A dataset provided by the European Space Agency

Name 015896
Title Simultaneous XMM-Chandra Observations of PKS2155-304
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158960101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158960901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158961001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158961101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158961201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158961301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158961401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0158961501

DOI 10.5270/esa-i0q5q86
Author Mr Fred Jansen XMM-Newton PM
Description Cross-calibration with Chandra is important and best done on simultaneous observations of objects with smooth continua as the whole of the detectors are illuminated. The proposed observation is part of the Chandra effort to understand the significant build-up of ACIS contamination. A simultaneous observation will help both us and them. They are planning a single 30ks ACIS-S + LETG observation this time numbered 4416 in the Chandra long-term schedule.
Publication A ~4.6 h quasi-periodic oscillation in the BL Lacertae PKS 2155-304? . Lachowicz, P., Gupta, A. C., et all. . A&A . 506-17 . 2009 . 2009A&A...506L..17L ,
Extinction and Distance to Anomalous X-ray Pulsars from X-ray Scattering Halos . Rivera-Ingraham, A., van Kerkwijk, M. H., . ApJ . 710-797 . 2010 . 2010ApJ...710..797R ,
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 ,
Cross Spectral Calibration of Suzaku, XMM-Newton, and Chandra with PKS 2155-304 as an Activity of IACHEC . Ishida, Manabu, Tsujimoto, Masahiro, et all. . PASJ . 63-657 . 2011 . 2011PASJ...63S.657I ,
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 ,
Detection of Intra-day Variability Timescales of Four High-energy Peaked Blazars with XMM-Newton . Gaur, Haritma, Gupta, Alok C., et all. . ApJ . 718-279 . 2010 . 2010ApJ...718..279G ,
Modelling the spectral response of the Swift-XRT CCD camera: experience learnt from in-flight calibration . Godet, O., Beardmore, A. P., et all. . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-11-23T00:46:22Z/2006-05-02T06:26:09Z
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 2006-05-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-05-02T00:00:00Z, 015896, 17.56_20190403_1200. https://doi.org/10.5270/esa-i0q5q86