Published June 20, 2015 | Version v1
Journal article Metadata-only

Ultraviolet/X-ray variability and the extended X-ray emission of the radio-loud broad absorption line quasar PG 1004+130

Creators

  • 1. Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802 (United States)
  • 2. Department of Chemistry and Physical Sciences, The College of St. Scholastica, Duluth, MN 55811 (United States)
  • 3. Department of Physics and Astronomy, University of Western Ontario, London, ON, N6A 3K7 (Canada)

Description

We present the results of recent Chandra, XMM-Newton, and Hubble Space Telescope observations of the radio-loud (RL), broad absorption line (BAL) quasar PG 1004+130. We compare our new observations to archival X-ray and UV data, creating the most comprehensive, high signal-to-noise, multi-epoch, spectral monitoring campaign of a RL BAL quasar to date.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/806/2/210

Additional details

Identifiers

DOI
10.1088/0004-637X/806/2/210;

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
806
Journal Issue
2
Journal Page Range
[15 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
51041703
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ABSORPTION; EMISSION; MONITORING; NOISE; QUASARS; SIGNALS; SPACE; TELESCOPES; ULTRAVIOLET RADIATION; X RADIATION; X-RAY GALAXIES
Descriptors DEC
COSMIC RADIO SOURCES; COSMIC RAY SOURCES; COSMIC X-RAY SOURCES; ELECTROMAGNETIC RADIATION; GALAXIES; IONIZING RADIATIONS; RADIATIONS; SORPTION