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Journal articles
Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging
H. Dannerbauer
1, *
Emanuele Daddi
1
G. E. Morrison
2
B. Altieri
3
P. Andreani
4, 5
H. Aussel
1
S. Berta
6
A. Bongiovanni
7
A. Cava
7
J. Cepa
7
Alessandro Cimatti
8
H. Dominguez
9
D. Elbaz
1
N. Forster Schreiber
6
R. Genzel
6
C. Gruppioni
9
B. Horeau
1
H. S. Hwang
1
E. Le Floc'H
1
J. Le Pennec
1
D. Lutz
6
G. Magdis
1
B. Magnelli
6
R. Maiolino
10
R. Nordon
6
A. M. Perez Garcia
7
A. Poglitsch
6
P. Popesso
6
F. Pozzi
8
L. Riguccini
1
G. Rodighiero
11
A. Saintonge
6
P. Santini
12
M. Sanchez-Portal
3
L. Shao
6
E. Sturm
6
L. Tacconi
6
I. Valtchanov
3
*
Corresponding author
H. Dannerbauer 1
Correspondent author
Emanuele Daddi 1
Author
G. E. Morrison 2
Author
B. Altieri 3
Author
L. Tacconi 6
Author
I. Valtchanov 3
Author
1
AIM (UMR_7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation (AIM - UMR 7158 - UMR E 9005,
ex "Astrophysique Interactions Multi-échelles",
Service d'astrophysique,
CEA/Saclay,
Orme des Merisiers
F-91191 GIF SUR YVETTE CEDEX - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : UMR_E_9005 (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Université Paris-Saclay (Espace Technologique, Bat. Discovery - RD 128 - 2e ét., 91190 Saint-Aubin - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7158 (France)
- UP - Université de Paris : UMR_7158 (85 boulevard Saint-Germain 75006 Paris - France)
2
Institute for Astronomy [Honolulu] (2680 Woodlawn Dr., Honolulu, HI 96822, USA - United States)
- UHM - University of Hawai‘i [Mānoa] (1890 East-West Rd, Honolulu, HI 96822 - United States)
3
Herschel Science Centre (Herschel Science Centre, European Space Astronomy Centre, European Space Agency (ESA), Post Office Box 78, 28691 Villanueva de la Cañada, Madrid, Spain - Spain)
- ESA - European Space Agency (France)
4
ESO - European Southern Observatory (Karl-Schwarzchild Str. 2 D-85748 Garching bei Munchen - Germany)
5
OAT - INAF - Osservatorio Astronomico di Trieste (Via G.B. Tiepolo 11 34143 TRIESTE, Italy - Italy)
- INAF - Istituto Nazionale di Astrofisica (Viale del Parco Mellini 84, 00136 Roma - Italy)
6
MPE - Max Planck Institute for Extraterrestrial Physics (Germany)
- Max-Planck-Gesellschaft (Jägerstrasse, 10-11, D-10117 Berlin - Germany)
7
IAC - Instituto de Astrofisica de Canarias (Calle Vía Láctea, s/n, 38205 San Cristóbal de La Laguna, Santa Cruz de Tenerife - Spain)
8
Dipartimento di Astronomia (Dipartimento di Astronomia, Università di Bologna, Via Ranzani 1, I-40127 Bologna - Italy)
- UNIBO - Alma Mater Studiorum Università di Bologna [Bologna] (Via Zamboni, 33 - 40126 Bologna - Italy)
9
IASF-Bo - Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (Via gobetti 101 40129 Bologna - Italy)
- INAF - Istituto Nazionale di Astrofisica (Viale del Parco Mellini 84, 00136 Roma - Italy)
10
IASF-Roma - Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (Via del Fosso del Cavaliere 100 00133 Roma - Italy)
- INAF - Istituto Nazionale di Astrofisica (Viale del Parco Mellini 84, 00136 Roma - Italy)
11
Dipartimento di Astronomia [Padova] (Italy)
- Universita degli Studi di Padova (Via 8 Febbraio 2, 35122 Padova - Italy)
12
OAR - INAF - Osservatorio Astronomico di Roma (Via Frascati 33, 00040, Monte Porzio Catone - Italy)
- INAF - Istituto Nazionale di Astrofisica (Viale del Parco Mellini 84, 00136 Roma - Italy)
Abstract : We present a search for Herschel-PACS counterparts of dust-obscured, high-redshift objects previously selected at submillimeter and millimeter wavelengths in the Great Observatories Origins Deep Survey North field. We detect 22 of 56 submillimeter galaxies (39%) with a SNR of $\geq$3 at 100 $\mu$m down to 3.0 mJy, and/or at 160 $\mu$m down to 5.7 mJy. The fraction of SMGs seen at 160 $\mu$m is higher than that at 100 $\mu$m. About 50% of radio-identified SMGs are associated with PACS sources. We find a trend between the SCUBA/PACS flux ratio and redshift, suggesting that these flux ratios could be used as a coarse redshift indicator. PACS undetected submm/mm selected sources tend to lie at higher redshifts than the PACS detected ones. A total of 12 sources (21% of our SMG sample) remain unidentified and the fact that they are blank fields at Herschel-PACS and VLA 20 cm wavelength may imply higher redshifts for them than for the average SMG population (e.g., $z>3-4$). The Herschel-PACS imaging of these dust-obscured starbursts at high-redshifts suggests that their far-infrared spectral energy distributions have significantly different shapes than template libraries of local infrared galaxies.
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Journal articles
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https://hal-cea.archives-ouvertes.fr/cea-01001863
Contributor : Bruno Savelli <>
Submitted on : Monday, November 2, 2020 - 3:03:45 PM
Last modification on : Saturday, June 12, 2021 - 11:54:01 AM
Contributor : Bruno Savelli <>
Submitted on : Monday, November 2, 2020 - 3:03:45 PM
Last modification on : Saturday, June 12, 2021 - 11:54:01 AM
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Identifiers
- HAL Id : cea-01001863, version 1
- ARXIV : 1007.1902
- DOI : 10.1088/2041-8205/720/2/L144
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CEA | INSU | CNRS | UP-SCIENCES
Citation
H. Dannerbauer, Emanuele Daddi, G. E. Morrison, B. Altieri, P. Andreani, et al.. Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging. The Astrophysical journal letters, Bristol : IOP Publishing, 2010, 720 (2), pp.L144-L148. ⟨10.1088/2041-8205/720/2/L144⟩. ⟨cea-01001863⟩
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