A dataset provided by the European Space Agency

Name 013452
Title AB Dor: RGS wavelength scale calibrations (RC)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134520301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134520401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134520501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134520601
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134522401

DOI 10.5270/esa-te3l773
Author Dr Fred Jansen XMM-Newton PS
Description Routine Calibration - RGS wavelength scale, use obs 10 or 11 for standard setup Obs #18: RGS cooling A rev 532 Obs #17: RGS Cooling B rev 537 Obs #20: RGS Cooling C rev 546 obs #21: RC rev 560 obs #22: RC rev 571 obs #23: RC rev 604 obs #24: RC rev 636 obs #25 and #26: RC rev 667
Publication Three years in the coronal life of AB Dor. I. Plasma emission measure distributions and abundances at different activity levels . Sanz-Forcada, J., Maggio, A., . A&A . 408-1087 . 2003 . 2003A&A...408.1087S ,
High mass X-ray binaries in the LMC: Dependence on the stellar population age and the ''propeller.. effect . Shtykovskiy, P., Gilfanov, M., . A&A . 431-597 . 2005 . 2005A&A...431..597S ,
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 ,
Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 735-68 . 2011 . 2011ApJ...735...68K ,
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 ,
A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 747-107 . 2012 . 2012ApJ...747..107K ,
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 , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-01-20T00:12:35Z/2003-06-01T00:40:39Z
Version PPS_NOT_AVAILABLE
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 2003-06-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-06-01T00:00:00Z, 013452, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-te3l773