A dataset provided by the European Space Agency

Name 060012
Title Triggered Observations of a LAT Monitored Blazar in Quiescence
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600121401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600121501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600121601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600121701

DOI https://doi.org/10.5270/esa-jma612s
Author Prof Markus Boettcher
Description Most multiwavelength campaigns on blazars are triggered by a flaring state. Because of this strategy and the difficulty of measuring spectra and variability of blazars in low states, the quiescent states of blazars are poorly understood. XMM-Newton, in combination with Fermi-LAT, now offers the opportunity to do such studies. For this reason, we propose triggered observations of a blazar on the list of Fermi-LAT Monitored Blazars in quiescence, which we define as a Fermi-LAT detected flux above 100 MeV smaller than the lowest flux or upper limit ever measured by EGRET, for at least one week. 80 ksec of XMM-Newton exposure will be coordinated with intensive monitoring by the WEBT to obtain simultaneous radio through gamma-ray coverage.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-09-08T06:10:15Z/2009-09-14T14:07:16Z
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 2010-11-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-11-17T00:00:00Z, 060012, 17.56_20190403_1200. https://doi.org/10.5270/esa-jma612s