A dataset provided by the European Space Agency

Name 030319
Title A Modern Quasar SED from XMM-Newton, Spitzer, and SDSS


DOI 10.5270/esa-0cz1gzt
Author Dr Gordon Richards
Description We request 7 XMM-Newton pointings in the field of the Spitzer First Look Survey to obtain uniform X-ray data on 100 quasars, including 10 luminous, type I quasars from the Sloan Digital Sky Survey. With 14.0 ks exposures (98.0 ks total), we will obtain more than 500 counts on each of the 10 luminous quasars and at least 40 counts on 100 other quasars in the field of view. We will characterize the X-ray, UV, optical, IR, and radio SED of quasars as a function of various properties, thus permitting better estimates of bolometric luminosity, black hole mass, and accretion rate in addition to providing better observational templates for comparison with accretion disk models.
Publication The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS . 463-4490 . 2016 . 2016MNRAS.463.4490C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 . Pons, E., Watson, M. G., . A&A . 594-72 . 2016 . 2016A&A...594A..72P ,
Dependence of the broad Fe Kalpha line on the physical parameters of AGN . Liu, Zhu, Yuan, Weimin, et all. . MNRAS . 463-684 . 2016 . 2016MNRAS.463..684L ,
Eight-Dimensional Mid-Infrared-Optical Bayesian Quasar Selection . Richards, Gordon T., Deo, Rajesh P., et all. . AJ . 137-3884 . 2009 . 2009AJ....137.3884R ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-03-31T20:06:07Z/2006-04-01T03:22:16Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2007-05-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-05-05T00:00:00Z, 030319, 17.56_20190403_1200. https://doi.org/10.5270/esa-0cz1gzt