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The Composite Nature of Dust-obscured Galaxies (DOGs) at <i>z</i> ∼ 2-3 in the COSMOS Field. II. The AGN Fraction
| Indexado |
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| DOI | 10.3847/1538-3881/AB16CD | ||||
| Año | 2019 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
We present the X-ray properties of 108 Dust-Obscured Galaxies (DOGs; F-24 mu m/F-R > 1000) in the COSMOS field, all of which are detected in at least three far-infrared bands with the Herschel Observatory. Out of the entire sample, 22 are individually detected in the hard 2-8 keV X-ray band by the Chandra COSMOS Legacy survey, allowing us to classify them as AGN. Six (27%) of them are Compton-thick AGN candidates with column densities N-H > 10(24) cm(-2), while 15 are moderately obscured AGNs with 10(22) < N-H < 10(24) cm(-2). Additionally, we estimate AGN contributions to the IR luminosity (8-1000 mu m rest-frame) greater than 20% for 19 DOGs based on SED decomposition using Spitzer/MIPS 24 mu m and the five Herschel bands (100-500 mu m). Only 7 of these are detected in X-rays individually. We performed an X-ray stacking analysis for the 86 undetected DOGs. We find that the AGN fraction in DOGs increases with 24 mu m flux and that it is higher than that of the general 24 mu m population. However, no significant difference is found when considering only X-ray detections. This strongly motivates the combined use of X-ray and far-IR surveys to successfully probe a wider population of AGNs, particularly for the most obscured ones.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Sampedro, Laura | Mujer |
UNIV FED RIO DE JANEIRO - Brasil
Universidade Federal do Rio de Janeiro - Brasil |
| 2 | Treister, Ezequiel | Hombre |
Pontificia Universidad Católica de Chile - Chile
|
| 3 | Menendez-Delmestre, Karin | Mujer |
UNIV FED RIO DE JANEIRO - Brasil
Universidade Federal do Rio de Janeiro - Brasil |
| 4 | Cardamone, Carolin | Mujer |
Wheelock Coll - Estados Unidos
Wheelock College of Education & Human Development - Estados Unidos |
| 5 | Civano, F. | Mujer |
Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos |
| 6 | Goncalves, T. | - |
UNIV FED RIO DE JANEIRO - Brasil
Universidade Federal do Rio de Janeiro - Brasil |
| 7 | Hasinger, Guenther | - |
Univ Hawaii - Estados Unidos
University of Hawaii at Manoa - Estados Unidos University of Hawaiʻi at Mānoa - Estados Unidos University Hawaii Institute for Astronomy - Estados Unidos |
| 8 | Koekemoer, Anton | Hombre |
Space Telescope Sci Inst - Estados Unidos
STScI - Estados Unidos Space Telescope Science Institute - Estados Unidos |
| 9 | Lanzuisi, Giorgio | Hombre |
UNIV BOLOGNA - Italia
Istituto Nazionale di Astrofisica - Italia Alma Mater Studiorum Università di Bologna - Italia Osservatorio Astronomico Di Bologna - Italia |
| 10 | Floc'H, E. Le | Hombre |
CNRS Centre National de la Recherche Scientifique - Francia
CEA Saclay - Francia Univ Paris Diderot - Francia |
| 10 | Le Floc'h, E. | Hombre |
Univ Paris Diderot - Francia
CNRS Centre National de la Recherche Scientifique - Francia CEA Saclay - Francia |
| 11 | Lusso, Elisabeta | Mujer |
Univ Durham - Reino Unido
University of Durham - Reino Unido Durham University - Reino Unido |
| 12 | Lutz, D. | Hombre |
Max Planck Inst Extraterr Phys - Alemania
Max Planck Institute for Extraterrestrial Physics - Alemania |
| 13 | Marchesi, S. | Hombre |
Clemson Univ - Estados Unidos
Clemson University - Estados Unidos |
| 14 | Miyaji, Takamitsu | - |
Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México |
| 15 | Pozzi, Francesca | Mujer |
UNIV BOLOGNA - Italia
