A dataset provided by the European Space Agency

Name 016096
Title Timing verification with the Crab
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160960901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160961001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160961101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160961201
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160961301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160961401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0160961501

DOI 10.5270/esa-t1xoxs1
Author Mr Fred Jansen XMM-Newton PS
Description In order to verify the absolute timing there is the opportunity to contemporaneously observe the Crab with Chandra and in the optical using an MPE developed fast photometer to get a radio-ephemeris independent phase solution between the optical and X-ray pulses. The optical (and Chandra) observation are scheduled for ~ September 26. Since the accuracy of determining the pulse period is correlated with the total range of the observation we propose to perform 2 observations of 10 ks in up to three consecutive orbits, in order to have a long time base line. For the pn the electronic chopper might be required in order to avoid counting mode. This will be arranged via OCR if needed. Obs. greater equal 04 are routine cal. 3x5 ks in single orbit.
Publication On Calibrations Using the Crab Nebula and Models of the Nebular X-Ray Emission . Weisskopf, M. C., Guainazzi, M., et all. . ApJ . 713-912 . 2010 . 2010ApJ...713..912W ,
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 ,
Modelling the spectral response of the Swift-XRT CCD camera: experience learnt from in-flight calibration . Godet, O., Beardmore, A. P., et all. . A&A . 494-775 . 2009 . 2009A&A...494..775G ,
The relative and absolute timing accuracy of the EPIC-pn camera on XMM-Newton, from X-ray pulsations of the Crab and other pulsars . Martin-Carrillo, A., Kirsch, M. G. F., et all. . A&A . 545-126 . 2012 . 2012A&A...545A.126M ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
The soft component and the iron line as signatures of the disc inner radius in Galactic black hole binaries . Kolehmainen, Mari, Done, Chris, . MNRAS . 437-316 . 2014 . 2014MNRAS.437..316K ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-10-01T11:48:26Z/2006-03-02T03:57:19Z
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 2006-03-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-03-04T00:00:00Z, 016096, 17.56_20190403_1200. https://doi.org/10.5270/esa-t1xoxs1