The European Large Area ISO Survey -: VI.: Discovery of a new hyperluminous infrared galaxy

被引：17

作者：

Morel, T

Efstathiou, A

Serjeant, S

Márquez, I

Masegosa, J

Héraudeau, P

Surace, C

Verma, A

Oliver, S

Rowan-Robinson, M

Georgantopoulos, I

Farrah, D

Alexander, DM

Pérez-Fournon, I

Willott, CJ

Cabrera-Guerra, F

Gonzalez-Solares, EA

Cabrera-Lavers, A

Gonzalez-Serrano, JI

Ciliegi, P

Pozzi, F

Matute, I

Flores, H

机构：

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

[2] Univ Kent, Sch Phys Sci, Unit Space Sci & Astrophys, Canterbury CT2 7NR, Kent, England

[3] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain

[4] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[5] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany

[6] Univ Sussex, Ctr Astron, Brighton BN1 9QJ, E Sussex, England

[7] Natl Observ Athens, Astron Inst, GR-15236 Athens, Greece

[8] SISSA, Int Sch Adv Studies, I-34014 Trieste, Italy

[9] Penn State Univ, Davey Lab, University Pk, PA 16802 USA

[10] Inst Astrofis Canarias, Tenerife 38200, Canary Islands, Spain

[11] Univ Oxford, Dept Phys, Oxford OX1 3RH, England

[12] Univ Cantabria, Fac Ciencias, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain

[13] Osservatorio Astron Bologna, I-40127 Bologna, Italy

[14] Univ Studi Roma TRE, Dipartimento Fis, I-00146 Rome, Italy

[15] CEA Saclay, F-91191 Gif Sur Yvette, France

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2001年 / 327卷 / 04期

关键词：

surveys; quasars : individual : ELAISP90_J164010+410502 ([CCS88; 163831.4+411107); galaxies : starburst; infrared : galaxies;

D O I：

10.1046/j.1365-8711.2001.04803.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the discovery of the first hyperluminous infrared galaxy (HyLIG) in the course of the European Large Area ISO Survey (ELAIS). This object has been detected by ISO at 6.7, 15 and 90 mum, and is found to be a broad-line, radio-quiet quasar at a redshift z=1.099. From a detailed multicomponent model fit of the spectral energy distribution, we derive a total IR luminosity L-IR (1-1000 mum) approximate to 1.0 x 10(13) h(65)(-2) L-circle dot (q(0) = 0.5), and discuss the possible existence of a starburst contributing to the far-IR output. Observations to date present no evidence for lens magnification. This galaxy is one of the very few HyLIGs with a X-ray detection. On the basis of its soft X-ray properties, we suggest that this broad-line object may be the face-on analogue of narrow-line, Seyfert-like HyLIGs.

引用

页码：1187 / 1192

页数：6

共 47 条

[1] Detection of CO (3-2) emission at z=2.64 from the gravitationally lensed quasar MG 0414+0534 [J].