Istituto Nazionale di Astrofisica - Italia Osservatorio Astronomico Di Bologna - Italia Alma Mater Studiorum Università di Bologna - Italia |
| 16 | Ricci, C. | Hombre |
Pontificia Universidad Católica de Chile - Chile
Universidad Diego Portales - Chile Peking Univ - China CASSACA - Chile China Chile Joint Ctr Astron - Chile Peking University - China Chinese Academy of Sciences South America Center for Astronomy - Chile |
| 17 | Rodighiero, G. | Mujer |
Univ Padua - Italia
Università degli Studi di Padova - Italia University of Durham - Italia |
| 18 | Pannella, M. | Hombre |
Max Planck Inst Plasma Phys - Alemania
Max Planck Institute for Plasma Physics - Alemania |
| 19 | Sanders, David | Hombre |
Univ Hawaii - Estados Unidos
University of Hawaii at Manoa - Estados Unidos University of Hawaiʻi at Mānoa - Estados Unidos University Hawaii Institute for Astronomy - Estados Unidos |
| 20 | Schawinski, K. | Hombre |
Swiss Fed Inst Technol - Suiza
ETH Zurich - Suiza |
| 21 | Suh, Hyewon | Mujer |
Natl Astron Observ Japan - Estados Unidos
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón |
| Fuente |
|---|
| FONDECYT |
| CONICYT-Chile |
| CONACYT |
| NASA |
| Seventh Framework Programme |
| BMVIT (Austria) |
| ESA-PRODEX (Belgium) |
| CEA/CNES (France) |
| ASI/INAF (Italy) |
| CICYT/MCYT (Spain) |
| DLR (Germany) |
| UNAM-DGAPA PAPIIT |
| Anillo de Ciencia y Tecnologia |
| CSA (Canada) |
| NAOC (China) |
| ASI (Italy) |
| MCINN (Spain) |
| SNSB (Sweden) |
| NASA (USA) |
| ESA Member States |
| ETH Zurich |
| Borders |
| Peking University |
| CEA, CNES, CNRS (France) |
| STFC, UKSA (UK) |
| European Union COFUND/Durham Junior Research Fellowship (EU grant) |
| FP7 Career Integration Grant "eEASy" |
| Productivity in Research Grant of the Brazilian National Council for Scientific and Technological Development (CNPq) |
| China-CONICYT fund |
| Italy Max-Planck-Institute f�r Plasma Physics |
| Vicolo dell |
| People's Republic of China Chinese Academy of Sciences South America Center for Astronomy and China-Chile Joint Center for Astronomy |
| Agradecimiento |
|---|
| E.T. acknowledges support from CONICYT-Chile grants Basal-CATA PFB-06/2007 and AFB-170002, FONDECYT Regular 1160999 and 1190818, and Anillo de ciencia y tecnologia ACT1720033. K.M.D. and T.S.G. are thankful for the support of the Productivity in Research Grant of the Brazilian National Council for Scientific and Technological Development (CNPq). T. M. and the development of CSTACK are supported by CONACyT IB 252531 and UNAM-DGAPA PAPIIT IN104216 E. L. is supported by a European Union COFUND/Durham Junior Research Fellowship (under EU grant agreement No. 609412) G.L. acknowledges support from the FP7 Career Integration Grant "eEASy" (CIG 321913) and grant ASI/INAF I/037/12/0-011/13. C. R. acknowledge financial support from FONDECYT 1141218, Basal-CATA PFB-06/2007 and the China-CONICYT fund. |
| Laurie A. Riguccini Ezequiel Treister Karin Men�ndez-Delmestre Carolin Cardamone Francesca Civano Thiago S. Gon�alves Guenther Hasinger Anton M. Koekemoer Giorgio Lanzuisi Emeric Le Floc’h Elisabeta Lusso Dieter Lutz Stefano Marchesi Takamitsu Miyaji Francesca Pozzi Claudio Ricci Giulia Rodighiero Mara Salvato Dave Sanders Kevin Schawinski Hyewon Suh Laurie A. Riguccini Ezequiel Treister Karin Men�ndez-Delmestre Carolin Cardamone Francesca Civano Thiago S. Gon�alves Guenther Hasinger Anton M. Koekemoer Giorgio Lanzuisi Emeric Le Floc’h Elisabeta Lusso Dieter Lutz Stefano Marchesi Takamitsu Miyaji Francesca Pozzi Claudio Ricci Giulia Rodighiero Mara Salvato Dave Sanders Kevin Schawinski Hyewon Suh Observat�rio do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Ant�nio 43, Sa�de, Rio de Janeiro, RJ 20080-090, Brazil Instituto de Astrof�sica, Facultad de