A dataset provided by the European Space Agency

Name 012372
Title AB Dor: RGS wavelength scale calibrations & PV
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123720201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123720301

DOI 10.5270/esa-bll6885
Author Dr Fred Jansen XMM-Newton PS
Description CAL-RGS wavelength scale calibrations For the MOS cameras a default offset table needs to be used, in place of a calculated one. PV-We will acquire high resolution spectra of AB Dor with the RGS, in order to study the physical characteristics of the stellar corona. The source will be observed for 100,000 sec, which covers two rotational periods. This dataset will demonstrate the potential of the RGS for performing phase-resolved spectroscopy.
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 ,
Exploring the X-ray sky with the XMM-Newton bright serendipitous survey . Della Ceca, R., Maccacaro, T., et all. . A&A . 428-383 . 2004 . 2004A&A...428..383D ,
High-precision multi-band measurements of the angular clustering of X-ray sources . Ebrero, J., Mateos, S., et all. . A&A . 500-749 . 2009 . 2009A&A...500..749E ,
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-Newton view of stellar corona...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-05-01T02:30:21Z/2000-10-28T07:23:28Z
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 2001-10-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2001-10-11T00:00:00Z, 012372, 17.56_20190403_1200. https://doi.org/10.5270/esa-bll6885