A dataset provided by the European Space Agency

Name 069132
Title The nature of X-ray emission in BL Lac objects
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691320301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691320601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691320701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691320801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691320901

DOI 10.5270/esa-f21mx2e
Author Dr Francesco Massaro
Description The 77% of TeV extragalactic sources are BL Lacs. They belong to the High frequency peaked BL Lacs (HBLs) subclass characterized by a low-energy component with power peaking between the UV and the X-rays. We propose xmm~observations of a selected sample of HBLs, to study the spectral behavior of their optical to X-ray component. In addition, on the basis of our previous X-ray analyses of TeV e non TeV HBLs, these proposed xmm~observations will allow us to identify BL Lac candidates for future TeV observations.
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band . Arsioli, B., Chang, Y.-L., . A&A . 598-134 . 2017 . 2017A&A...598A.134A ,
Two new magnetic cataclysmic variables discovered in the 3XMM catalogue . Webb, N. A., Schwope, A., et all. . A&A . 615-133 . 2018 . 2018A&A...615A.133W ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-05-28T05:40:35Z/2013-01-09T02:51:21Z
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 2014-01-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-01-25T00:00:00Z, 069132, 17.56_20190403_1200. https://doi.org/10.5270/esa-f21mx2e