CANDIDATE GRAVITATIONALLY LENSED DUSTY STAR-FORMING GALAXIES IN THE HERSCHEL WIDE AREA SURVEYS

被引：57

作者：

Nayyeri, H. ^{[1
]}

Keele, M. ^{[1
]}

Cooray, A. ^{[1
]}

Riechers, D. A. ^{[2
]}

Ivison, R. J. ^{[3
,4
]}

Harris, A. I. ^{[5
]}

Frayer, D. T. ^{[6
]}

Baker, A. J. ^{[7
]}

Chapman, S. C. ^{[8
]}

Eales, S. ^{[9
]}

Farrah, D. ^{[10
]}

Fu, H. ^{[11
]}

Marchetti, L. ^{[12
]}

Marques-Chaves, R. ^{[13
,14
]}

Martinez-Navajas, P. I. ^{[13
,14
]}

Oliver, S. J. ^{[15
]}

Omont, A. ^{[16
]}

Perez-Fournon, I. ^{[13
,14
]}

Scott, D. ^{[17
]}

Vaccari, M. ^{[18
,19
]}

Vieira, J. ^{[20
,21
]}

Viero, M. ^{[22
]}

Wang, L. ^{[23
]}

Wardlow, J. ^{[24
,25
]}

机构：

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

[2] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

[3] European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[4] Univ Edinburgh, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[5] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[6] Natl Radio Astron Observ, Green Bank, WV 24944 USA

[7] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA

[8] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[9] Cardiff Univ, Sch Phys & Astron, Cardiff CF10 3AX, S Glam, Wales

[10] Virginia Polytech Inst & State Univ, Dept Phys, Blacksburg, VA 24061 USA

[11] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA

[12] Open Univ, Dept Phys Sci, Milton Keynes MK7 6AA, Bucks, England

[13] Inst Astrofis Canarias, E-38205 Tenerife, Spain

[14] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain

[15] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England

[16] Univ Paris 06, UMR CNRS 7095, Inst Astrophys Paris, F-75014 Paris, France

[17] Univ British Columbia, Dept Phys & Astron, 2329 West Mall, Vancouver, BC V6T 1Z4, Canada

[18] Univ Western Cape, Dept Phys & Astron, Robert Sobukwe Rd, ZA-7535 Cape Town, South Africa

[19] INAF Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy

[20] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA

[21] Univ Illinois, Dept Phys, 1002 W Green St, Urbana, IL 61801 USA

[22] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[23] SRON Netherlands Inst Space Res, Landleven 12, NL-9747 AD Groningen, Netherlands

[24] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark

[25] Univ Durham, Dept Phys, Ctr Extragalact Astron, South Rd, Durham DH1 3LE, England

来源：

ASTROPHYSICAL JOURNAL | 2016年 / 823卷 / 01期

基金：

英国科学技术设施理事会; 欧洲研究理事会; 美国国家科学基金会;

关键词：

galaxies: high-redshift; galaxies: starburst; gravitational lensing: strong; sub-millimeter: galaxies; ULTRALUMINOUS INFRARED GALAXIES; DEEP-FIELD-SOUTH; HIGH-REDSHIFT GALAXIES; SURVEY ALMA RESOLVES; BASE-LINE CAMPAIGN; CO EMISSION-LINES; SUBMILLIMETER GALAXIES; NUMBER COUNTS; STARBURST GALAXY; MOLECULAR GAS;

D O I：

10.3847/0004-637X/823/1/17

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a list of candidate gravitationally lensed dusty star-forming galaxies (DSFGs) from the HerMES Large Mode Survey and the Herschel Stripe 82 Survey. Together, these partially overlapping surveys cover 372 deg(2) on the sky. After removing local spiral galaxies and known radio-loud blazars, our candidate list of lensed DSFGs is composed of 77 sources with 500 mu m flux densities (S-500) greater than 100 mJy. Such sources are dusty starburst galaxies similar to the first bright sub-millimeter galaxies (SMGs) discovered with SCUBA. We expect a large fraction of this list to be strongly lensed, with a small fraction made up of bright SMG-SMG mergers that appear as hyper-luminous infrared galaxies (L-IR > 10(13) L-circle dot). Thirteen of the 77 candidates have spectroscopic redshifts from CO spectroscopy with ground-based interferometers, putting them at z > 1 and well above the redshift of the foreground lensing galaxies. The surface density of our sample is 0.21 +/- 0.03 deg(-2). We present follow-up imaging of a few of the candidates to confirm their lensing nature. The sample presented here is an ideal tool for higher-resolution imaging and spectroscopic observations to understand the detailed properties of starburst phenomena in distant galaxies.

引用

页数：22

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