A dataset provided by the European Space Agency

Name 041258
Title RGS AB Dor: Routine Calibrations
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580801

DOI 10.5270/esa-sfyo63t
Author Dr Arvind Parmar XMM-Newton MM
Description RGS Routine Calibration: AB Dor
Publication 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 ,
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 ,
Final verdict from XMM-Newton: the X-ray obscured Seyfert galaxy NGC 5506 has a broad Fe Kalpha line . Guainazzi, M., Bianchi, S., et all. . MNRAS . 406-2013 . 2010 . 2010MNRAS.406.2013G ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
X-ray activity cycle on the active ultra-fast rotator AB Doradus A?. Implication of correlated coronal and photometric variability . Lalith...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-12-31T20:30:18Z/2012-01-01T08:34:38Z
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 2012-01-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-01-01T00:00:00Z, 041258, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-sfyo63t