Image deconvolution of the radio ring PKS 1830-211

被引：25
作者：
Courbin, F
Lidman, C
Frye, BL
Magain, P
Broadhurst, TJ
Pahre, MA
Djorgovski, SG
机构：
[1] Univ Liege, Inst Astrophys & Geophys, B-4000 Liege, Belgium
[2] Observ Paris, URA 173 CNRS, DAEC, Paris, France
[3] European So Observ, Santiago 19, Chile
[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[5] CALTECH, Palomar Observ, Pasadena, CA 91125 USA
来源：
ASTROPHYSICAL JOURNAL | 1998年 / 499卷 / 02期
基金：
美国国家航空航天局; 美国国家科学基金会;
关键词：
cosmology; observations; gravitational lensing; infrared; general methods; data analysis; quasars; individual; (PKS; 1830-211); techniques; image processing;
D O I：
10.1086/311376
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
New high-quality Keck and ESO images of PKS 1830-211 are presented. By applying a powerful new deconvolution algorithm to these optical and infrared data, both images of the flat spectrum core of the radio source have been identified. An extended source is also detected in the optical images which is consistent with the expected location of the lensing galaxy. The source counterparts are very red at I - K similar to 7, which suggests strong Galactic absorption with additional absorption by the lensing galaxy at z = 0.885 and is consistent with the detection of high-redshift molecules in the lens.
引用
收藏
页码：L119 / L123
页数：5
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