A dataset provided by the European Space Agency

Name 050514
Title Outflow variability and black hole occultation in NGC 1365
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505140201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505140401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505140501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505140601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505140701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505140801

DOI 10.5270/esa-60097fr
Author Dr Guido Risaliti
Description We propose a 360 ksec observation of the Seyfert Galaxy NGC 1365, a source having a unique set of properties, which make it the best suited target among X-ray absorbed AGNs to study the innermost region of AGNs: FeXXV and FeXXVI Kalpha and Kbeta absorption lines (the highest S-N detection so far among AGNs), rapidly varying cold absorber (N_H variations of ~10^{23}cm^{-2} in a few hours, changes from Compton-thick to Compton-thin in two days), a relativistic iron emission line. This new long observation will constrain the dimensions of the absorbers, and, for the first time, allow the investigation of the dynamics and physical conditions of the hot absorber responsible of the iron absorption lines.
Publication The XMM-NEWTON Long Look of NGC 1365: Lack of a High-Soft State in its Ultraluminous X-Ray Sources . Soria, R., Risaliti, G., et all. . ApJ . 695-1614 . 2009 . 2009ApJ...695.1614S ,
Variable Partial Covering and A Relativistic Iron Line in NGC 1365 . Risaliti, G., Miniutti, G., et all. . ApJ . 696-160 . 2009 . 2009ApJ...696..160R ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
The XMM-Newton long look of NGC 1365: uncovering of the obscured X-ray source . Risaliti, G., Salvati, M., et all. . MNRAS . 393-1 . 2009 . 2009MNRAS.393L...1R ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
AGN-starburst connection in action: the half million second RGS spectrum of NGC 1365 . Guainazzi, M., Risaliti, G., et all. . A&A . 505-589 . 2009 . 2009A&A...505..589G ,
A new technique to efficiently select Compton-thick AGN . Severgnini, P., Caccianiga, A., . A&A . 542-46 . 2012 . 2012A&A...542A..46S ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-06-30T07:08:06Z/2007-07-05T20:25:40Z
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 2009-01-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-01-20T00:00:00Z, 050514, 17.56_20190403_1200. https://doi.org/10.5270/esa-60097fr