A dataset provided by the European Space Agency

Name 010666
Title XMM GT observation of a Broad Absorption Line Quasars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106660701

DOI 10.5270/esa-zdczlrj
Author Dr Jean Clavel
Description GT- We propose to observe the Broad-Absorption Line (BAL) Quasar LBQS~2212-1759 with XMM. This is one of the few BALQSO detected with ROSAT with a PSPC count rate of 0.049+--0.002 cts-s. A 50 ks exposure time yields ~ 22,000 cts with EPIC-pn (thin) and 850 cts with one RGS, i.e. a S-N ratio of ~ 3 per 10~ev channel when combining both RGS and all orders. The spectra will be used to measure the X-ray absorption, compare it with the optical absorbing column and infer the physical conditions of the BAL gas.
Publication An XMM-Newton study of the hard X-ray sky . Piconcelli, E., Cappi, M., et all. . A&A . 412-689 . 2003 . 2003A&A...412..689P ,
Exploring the X-ray sky with the XMM-Newton bright serendipitous survey . Della Ceca, R., Maccacaro, T., et all. . A&A . 428-383 . 2004 . 2004A&A...428..383D ,
Long observations of the BALQSO LBQS 2212-1759 with XMM-Newton . Clavel, J., Schartel, N., . A&A . 446-439 . 2006 . 2006A&A...446..439C ,
Identifying XMM-Newton observations affected by solar wind charge exchange - Part II . Carter, J. A., Sembay, S., . A&A . 527-115 . 2011 . 2011A&A...527A.115C ,
High-precision multi-band measurements of the angular clustering of X-ray sources . Ebrero, J., Mateos, S., et all. . A&A . 500-749 . 2009 . 2009A&A...500..749E ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
The XMM-Newton Wide Angle Survey (XWAS): the X-ray spectrum of type-1 AGN . Mateos, S., Carrera, F. J., et all. . A&A . 510-35 . 2010 . 2010A&A...510A..35M ,
Average Fe Kalpha emission from distant AGN . Corral, A., Page, M. J., et all. . A&A . 492-71 . 2008 . 2008A&A...492...71C ,
X-ray absorption in distant type II QSOs . Krumpe, M., Lamer, G., et all. . A&A . 483-...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-11-17T15:39:07Z/2001-11-19T04:51:47Z
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 2003-02-19T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-02-19T00:00:00Z, 010666, 17.56_20190403_1200. https://doi.org/10.5270/esa-zdczlrj