A dataset provided by the European Space Agency

Name 011409
Title EPIC mode and pile-up dependence - PKS0537


DOI 10.5270/esa-0c3uzmp
Author Dr Fred Jansen XMM-Newton PS
Description CAL- The effect of changing count rates on the spectral responce is measured by observing similar AGN spectra at a range of fluxes. New proposal for observations on PKS0537 in replacement of PG1634+706 (propId = 10252), which was lacking visibility with XMM.
Publication PKS 0537-286, carrying the information of the environment of SMBHs in the early Universe . Bottacini, E., Ajello, M., et all. . A&A . 509-69 . 2010 . 2010A&A...509A..69B ,
XMM-Newton spectroscopy of high-redshift quasars . Page, K. L., Reeves, J. N., et all. . MNRAS . 364-195 . 2005 . 2005MNRAS.364..195P ,
The first XMM-Newton spectrum of a high redshift quasar - PKS 0537-286 . Reeves, J. N., Turner, M. J. L., et all. . A&A . 365-116 . 2001 . 2001A&A...365L.116R ,
The HELLAS2XMM survey. IV. Optical identifications and the evolution of the accretion luminosity in the Universe . Fiore, F., Brusa, M., et all. . A&A . 409-79 . 2003 . 2003A&A...409...79F ,
The HELLAS2XMM survey. V. Near-Infrared observations of X-ray sources with extreme X-O ratios . Mignoli, M., Pozzetti, L., et all. . A&A . 418-827 . 2004 . 2004A&A...418..827M ,
The HELLAS2XMM survey. VI. X-ray absorption in the 1df AGN sample through a spectral analysis . Perola, G. C., Puccetti, S., et all. . A&A . 421-491 . 2004 . 2004A&A...421..491P ,
The HELLAS2XMM Survey. I. The X-Ray Data and the logN-logS Relation . Baldi, A., Molendi, S., et all. . ApJ . 564-190 . 2002 . 2002ApJ...564..190B ,
The Resolved Fraction of the Cosmic X-Ray Background . Moretti, A., Campana, S., et all. . ApJ . 588-696 . 2003 . 2003ApJ...588..696M , ...
Instrument EMOS1, EMOS2, EPN, OM
Temporal Coverage 2000-03-19T12:11:49Z/2000-03-20T02:55:52Z
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 2003-03-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-03-02T00:00:00Z, 011409, 17.56_20190403_1200. https://doi.org/10.5270/esa-0c3uzmp