F�sica, Pontificia Universidad Cat�lica de Chile, Casilla 306, Santiago 22, Chile Math and Science Department, Wheelock College, Boston, MA 02215, USA Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Dipartimento di Fisica e Astronomia, Universita di Bologna, viale Berti Pichat 6/2, I-40127 Bologna, Italy INAF Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127, Bologna, Italy Laboratoire AIM, CEA/DSM-CNRS-Universit� Paris Diderot, IRFU/Service d’Astrophysique, B�t.709, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex, France Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK Max-Planck-Institut f�r extraterrestrische Physik, Postfach 1312, Giessenbachstrasse 1, D-85741 Garching, Germany Department of Physics & Astronomy, Clemson University, Clemson, SC 29634, USA Universidad Nacional Aut�noma de M�xico sede Ensenada, Carret. Tijuna-Ensenada Km 103, Ensenada 22860, BC, Mexico Dipartimento di Fisica e Astronomia, Universit� degli Studi di Bologna, Viale Berti Pichat 6/2, I-40127 Bologna, Italy N�cleo de Astronom�a de la Facultad de Ingenier�a, Universidad Diego Portales, Av. Ej�rcito Libertador 441, Santiago, Chile Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China Chinese Academy of Sciences South America Center for Astronomy and China-Chile Joint Center for Astronomy, Camino El Observatorio 1515, Las Condes, Santiago, Chile Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, Vicolo dell Osservatorio 3, I-35122, Italy Max-Planck-Institute f�r Plasma Physics, Boltzmann Strasse 2, Garching D-85748, Germany Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland Subaru Telescope, National Astronomical Observatory of Japan, 650 North A’ohoku Place, Hilo, HI 96720, USA CAPES/BJT Science Without Borders Postdoctoral Fellow, Brazil. Laurie A. Riguccini, Ezequiel Treister, Karin Men�ndez-Delmestre, Carolin Cardamone, Francesca Civano, Thiago S. Gon�alves, Guenther Hasinger, Anton M. Koekemoer, Giorgio Lanzuisi, Emeric Le Floc’h, Elisabeta Lusso, Dieter Lutz, Stefano Marchesi, Takamitsu Miyaji, Francesca Pozzi, Claudio Ricci, Giulia Rodighiero, Mara Salvato, Dave Sanders, Kevin Schawinski and Hyewon Suh 2019-06-01 2019-05-21 13:36:45 cgi/release: Article released bin/incoming: New from .zip yes We present the X-ray properties of 108 Dust-Obscured Galaxies (DOGs; F 24 μ m / F R �>�1000) in the COSMOS field, all of which are detected in at least three far-infrared bands with the Herschel Observatory. Out of the entire sample, 22 are individually detected in the hard 2–8 keV X-ray band by the Chandra COSMOS Legacy survey, allowing us to classify them as AGN. Six (27%) of them are Compton-thick AGN candidates with column densities N H �>�10 24 cm −2 , while 15 are moderately obscured AGNs with 10 22 �<� N H �<�10 24 cm −2 . Additionally, we estimate AGN contributions to the IR luminosity (8–1000 μ m rest-frame) greater than 20% for 19 DOGs based on SED decomposition using Spitzer /MIPS 24 μ m and the five Herschel bands (100–500 μ m). Only 7 of these are detected in X-rays individually. We performed an X-ray stacking analysis for the 86 undetected DOGs. We find that the AGN fraction in DOGs increases with 24 μ m flux and that it is higher than that of the general 24 μ m population. However, no significant difference is found when considering only X-ray detections. This strongly motivates the combined use of X-ray and far-IR surveys to successfully probe a wider population of AGNs, particularly for the most obscured ones. � 2019. The American Astronomical Society. All rights reserved. Aird J., Coil A. L., Georgakakis A. et al 2015 MNRAS 451 1892 10.1093/mnras/stv1062 Aird J., Coil A. 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