A dataset provided by the European Space Agency

Name 020267
Title UNDERSTANDING THE HIGH ENERGY FLARING ACTIVITY OF THE GALACTIC NUCLEUS
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0202670501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0202670601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0202670701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0202670801

DOI 10.5270/esa-k7eg6by
Author Dr ANDREA GOLDWURM
Description We propose to carry out a large (550 ks) XMM-Newton monitoring program of Sgr A ^* , the radiative manifestation of the putative massive black hole at the galactic center, to study in detail the broad band spectrum and timing properties of the source during its X-ray flaring activity. The program will be performed in coordination with INTEGRAL gamma-ray observations of the galactic center and with observations at lower frequencies. Although the galactic nucleus hosts the nearest and probably best studied massive black hole its physical and radiative properties and in particular its low level of high energy emission are still little understood. The discovery of bright X-ray flares from Sgr~A* with Chandra and XMM-Newton
Publication X-ray hiccups from Sagittarius A* observed by XMM-Newton. The second brightest flare and three moderate flares caught in half a day . Porquet, D., Grosso, N., et all. . A&A . 488-549 . 2008 . 2008A&A...488..549P ,
Discovery of a Superluminal Fe K Echo at the Galactic Center: The Glorious Past of Sgr A* Preserved by Molecular Clouds . Ponti, G., Terrier, R., et all. . ApJ . 714-732 . 2010 . 2010ApJ...714..732P ,
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 ,
Bursting behavior of the Galactic center faint X-ray transient GRS 1741.9-2853 . Trap, G., Falanga, M., et all. . A&A . 504-501 . 2009 . 2009A&A...504..501T ,
Discovery of X-ray eclipses from the transient source CXOGC J174540.0-290031 with XMM-Newton . Porquet, D., Grosso, N., et all. . A&A . 443-571 . 2005 . 2005A&A...443..571P ,
Repeated X-Ray Flaring Activity in Sagittarius A* . Belanger, G., Goldwurm, A., et all. . ApJ . 635-1095...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-03-28T15:03:52Z/2004-09-03T16:35:35Z
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 2006-05-19T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-05-19T00:00:00Z, 020267, 17.56_20190403_1200. https://doi.org/10.5270/esa-k7eg6by