2022MNRAS.515.3911B

Query : 2022MNRAS.515.3911B

2022MNRAS.515.3911B - Mon. Not. R. Astron. Soc., 515, 3911-3937 (2022/September-3)

PASSAGES: the Large Millimeter Telescope and ALMA observations of extremely luminous high-redshift galaxies identified by the Planck.

BERMAN D.A., YUN M.S., HARRINGTON K.C., KAMIENESKI P., LOWENTHAL J., FRYE B.L., WANG Q.D., WILSON G.W., ARETXAGA I., CHAVEZ M., CYBULSKI R., DE LA LUZ V., ERICKSON N., FERRUSCA D., HUGHES D.H., MONTANA A., NARAYANAN G., SANCHEZ-ARGUELLES D., SCHLOERB F.P., SOUCCAR K., TERLEVICH E., TERLEVICH R. and ZAVALA J.A.

Abstract (from CDS):

The Planck All-Sky Survey to Analyze Gravitationally-lensed Extreme Starbursts project aims to identify a population of extremely luminous galaxies using the Planck all-sky survey and to explore the nature of their gas fuelling, induced starburst, and the resulting feedback that shape their evolution. Here, we report the identification of 22 high-redshift luminous dusty star-forming galaxies (DSFGs) at z = 1.1-3.3 drawn from a candidate list constructed using the Planck Catalogue of Compact Sources and Wide-field Infrared Survey Explorer all-sky survey. They are confirmed through follow-up dust continuum imaging and CO spectroscopy using AzTEC and the Redshift Search Receiver on the Large Millimeter Telescope Alfonso Serrano. Their apparent infrared luminosities span (0.1-3.1) × 1014 L⊙ (median of 1.2 × 1014 L⊙), making them some of the most luminous galaxies found so far. They are also some of the rarest objects in the sky with a source density of ≲0.01 deg–2. Our Atacama Large Millimeter/submillimeter Array 1.1 mm continuum observations with θ ≈ 0.4 arcsec resolution show clear ring or arc morphologies characteristic of strong lensing. Their lensing-corrected luminosity of LIR ≳ 1013 L⊙ (star-formation rate ≳ 103 M⊙ yr–1) indicates that they are the magnified versions of the most intrinsically luminous DSFGs found at these redshifts. Our spectral energy distribution analysis finds little detectable active galactic nucleus (AGN) activity despite their enormous luminosity, and any AGN activity present must be extremely heavily obscured.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): galaxies: high-redshift - galaxies: ISM - galaxies: starburst - gravitational lensing: strong - infrared: galaxies - submillimetre: galaxies

Nomenclature: Tables 2+A1: [BYH2022] PJHHMMSS.s N=24.

Simbad objects: 43

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Number of rows : 43
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 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 [BYH2022] PJ011646.8 G 01 16 46.8 -24 37 02           ~ 7 0
3 SPT-S J012506-4723.7 rG 01 25 07.180 -47 23 55.50           ~ 19 0
4 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
5 [BYH2022] PJ014341.2 G 01 43 41.2 -01 47 26           ~ 2 0
6 [BYH2022] PJ022634.0 G 02 26 33.98 +23 45 28.3           ~ 4 0
7 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 7988 0
8 [BYH2022] PJ030510.6 G 03 05 10.62 -30 36 30.3           ~ 3 0
9 NGC 1275 Bla 03 19 48.1599902040 +41 30 42.108850836   13.10 12.48 11.09   ~ 4243 3
10 NAME Hubble Ultra Deep Field reg 03 32 39.0 -27 47 29           ~ 1900 0
11 ACT-S J053817-503058 rG 05 38 16.830 -50 30 52.00           ~ 33 1
12 PLCKESZ G157.43+30.33 ClG 07 48 45.6 +59 41 41           ~ 23 0
13 [BYH2022] PJ074851.7 LeG 07 48 51.72 +59 41 53.5           ~ 2 0
14 [BYH2022] PJ074852.6 G 07 48 52.6 +59 42 09           ~ 1 0
15 QSO J0831+5245 QSO 08 31 41.7108197808 +52 45 17.616994560   19.2   14.5 13.9 ~ 574 1
16 [BYH2022] PJ084648.6 G 08 46 48.6 +15 05 57           ~ 1 0
17 [BYH2022] PJ084650.1 LeG 08 46 50.16 +15 05 47.3           ~ 3 0
18 H-ATLAS J090403.9+005619 G 09 04 03.9 +00 56 19           ~ 2 0
19 [VV96] J102434.5+470911 Sy1 10 24 34.5 +47 09 11     20.5     ~ 489 0
20 [CNG2015] PLCK G145.2+50.9 LeG 10 53 22.56 +60 51 49.0           ~ 13 0
21 [BYH2022] PJ112713.4 G 11 27 13.44 +46 09 24.1           ~ 3 0
22 [BYH2022] PJ113805.5 G 11 38 05.53 +32 57 56.9           ~ 3 0
23 [BYH2022] PJ113921.7 G 11 39 21.60 +20 24 53.0           ~ 6 0
24 2MASX J11403845+5321569 G 11 40 38.452 +53 21 56.96           ~ 6 0
25 [BYH2022] PJ114038.5 G 11 40 38.5 +53 21 57           ~ 1 0
26 [BYH2022] PJ114329.5 G 11 43 29.5 +68 01 07           ~ 1 0
27 2MASX J11432955+6801060 EmG 11 43 29.5211412912 +68 01 06.616312464           ~ 3 0
28 3C 279 Bla 12 56 11.16657958 -05 47 21.5251510   18.01 17.75 15.87   ~ 3205 2
29 [BYH2022] PJ132217.5 LeG 13 22 17.52 +09 23 26.4           ~ 2 0
30 NAME NAv1.195 G 13 26 30.216 +33 44 07.60           ~ 17 0
31 NAME Cosmic Eyebrow LeG 13 29 34.18 +22 43 27.3           ~ 12 0
32 [BYH2022] PJ132935.3 G 13 29 35.3 +22 43 24           ~ 1 0
33 [BYH2022] PJ133634.9 G 13 36 34.94 +49 13 13.6           ~ 4 0
34 [BYH2022] PJ141230.5 G 14 12 30.5 +50 34 55           ~ 1 0
35 QSO J1415+1129 QSO 14 15 46.25 +11 29 43.4   17.63 17.23     ~ 678 0
36 [BYH2022] PJ144653.2 G 14 46 53.2 +17 52 33           ~ 2 0
37 [BYH2022] PJ144958.6 G 14 49 58.59 +22 38 36.8           ~ 3 0
38 [BYH2022] PJ154432.4 LeG 15 44 32.40 +50 23 46.0           ~ 7 0
39 NAME Eyelash LeG 21 35 11.60 -01 02 52.0           ~ 245 0
40 NAME Cosmic Eye G 21 35 12.730 -01 01 42.90           ~ 92 0
41 3C 454.3 Bla 22 53 57.7480438728 +16 08 53.561508864   16.57 16.10 15.22   ~ 3004 2
42 [BYH2022] PJ231356.6 G 23 13 56.64 +01 09 17.7           ~ 3 0
43 SPT-S J233227-5358.5 rG 23 32 26.50 -53 58 39.8           ~ 14 1

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