A dataset provided by the European Space Agency

Name: Capella: RGS wavelength scale and bore-sight calibrations &amp; PV
Published: 2003-08-22T00:00:00Z

Proposal ID	012192
Title	Capella: RGS wavelength scale and bore-sight calibrations & PV
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0121920101
DOI	https://doi.org/10.5270/esa-kh5u6wh
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	CAL-RGS wavelength and bore-sight calibrationsFor the MOS cameras a default offset table needs to be used, in place of acalculated one. Observation 11 needs MOS DIAGNOSTOC exposures to be inserted.PV-High Resolution Spectroscopy of CapellaWe will study the spectrum of Capella, the brightest coronal source in the sky,with the RGS, in order to characterize the thermal structure and other physicalparameters of its corona. In addition, the spectrum will be used to derive thewavelength scale of the RGS and its dependence on the geometrical parameters ofthe spectrometers.
Publications	A study of coronal abundances in RS CVn binaries% \|Audard, M., Gudel, M., et al. \| A&A \| 398-1137 \| 2003 \| 2003A&A...398.1137A \| http://ui.adsabs.harvard.edu/#abs/2003A&A...398.1137A 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 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 X-ray spectroscopic studies of stars \|Gudel, M., \| AdSpR \| 32-2045 \| 2003 \| 2003AdSpR..32.2045G \| http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32.2045G The XMM-Newton view of stellar coronae: High-resolution X-ray spectroscopy of Capella \|Audard, M., Behar, E., et al. \| A&A \| 365-329 \| 2001 \| 2001A&A...365L.329A \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.329A 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 Modeling the Ne IX Triplet Spectral Region of Capella with the Chandra and XMM-Newton Gratings \|Ness, Jan-Uwe, Brickhouse, Nancy S., et al. \| ApJ \| 598-1277 \| 2003 \| 2003ApJ...598.1277N \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...598.1277N Capella Corona Revisited: A Combined View from XMM-Newton RGS and Chandra HETGS and LETGS \|Gu, M. F., Gupta, R., et al. \| ApJ \| 649-979 \| 2006 \| 2006ApJ...649..979G \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...649..979G Coronal densities and temperatures for cool stars in different stages of activity \|Ness, J.-U., Audard, M., et al. \| AdSpR \| 32-937 \| 2003 \| 2003AdSpR..32..937N \| http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32..937N 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 Constraints on the Ubiquity of Coronal X-Ray Cycles \|Hoffman, John, Gunther, Hans M., \| ApJ \| 759-145 \| 2012 \| 2012ApJ...759..145H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...759..145H 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 Calibration and in-orbit performance of the reflection grating spectrometer onboard XMM-Newton \|de Vries, C. P., den Herder, J. W., et al. \| A&A \| 573-128 \| 2015 \| 2015A&A...573A.128D \| http://ui.adsabs.harvard.edu/#abs/2015A&A...573A.128D Investigations of stellar coronae with XMM-Newton \|Audard, M., \| AdSpR \| 32-927 \| 2003 \| 2003AdSpR..32..927A \| http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32..927A 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 X-Ray Spectrum of Fe16+ Revisited with a Multi-Ion Model \|Doron, Rami, Behar, Ehud, \| ApJ \| 574-518 \| 2002 \| 2002ApJ...574..518D \| http://ui.adsabs.harvard.edu/#abs/2002ApJ...574..518D 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 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 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	2000-03-25T11:36:59Z/2000-03-26T03:53:49Z
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	2003-08-22T00:00:00Z
Keywords	"default offset table", "bore sight calibrations", "brightest coronal source", "resolution spectroscopy", "rgs wavelength scale", "geometrical parameters", "rgs wavelength", "mos cameras", "mos diagnostoc", "wavelength scale", "thermal structure", "physical parameters"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2003, 'Capella: RGS wavelength scale and bore-sight calibrations & PV', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kh5u6wh