A dataset provided by the European Space Agency

Name 014800
Title Exploring the X-ray emission mechanism in the variable Seyfert 1, 1H 0419-577
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148000201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148000301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148000401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148000501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148000601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148000701

DOI 10.5270/esa-9kpw74k
Author Prof Ken Pounds
Description A brief 8 ksec observation of the bright Seyfert 1 1H 0419-577 early in the XMM mission showed the source to be a considerably brighter state (by a factor of 10) than 4 years earlier. Our first aim is to employ the full spectroscopic capability of XMM-Newton, in a repeated and longer (50 ksec) observation. Past observations of 1H 0419 show it to be a unique object, switching between low-hard and high-soft spectral states, analogous to the Galactic black hole sources. Our second objective is to monitor 1H 0419-577 (visible throughout the whole of the AO-2 period) with a series of 15 ksec observations, to constrain the timescale of the change of state and to follow its spectral evolution. We hope this will yield new insights into the emission mechanism in AGN.
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 ,
Evidence for ultra-fast outflows in radio-quiet AGNs. I. Detection and statistical incidence of Fe K-shell absorption lines . Tombesi, F., Cappi, M., et all. . A&A . 521-57 . 2010 . 2010A&A...521A..57T ,
Evidence for Ultra-fast Outflows in Radio-quiet Active Galactic Nuclei. II. Detailed Photoionization Modeling of Fe K-shell Absorption Lines . Tombesi, F., Cappi, M., et all. . ApJ . 742-44 . 2011 . 2011ApJ...742...44T ,
An XMM-Newton Observation of the Seyfert 1 Galaxy 1H 0419-577 in an Extreme Low State . Pounds, K. A., Reeves, J. N., et all. . ApJ . 605-670 . 2004 . 2004ApJ...605..670P ,
Resolving the Large-Scale Spectral Variability of the Luminous Seyfert 1 Galaxy 1H 0419-577: Evidence for a New Emission Component and Absorption by Cold Dense Matter . Pounds, K. A., Reeves, J. N., et all. . ApJ . 616-696 . 2004 . 2004ApJ...616..696P ,
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-09-25T18:02:42Z/2003-11-15T11:27:17Z
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 2005-01-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-01-01T00:00:00Z, 014800, 17.56_20190403_1200. https://doi.org/10.5270/esa-9kpw74k