2021A&A...653A..84P


Query : 2021A&A...653A..84P

2021A&A...653A..84P - Astronomy and Astrophysics, volume 653A84-84 (2021/9-1)

The ALPINE-ALMA [CII] survey. Dust mass budget in the early Universe.

POZZI F., CALURA F., FUDAMOTO Y., DESSAUGES-ZAVADSKY M., GRUPPIONI C., TALIA M., ZAMORANI G., BETHERMIN M., CIMATTI A., ENIA A., KHUSANOVA Y., DECARLI R., LE FEVRE O., CAPAK P., CASSATA P., FAISST A.L., YAN L., SCHAERER D., SILVERMAN J., BARDELLI S., BOQUIEN M., ENIA A., NARAYANAN D., GINOLFI M., HATHI N.P., JONES G.C., KOEKEMOER A.M., LEMAUX B.C., LOIACONO F., MAIOLINO R., RIECHERS D.A., RODIGHIERO G., ROMANO M., VALLINI L., VERGANI D. and ZUCCA E.

Abstract (from CDS):


Aims. The dust content of normal galaxies and the dust mass density (DMD) at high-z (z>4) are unconstrained given the source confusion and the sensitivity limitations of previous observations. The ALMA Large Program to INvestigate [CII] at Early times (ALPINE), which targeted 118 ultra-violet (UV)-selected star-forming galaxies at 4.4<z<5.9, provides a new opportunity to tackle this issue for the first time with a statistically robust dataset.
Methods. We exploited the rest-frame far-infrared (FIR) fluxes of 23 galaxies individually detected in their continuum emission, as well as stacked continuum images, to measure the dust content of the 118 UV-selected ALPINE galaxies. We focused on the dust scaling relations and, by comparison with predictions from chemical evolution models, we probed the evolutionary stage of UV-selected galaxies at high-z. By using the observed correlation between the UV luminosity and the dust mass, we estimated the DMD of UV-selected galaxies at z∼5, weighting the galaxies by means of the UV luminosity function. The derived DMD is compared with the value we estimated from ten ALPINE galaxies blindly detected in the FIR continuum, at the redshift of the ALPINE targets.
Results. Our ALMA survey allows the exploration for the first time of the dust content in normal star-forming galaxies at z>4 in a statistically robust sample of sources. The comparison of the observed dust scaling relations with chemical evolution models suggests that ALPINE galaxies are not likely progenitors of disc galaxies, but of intermediate- and low-mass proto-spheroids, resulting in present-day bulges of spiral or elliptical galaxies. Interestingly, this conclusion is in line with the independent morphological analysis that shows that the majority (∼70%) of the dust-continuum detected galaxies have a disturbed morphology. The DMD obtained at z∼5 from UV-selected sources is ∼30% of the value obtained from blind FIR-selected sources, showing that the UV selection misses the most dust-rich, UV-obscured galaxies.

Abstract Copyright: © ESO 2021

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

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GOODS J033217.00-274113.7 EmG 03 32 17.001 -27 41 13.73   28.90 26.89   25.2933 ~ 20 0
2 GOODS J033219.03-275238.2 EmG 03 32 19.01606 -27 52 38.0089   25.05 26.70 29.27 24.3429 ~ 25 0
3 GOODS J033222.97-274629.1 EmG 03 32 22.9703 -27 46 29.089   28.2739 27.45   25.6339 ~ 21 0
4 NAME Extended Chandra Deep Field South reg 03 32 30.0 -27 48 20           ~ 862 0
5 NAME Hubble Ultra Deep Field reg 03 32 39.0 -27 47 29           ~ 1900 0
6 COSMOS2015 552206 EmG 09 58 26.82130 +02 08 26.9804           ~ 11 0
7 COSMOS2015 494057 EmG 09 58 28.52 +02 03 06.8 27.59 28.369 27.394 26.16 24.65 ~ 67 0
8 COSMOS2015 514583 EmG 09 58 57.91 +02 04 51.5     27.565 25.90 24.59 ~ 27 0
9 COSMOS2015 539609 EmG 09 59 07.26 +02 07 21.3 27.70     26.25 24.32 ~ 16 0
10 COSMOS2015 873756 rG 10 00 02.710 +02 37 40.30           ~ 32 0
11 COSMOS2015 683613 EmG 10 00 09.431 +02 20 13.86         25.88 ~ 42 0
12 COSMOS2015 460378 EmG 10 00 11.39 +01 59 54.3 27.76 26.75     25.70 ~ 8 0
13 COSMOS2015 881725 EmG 10 00 13.55 +02 38 16.9     26.898 26.21 24.75 ~ 18 0
14 COSMOS2015 848185 EmG 10 00 21.504 +02 35 11.08   27.450 26.872     ~ 68 0
15 COSMOS2015 493583 EmG 10 00 23.36 +02 03 04.4     26.434 25.32 24.57 ~ 16 0
16 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 3639 0
17 CANDELS COSMOS F160W J100041.16+021714.1 EmG 10 00 41.16 +02 17 14.1   27.712 26.706     ~ 25 0
18 COSMOS2015 396844 EmG 10 00 59.63 +01 53 47.6 27.88 27.465 27.329 25.50 24.59 ~ 18 0
19 COSMOS2015 668056 EmG 10 01 12.50 +02 18 52.7     27.189 25.41 24.18 ~ 29 0
20 COSMOS2015 647354 EmG 10 01 20.12 +02 17 01.3 27.47 27.64 26.45 25.52 24.46 ~ 14 0
21 COSMOS2015 705527 EmG 10 01 33.45 +02 22 10.3   27.359 26.007 25.34 24.08 ~ 15 0
22 COSMOS2015 551281 EmG 10 01 37.47 +02 08 23.6     26.59 25.29 24.68 ~ 17 0
23 COSMOS2015 818760 EmG 10 01 54.86 +02 32 31.5     27.205 26.26 24.27 ~ 31 0
24 COSMOS2015 422677 EmG 10 01 59.46 +01 56 13.1 27.57 27.679 26.788 25.45 24.69 ~ 19 0
25 COSMOS2015 417567 EmG 10 02 04.098 +01 55 44.05           ~ 39 0
26 COSMOS2015 488399 EmG 10 03 01.150 +02 02 36.10         26.35 ~ 23 0

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