Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey

被引：86

作者：

Ciesla, L. ^{[1
,2
]}

Boselli, A. ^{[1
,2
]}

Smith, M. W. L. ^{[3
]}

Bendo, G. J. ^{[4
]}

Cortese, L. ^{[5
]}

Eales, S. ^{[3
]}

Bianchi, S. ^{[6
]}

Boquien, M. ^{[1
,2
]}

Buat, V. ^{[1
,2
]}

Davies, J. ^{[3
]}

Pohlen, M. ^{[3
]}

Zibetti, S. ^{[6
,7
]}

Baes, M. ^{[8
]}

Cooray, A. ^{[9
,10
]}

de Looze, I. ^{[8
]}

Alighieri, S. di Serego ^{[6
]}

Galametz, M. ^{[11
]}

Gomez, H. L. ^{[3
]}

Lebouteiller, V. ^{[12
]}

Madden, S. C. ^{[12
]}

Pappalardo, C. ^{[6
]}

Remy, A. ^{[12
]}

Spinoglio, L. ^{[13
]}

Vaccari, M. ^{[14
,15
]}

Auld, R. ^{[3
]}

Clements, D. L. ^{[16
]}

机构：

[1] Univ Aix Marseille, Lab Astrophys Marseille, LAM, F-13388 Marseille 13, France

[2] CNRS, UMR7326, F-13388 Marseille 13, France

[3] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[4] Univ Manchester, Sch Phys & Astron, Ctr Astrophys, UK ALMA Reg Ctr Node,Jodrell Bank, Manchester M13 9PL, Lancs, England

[5] European So Observ, D-85748 Garching, Germany

[6] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy

[7] Univ Copenhagen, Dark Cosmol Ctr, Niels Bohr Inst, DK-2100 Copenhagen, Denmark

[8] Univ Ghent, Sterrenkundig Observ, B-9000 Ghent, Belgium

[9] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[10] CALTECH, Pasadena, CA 91125 USA

[11] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

[12] CEA Saclay, Serv Astrophys, CEA, DSM IRFU, F-91191 Gif Sur Yvette, France

[13] INAF, Ist Fis Spazio Interplanetario, I-00133 Rome, Italy

[14] Univ Padua, Vicolo Osservatorio, Dipartimento Astron, I-35122 Padua, Italy

[15] Univ Western Cape, Dept Phys, Astrophys Grp, ZA-7535 Cape Town, South Africa

[16] Univ London Imperial Coll Sci Technol & Med, Astrophys Grp, Blackett Lab, London SW7 2AZ, England

来源：

ASTRONOMY & ASTROPHYSICS | 2012年 / 543卷

基金：

新加坡国家研究基金会; 美国国家航空航天局;

关键词：

galaxies: ISM; infrared: galaxies; surveys; catalogs; VIRGO-CLUSTER SURVEY; POLYCYCLIC AROMATIC-HYDROCARBONS; FAR-INFRARED PROPERTIES; SPIRE INSTRUMENT; HUBBLE SEQUENCE; STAR-FORMATION; DUST FORMATION; SKY SURVEY; NGC; 2403; SAMPLE;

D O I：

10.1051/0004-6361/201219216

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Herschel Reference Survey (HRS) is a guaranteed time Herschel key project aimed at studying the physical properties of the interstellar medium in galaxies of the nearby universe. This volume limited, K-band selected sample is composed of galaxies spanning the whole range of morphological types (from ellipticals to late-type spirals) and environments (from the field to the centre of the Virgo Cluster). We present flux density measurements of the whole sample of 323 galaxies of the HRS in the three bands of the Spectral and Photometric Imaging Receiver (SPIRE), at 250 mu m, 350 mu m and 500 mu m. Aperture photometry is performed on extended galaxies and point spread function (PSF) fitting on timeline data for unresolved objects; we carefully estimate errors and upper limits. The flux densities are found to be in good agreement with those of the HeViCS and KINGFISH key projects in all SPIRE bands, and of the Planck consortium at 350 mu m and 550 mu m, for the galaxies in common. This submillimetre catalogue of nearby galaxies is a benchmark for the study of the dust properties in the local universe, giving the zero redshift reference for any cosmological survey.

引用

页数：25

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