A dataset provided by the European Space Agency

Name 055623
Title Variable absorption in BAL QSOs: catching the origin of AGN winds
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556230101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556230201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556230701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556231001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556231101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556231201

DOI 10.5270/esa-a29zs04
Author Dr Margherita Giustini
Description We want to investigate the nature of the gas located in the central regions of QSOs. Hence, we propose to observe a small sample of four BAL QSOs, among the X-ray brightest in the Palomar Green sample. Our goal is to monitor the variability of their absorption properties to study the physics of the wind seen in BAL QSOs along the line of sight. As such, timescales of days and years must be investigated to probe distances between tens to thousands gravitational radii from the central SMBH. To this end, each source must have been observed at least three times by XMM-Newton (in at least 2 close pointings for the intra-day variability plus a distant one for the intra-year variability). We thus request that XMM-Newton re-observes some BAL QSOs for a total of 240 ks.
Publication Variable X-ray absorption in the mini-BAL QSO PG 1126-041 . Giustini, M., Cappi, M., et all. . A&A . 536-49 . 2011 . 2011A&A...536A..49G ,
A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 . Georgakakis, Antonis, Nandra, K., . MNRAS . 414-992 . 2011 . 2011MNRAS.414..992G ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
CAIXA: a catalogue of AGN in the XMM-Newton archive. III. Excess variance analysis . Ponti, G., Papadakis, I., et all. . A&A . 542-83 . 2012 . 2012A&A...542A..83P ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
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 ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-06-08T11:55:29Z/2008-12-13T23:23:47Z
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 2010-01-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-01-17T00:00:00Z, 055623, 17.56_20190403_1200. https://doi.org/10.5270/esa-a29zs04