A dataset provided by the European Space Agency

Name: AB Dor: RGS wavelength scale calibrations &amp; PV
Published: 2001-10-11T00:00:00Z

Proposal ID	012372
Title	AB Dor: RGS wavelength scale calibrations & PV
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123720201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123720301
DOI	https://doi.org/10.5270/esa-bll6885
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	CAL-RGS wavelength scale calibrationsFor the MOS cameras a default offset table needs to be used, in place of acalculated one.PV-We will acquire high resolution spectra of AB Dor with the RGS, in order tostudy the physical characteristics of the stellar corona. The source will beobserved for 100,000 sec, which covers two rotational periods. This dataset willdemonstrate the potential of the RGS for performing phase-resolved spectroscopy.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2003A&A...408.1087S Exploring the X-ray sky with the XMM-Newton bright serendipitous survey \|Della Ceca, R., Maccacaro, T., et al. \| A&A \| 428-383 \| 2004 \| 2004A&A...428..383D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...428..383D High-precision multi-band measurements of the angular clustering of X-ray sources \|Ebrero, J., Mateos, S., et al. \| A&A \| 500-749 \| 2009 \| 2009A&A...500..749E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...500..749E The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 735-68 \| 2011 \| 2011ApJ...735...68K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...735...68K Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 747-107 \| 2012 \| 2012ApJ...747..107K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...747..107K The XMM-Newton view of stellar coronae: X-ray spectroscopy of the corona of AB Doradus \|Gudel, M., Audard, M., et al. \| A&A \| 365-336 \| 2001 \| 2001A&A...365L.336G \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.336G Are stellar coronae optically thin in X-rays?. A systematic investigation of opacity effects \|Ness, J.-U., Schmitt, J. H. M. M., et al. \| A&A \| 407-347 \| 2003 \| 2003A&A...407..347N \| http://ui.adsabs.harvard.edu/#abs/2003A&A...407..347N On the sizes of stellar X-ray coronae \|Ness, J.-U., Gudel, M., et al. \| A&A \| 427-667 \| 2004 \| 2004A&A...427..667N \| http://ui.adsabs.harvard.edu/#abs/2004A&A...427..667N Identifying XMM-Newton observations affected by solar wind charge exchange. Part I \|Carter, J. A., Sembay, S., \| A&A \| 489-837 \| 2008 \| 2008A&A...489..837C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...489..837C High precision X-ray log N - log S distributions: implications for the obscured AGN population \|Mateos, S., Warwick, R. S., et al. \| A&A \| 492-51 \| 2008 \| 2008A&A...492...51M \| http://ui.adsabs.harvard.edu/#abs/2008A&A...492...51M Flare X-Ray Observations of AB Doradus: Evidence of Stellar Coronal Opacity \|Matranga, M., Mathioudakis, M., et al. \| ApJ \| 621-125 \| 2005 \| 2005ApJ...621L.125M \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...621L.125M XMM-Newton EPIC Background Modeling for Extended Sources \|Nevalainen, J., Markevitch, M., \| ApJ \| 629-172 \| 2005 \| 2005ApJ...629..172N \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...629..172N The XMM-Newton serendipitous survey. VI. The X-ray luminosity function \|Ebrero, J., Carrera, F. J., et al. \| A&A \| 493-55 \| 2009 \| 2009A&A...493...55E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493...55E Breaking the sigma8-Omega m Degeneracy Using the Clustering of High-z X-ray Active Galactic Nuclei \|Basilakos, Spyros, Plionis, Manolis, \| ApJ \| 714-185 \| 2010 \| 2010ApJ...714L.185B \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714L.185B 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 Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis, A. E., Chavushyan, V., et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C 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 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 The XMM-Newton serendipitous source catalogue \|Watson, M. G., Pye, J. P., et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W 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 Simulated X-ray cycles in rapidly rotating solar-like stars \|McIvor, T., Jardine, M., et al. \| MNRAS \| 367-592 \| 2006 \| 2006MNRAS.367..592M \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367..592M The relationship between O IIIlambda5007 A equivalent width and obscuration in active galactic nuclei \|Caccianiga, A., Severgnini, P., \| MNRAS \| 415-1928 \| 2011 \| 2011MNRAS.415.1928C \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.415.1928C 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 Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era \|Evans, P. A., Osborne, J. P., et al. \| MNRAS \| 448-2210 \| 2015 \| 2015MNRAS.448.2210E \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.448.2210E 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 Why solar astronomers should be interested in stars \|Pallavicini, R., \| AdSpR \| 32-885 \| 2003 \| 2003AdSpR..32..885P \| http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32..885P 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 Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S 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 The evolving X-ray spectrum of active galactic nuclei: Evidence for an increasing reflection fraction with redshift \|Avirett-Mackenzie, M. S., Ballantyne, D. R., \| MNRAS \| 486-3488 \| 2019 \| 2019MNRAS.486.3488A \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.3488A 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 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	2000-05-01T02:30:21Z/2000-10-28T07:23:28Z
Version	17.56_20190403_1200
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	2001-10-11T00:00:00Z
Keywords	"covers rotational periods", "default offset table", "000 sec", "physical characteristics", "mos cameras", "stellar corona", "ab dor", "resolution spectra"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2001, 'AB Dor: RGS wavelength scale calibrations & PV', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bll6885