A dataset provided by the European Space Agency

Name: RGS AB Dor: Routine Calibrations
Published: 2012-01-01T00:00:00Z

Proposal ID	041258
Title	RGS AB Dor: Routine Calibrations
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412580801
DOI	https://doi.org/10.5270/esa-sfyo63t
Principal Investigator, PI	Dr Arvind Parmar XMM-Newton MM
Abstract	RGS Routine Calibration: AB Dor
Publications	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 al. \| ApJ \| 735-68 \| 2011 \| 2011ApJ...735...68K \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 747-107 \| 2012 \| 2012ApJ...747..107K \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 406-2013 \| 2010 \| 2010MNRAS.406.2013G \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.406.2013G An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C X-ray activity cycle on the active ultra-fast rotator AB Doradus A?. Implication of correlated coronal and photometric variability \|Lalitha, S., Schmitt, J. H. M. M., \| A&A \| 559-119 \| 2013 \| 2013A&A...559A.119L \| http://ui.adsabs.harvard.edu/#abs/2013A&A...559A.119L Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars \|Pye, J. P., Rosen, S., et al. \| A&A \| 581-28 \| 2015 \| 2015A&A...581A..28P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...581A..28P The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi, P., Haberl, F., et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M The Rotation of the Hot Gas around the Milky Way \|Hodges-Kluck, Edmund J., Miller, Matthew J., \| ApJ \| 822-21 \| 2016 \| 2016ApJ...822...21H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld, N., Buckley, D. A. H., et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou, Po-Sheng, Chu, You-Hua, et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O Superflares on AB Doradus observed with TESS \|Schmitt, J. H. M. M., Ioannidis, P., et al. \| A&A \| 628-79 \| 2019 \| 2019A&A...628A..79S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..79S New optically identified supernova remnants in the Large Magellanic Cloud \|Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Indications of stellar coronal mass ejections through coronal dimmings \|Veronig, Astrid M., Odert, Petra, et al. \| NatAs \| 5-697 \| 2021 \| 2021NatAs...5..697V \| http://ui.adsabs.harvard.edu/#abs/2021NatAs...5..697V Are Compton-thin AGNs Globally Compton Thin? \|Tzanavaris, P., Yaqoob, T., et al. \| ApJ \| 922-85 \| 2021 \| 2021ApJ...922...85T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...922...85T Helium absorption in exoplanet atmospheres is connected to stellar coronal abundances \|Poppenhaeger, K., \| MNRAS \| 512-1751 \| 2022 \| 2022MNRAS.512.1751P \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.1751P Study of the energetic X-ray superflares from the active fast rotator AB doradus \|Didel, Shweta, Pandey, Jeewan C., et al. \| MNRAS \| 527-1705 \| 2024 \| 2024MNRAS.527.1705D \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527.1705D A Statistical Study of Soft X-Ray Flares on Solar-type Stars \|Zhao, Z. H., Hua, Z. Q., et al. \| ApJ \| 961-130 \| 2024 \| 2024ApJ...961..130Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..130Z AB Dor: Coronal Imaging and Activity Cycles \|Singh, Gurpreet, Pandey, J. C., \| ApJ \| 966-86 \| 2024 \| 2024ApJ...966...86S \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966...86S Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords	"ab dor", "rgs ab dor", "rgs routine calibration", "routine calibrations"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Arvind Parmar XMM-Newton MM, 2012, 'RGS AB Dor: Routine Calibrations', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-sfyo63t