolet (UV) rest-frame emission. This represents a challenge for modeling their spectral energy distributions (SED) with codes based on an energy budget between the stellar and dust components. This could potentially weaken the solidity of the physical parameters measured with these modeling tools.
Aims. We want to verify the validity of energy balance modeling on a sample of galaxies observed from the UV to the sub-millimeter rest frame with ALMA and decipher what information can be reliably retrieved from the analysis of the full SED and from subsets of wavelengths.
Methods. We select 17 sources at z~=2 in the Hubble Ultra-Deep Field (HUDF) and in the GOODS-South field detected with ALMA and Herschel and for which UV to near-infrared rest-frame ancillary data are available. We fit the data with CIGALE exploring different configurations for dust attenuation and star formation histories, considering either the full dataset or one that is reduced to the stellar and dust emission. We compare estimates of the dust luminosities, star formation rates, and stellar masses.
Results. The fit of the stellar continuum alone with the starburst attenuation law can only reproduce up to 50% of the total dust luminosity observed by Herschel and ALMA. This deficit is found to be marginally consistent with similar quantities estimated in the COSMOS field and is found to increase with the specific star formation rate. The combined stellar and dust SEDs are well fitted when different attenuation laws are introduced. Shallow attenuation curves are needed for the galaxies whose cold dust distribution is very compact compared to starlight. The stellar mass estimates are affected by the choice of the attenuation law. The star formation rates are robustly estimated as long as dust luminosities are available. The large majority of the galaxies are above the average main sequence of star forming galaxies and one source is a strong starburst.

Abstract Copyright: © V. Buat et al. 2019

Journal keyword(s): galaxies: high-redshift - galaxies: ISM - infrared: galaxies - dust - extinction

Simbad objects: 21

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Number of rows : 21
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 CANDELS UDS F160W J033214.55-275256.5 AGN 03 32 14.5474 -27 52 56.556   25.7335 24.93 24.52 24.6603 ~ 21 0
2 EIS-DEEP CDFS-3 Ks 1 388 G 03 32 17.21 -27 50 37.2           ~ 22 0
3 NAME GOODS Southern Field reg 03 32 28.0 -27 48 30           ~ 1235 1
4 CANDELS UDS F160W J033228.51-274658.1 AGN 03 32 28.513 -27 46 58.48   26.2       ~ 32 0
5 ASPECS LP.1mm.C07 G 03 32 35.0756 -27 46 47.575           ~ 6 0
6 NAME BzK 4892 AGN 03 32 35.73 -27 49 16.2   25.681 27.798 25.00 24.645 ~ 79 0
7 CANDELS GDS F160W J033235.76-274655.0 G 03 32 35.7654 -27 46 55.050           ~ 1 0
8 ASPECS LP.1mm.C02 G 03 32 36.971 -27 47 27.24   27.66 26.94   25.84 ~ 25 0
9 [SWM2014] GOODS-S 16960 rG 03 32 37.734 -27 50 00.71   24.914   23.95 23.640 ~ 25 0
10 ASPECS LP.3mm.01 AGN 03 32 38.541 -27 46 34.03 26.9734 25.3657 24.647 24.68 24.6471 ~ 60 0
11 NAME Hubble Ultra Deep Field reg 03 32 39.0 -27 47 29           ~ 1533 0
12 GOODS-MUSIC 2690 AGN 03 32 39.248 -27 53 25.61       25.32   ~ 12 0
13 ASPECS LP.1mm.C10 AGN 03 32 40.055 -27 47 55.42 25.2984 24.0577 23.690 23.701 23.084 ~ 58 0
14 CANDELS GDS F160W J033223.50-275449.4 G 03 32 40.7249 -27 47 49.262           ~ 1 0
15 ASPECS LP.3mm.03 G 03 32 41.024 -27 46 31.39   29.3567 28.57   26.99 ~ 27 0
16 ASPECS LP.1mm.C11 G 03 32 43.3236 -27 46 46.798           ~ 4 0
17 ASPECS LP.3mm.07 G 03 32 43.526 -27 46 39.07   28.0435 27.14     ~ 32 0
18 ASPECS LP.3mm.09 AGN 03 32 44.026 -27 46 35.70   29.7791 27.82     ~ 27 0
19 GNS 5040 G 03 32 54.68 -27 51 40.5           ~ 10 0
20 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 2676 0
21 ELAIS N1 reg 16 10 01 +54 30.6           ~ 377 0

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2023.01.27-21:15:06

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