The Hubble Deep Field South: STIS imaging

被引：43

作者：

Gardner, JP

Baum, SA

Brown, TM

Carollo, CM

Christensen, J

Dashevsky, I

Dickinson, ME

Espey, BR

Ferguson, HC

Fruchter, AS

Gonnella, AM

Gonzalez-Lopezlira, RA

Hook, RN

Kaiser, ME

Martin, CL

Sahu, KC

Savaglio, S

Smith, TE

Teplitz, HI

Williams, RE

Wilson, J

机构：

[1] NASA, Goddard Space Flight Ctr, Astron & Solar Phys Lab, Greenbelt, MD 20771 USA

[2] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[3] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[4] Space Telescope European Coordinating Facil, D-85748 Garching, Germany

来源：

ASTRONOMICAL JOURNAL | 2000年 / 119卷 / 02期

关键词：

cosmology : observations; galaxies : evolution; galaxies : statistics; surveys;

D O I：

10.1086/301215

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the imaging observations made with the Space Telescope Imaging Spectrograph (STIS) of the Hubble Deep Field South. The field was imaged in four bandpasses: a clear CCD bandpass for 156 ks, a long-pass filter for 22-25 ks pixel(-1) typical exposure, a near-UV bandpass for 23 ks, and a far-UV bandpass for 52 ks. The clear, visible image is the deepest observation ever made in the UV-optical wavelength region, reaching a 10 sigma AB magnitude of 29.4 for an object of area 0.2 arcsec(2). The field contains QSO J2233-606, the target of the STIS spectroscopy, and extends 50 " x 50 " for the visible images, and 25 " x 25 " for the ultraviolet images. We present the images, catalog of objects, and galaxy counts obtained in the field.

引用

页码：486 / 508

页数：23

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