A dataset provided by the European Space Agency

Name 015049
Title flaring blazars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150495601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150498701

DOI 10.5270/esa-p8kgt6r
Author Dr gianpiero tagliaferri
Description We ask for 3 blocks of 50 ks each to observe in Triggered Observation mode up to 3 blazars, conditional to stringent and well defined triggering criteria based on optical brightening or X-ray brightening or detection in the TeV band. The XMM-Newton satellite, with its high throughput and good spectral resolution, is crucial for determining the spectral distribution and its time evolution for blazars in a flaring state, and thus for constraining any emission model.
Publication Disentangling the synchrotron and inverse Compton variability in the X-ray emission of the intermediate BL Lacertae object S5 0716+71 . Ferrero, E., Wagner, S. J., et all. . A&A . 457-133 . 2006 . 2006A&A...457..133F ,
Signatures of synchrotron emission and of electron acceleration in the X-ray spectra of Mrk 421 . Tramacere, A., Massaro, F., . A&A . 466-521 . 2007 . 2007A&A...466..521T ,
On the Putative Detection of z > 0 X-Ray Absorption Features in the Spectrum of Mrk 421 . Rasmussen, Andrew P., Kahn, Steven M., et all. . ApJ . 656-129 . 2007 . 2007ApJ...656..129R ,
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 ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
Studying the X-ray-UV Variability of Active Galactic Nuclei with data from Swift and XMM archives . Turriziani, Sara, . JPhCS . 280-12005 . 2011 . 2011JPhCS.280a2005T ,
New constraints on the X-ray spectral properties of type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., et all. . MNRAS . 417-992 . 2011 . 2011MNRAS.417..992S ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-11-14T16:14:04Z/2004-04-05T05:42:13Z
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 2005-05-13T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-05-13T00:00:00Z, 015049, 17.56_20190403_1200. https://doi.org/10.5270/esa-p8kgt6r