A dataset provided by the European Space Agency

Name 050203
Title Rapid Flares from TeV Blazars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502030101

DOI 10.5270/esa-c2k9xfr
Author Prof Wei Cui
Description We propose to observe a known TeV blazar in outburst. The observation will be supported by coordinated ground-based observations at TeV energies. The main thrust of the proposed observation is to study the flaring phenomenon on sub-hour timescales jointly at X-ray and TeV energies. XMM covers a critical spectral range for studying TeV blazars, because the SED of such sources peaks in or near its passing band. The data will also allow investigations of correlated variability of the X-ray and TeV emission, spectral hysteresis, and hardness-intensity correlation. The results may shed significant light on the properties of emitting regions in the jet of TeV blazars, emission mechanisms, and the composition of the jet (i.e., leptonic vs hadronic).
Publication Simultaneous Multiwavelength Observations of Markarian 421 During Outburst . Acciari, V. A., Aliu, E., et all. . ApJ . 703-169 . 2009 . 2009ApJ...703..169A ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Detecting the Warm-Hot Intergalactic Medium through X-Ray Absorption Lines . Yao, Yangsen, Shull, J. Michael, et all. . ApJ . 746-166 . 2012 . 2012ApJ...746..166Y ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues . Vagnetti, F., Turriziani, S., . A&A . 536-84 . 2011 . 2011A&A...536A..84V ,
Properties of the integrated spectrum of serendipitous 2XMM catalog sources . Chaudhary, P., Brusa, M., et all. . A&A . 518-58 . 2010 . 2010A&A...518A..58C ,
Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line . Chaudhary, P., Brusa, M., et all. . A&A . 537-6 . 2012 . 2012A&A...537A...6C ,
A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
Insight into Active Galactic Nucleus and Host Galaxy Co...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-05-07T01:34:05Z/2008-05-07T13:34:25Z
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 2009-06-19T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-06-19T00:00:00Z, 050203, 17.56_20190403_1200. https://doi.org/10.5270/esa-c2k9xfr