A dataset provided by the European Space Agency

Name 012270
Title EPIC Effective Area vs. Energy (G21.5-09)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122701001

DOI 10.5270/esa-8f9d9e9
Author Dr Fred Jansen XMM-Newton PS
Description CAL- Supplementing the 3C58 calibration, we use the SNR G21.5-09 which has a slightly steeper slope, but similar count rate. Offsets in the Z-direction are used to complement the 3C58 vignetting data, while avoiding bright stars.
Publication Timing analysis of the core of the Crab-like SNR G21.5-0.9 . La Palombara, N., Mereghetti, S., . A&A . 383-916 . 2002 . 2002A&A...383..916L ,
The nature of the X-ray halo of the plerion G21.5-0.9 unveiled by XMM-Newton and Chandra . Bocchino, F., van der Swaluw, E., et all. . A&A . 442-539 . 2005 . 2005A&A...442..539B ,
Cross-calibration of the X-ray instruments onboard the Chandra, INTEGRAL, RXTE, Suzaku, Swift, and XMM-Newton observatories using G21.5-0.9 . Tsujimoto, M., Guainazzi, M., et all. . A&A . 525-25 . 2011 . 2011A&A...525A..25T ,
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 ,
The missing link: a low-mass X-ray binary in M31 seen as an ultraluminous X-ray source . Middleton, Matthew J., Sutton, Andrew D., et all. . MNRAS . 420-2969 . 2012 . 2012MNRAS.420.2969M ,
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 ,
A Multiwavelength Study on the High-energy Behavior of the Fermi-LAT Pulsars . Marelli, Martino, De Luca, Andrea, . ApJ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-04-07T12:36:39Z/2001-04-09T22:25:05Z
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 2003-08-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-08-08T00:00:00Z, 012270, 17.56_20190403_1200. https://doi.org/10.5270/esa-8f9d9e9