OBSERVATIONS OF 3C-273 WITH THE GODDARD HIGH-RESOLUTION SPECTROGRAPH ON THE HUBBLE SPACE TELESCOPE

被引：21

作者：

BRANDT, JC

HEAP, SR

BEAVER, EA

BOGGESS, A

CARPENTER, KG

EBBETS, DC

HUTCHINGS, JB

JURA, M

LECKRONE, DS

LINSKY, JL

MARAN, SP

SAVAGE, BD

SMITH, AM

TRAFTON, LM

WALTER, FM

WEYMANN, RJ

SNOW, M

RANDALL, CE

LINDLER, DJ

SHORE, SN

MORRIS, SL

GILLILAND, RL

LU, L

ROBINSON, RD

机构：

[1] NASA,GODDARD SPACE FLIGHT CTR,ASTRON & SOLAR PHYS LAB,CODE 681,GREENBELT,MD 20771

[2] UNIV CALIF SAN DIEGO,CTR ASTROPHYS & SPACE SCI,C-011,LA JOLLA,CA 92093

[3] NASA,GODDARD SPACE FLIGHT CTR,CODE 440,GREENBELT,MD 20771

[4] BALL AEROSP SYST GRP,BOULDER,CO 80306

[5] DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADA

[6] UNIV CALIF LOS ANGELES,DEPT ASTRON,LOS ANGELES,CA 90024

[7] NATL INST STAND & TECHNOL,DIV QUANTUM PHYS,BOULDER,CO 80309

[8] UNIV COLORADO & NATL INST STAND & TECHNOL,JOINT INST LAB ASTROPHYS,BOULDER,CO 80309

[9] NASA,GODDARD SPACE FLIGHT CTR,ASTRON & SOLAR PHYS LAB,CODE 680,GREENBELT,MD 20771

[10] UNIV WISCONSIN,DEPT AUGEN,MADISON,WI 53706

[11] UNIV TEXAS,MCDONALD OBSERV,AUSTIN,TX 78712

[12] UNIV TEXAS,DEPT ASTRON,AUSTIN,TX 78712

[13] SUNY STONY BROOK,STONY BROOK,NY 11794

[14] CARNEGIE INST WASHINGTON,OBSERV,PASADENA,CA 91101

[15] NASA,GODDARD SPACE FLIGHT CTR,COMP SCI CORP,CODE 681,GREENBELT,MD 20771

[16] SPACE TELESCOPE SCI INST,BALTIMORE,MD 21218

[17] UNIV WISCONSIN,DEPT ASTRON,MADISON,WI 53706

来源：

ASTRONOMICAL JOURNAL | 1993年 / 105卷 / 03期

关键词：

D O I：

10.1086/116475

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The observations of the quasar 3C 273 taken with the Goddard High Resolution Spectrograph in 1991 February are presented here. We have included both the reduced raw data, and smoothed and deconvolved spectra. Also, a list of observed absorption lines is presented. The data comprise 11 spectra, including 1 low resolution observation and 10 medium resolution observations. The wavelength region covered ranged from about 1150 to 2820 angstrom, but was not all inclusive. The procedures used to obtain and reduce the data, including corrections for fixed pattern noise, compensation for the effects of spherical aberration in the HST primary mirror, and objective detection of weak absorption lines, are described. We also have included a short discussion on the detection of galactic Ni II and Virgo cluster metal lines.

引用

页码：831 / 846

页数：16

共 21 条

[11] ITERATIVE TECHNIQUE FOR RECTIFICATION OF OBSERVED DISTRIBUTIONS [J].