A dataset provided by the European Space Agency

Name 020100
Title AN XMM-NEWTON MONITORING CAMPAIGN OF THE ACCRETION FLOW IN IGRJ16318-4848
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201000201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201000301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201000401

DOI 10.5270/esa-9uhspg7
Author Dr MATTEO GUAINAZZI
Description The prominent, large equivalent width Fe K-alpha, Fe K-beta, and Ni K-beta fluorescent emission lines in the X-ray spectrum of IGRJ16138-4848 represent an almost unique laboratory to study the conditions of the accretion flows in binary systems. There is evidence for changes of the quantities defining the accretion flow on different timescales, possibly related to the overall X-ray output. We propose a monitoring campaign of IGRJ16138-4848 during the XMM-Newton AO3, in order to study the relation between the X-ray output and the physical state of the accreting matter, and the evolution of the accretion flow geometry, distribution and covering factor. We request 4 observations, covering timescales from days to months, for a total allocation time of 80 ks.
Publication 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 ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
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-INTEGRAL monitoring campaign of IGR J16318-4848 . Ibarra, A., Matt, G., et all. . A&A . 465-501 . 2007 . 2007A&A...465..501I ,
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations . Muno, M. P., Gaensler, B. M., et all. . ApJ . 680-639 . 2008 . 2008ApJ...680..639M ,
The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population . Warwick, R. S., Perez-Ramirez, D., . MNRAS . 413-595 . 2011 . 2011MNRAS.413..595W ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
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 win...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-02-18T02:19:51Z/2004-08-20T10:12:17Z
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 2005-09-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-09-09T00:00:00Z, 020100, 17.56_20190403_1200. https://doi.org/10.5270/esa-9uhspg7