Observations of the Hubble Deep Field with the Infrared Space Observatory .4. Association of sources with Hubble Deep Field galaxies

被引：42

作者：

Mann, RG

Oliver, SJ

Serjeant, SBG

RowanRobinson, M

Baker, A

Eaton, N

Efstathiou, A

Goldschmidt, P

Mobasher, B

Sumner, TJ

Danese, L

Elbaz, D

Franceschini, A

Egami, E

Kontizas, M

Lawrence, A

McMahon, R

NorgaardNielsen, HU

PerezFournon, I

GonzalezSerrano, JI

机构：

[1] SERV ASTROPHYS, F-91191 GIF SUR YVETTE, FRANCE

[2] SISSA, I-34014 TRIESTE, ITALY

[3] OSSERV ASTRON PADOVA, I-35122 PADUA, ITALY

[4] MAX PLANCK INST EXTRATERR PHYS, D-37075 GARCHING, GERMANY

[5] NATL OBSERV ATHENS, ASTRON INST, GR-11810 ATHENS, GREECE

[6] UNIV EDINBURGH, INST ASTRON, EDINBURGH EH9 3HJ, MIDLOTHIAN, SCOTLAND

[7] UNIV CAMBRIDGE INST ASTRON, INST ASTRON, CAMBRIDGE CB3 0HA, ENGLAND

[8] DANISH SPACE RES INST, DK-2800 LYNGBY, COPENHAGEN, DENMARK

[9] INST ASTROFIS CANARIAS, E-38200 LA LAGUNA, TENERIFE, SPAIN

[10] INST FIS CANTABRIA, SANTANDER, SPAIN

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1997年 / 289卷 / 02期

关键词：

galaxies; evolution; starburst; infrared;

D O I：

10.1093/mnras/289.2.482

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 mu m in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches, We find 15 ISO sources to be reliably associated with bright [I-814(AB) < 23] galaxies in the HDF, and one with an I-814(AB)=19.9 star, while a further 11 are associated with objects in the Hubble Flanking Fields (10 galaxies and one star), Amongst optically bright HDF galaxies, ISO tends to detect luminous, star-forming galaxies at fairly high redshift and with disturbed morphologies, in preference to nearby ellipticals.

引用

页码：482 / 489

页数：8

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