A dataset provided by the European Space Agency

Name: EPIC Gain, contamination and CTI monitoring-Vela SNR
Published: 2017-11-06T23:00:00Z

Proposal ID	041299
Title	EPIC Gain, contamination and CTI monitoring-Vela SNR
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991301 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991601
DOI	https://doi.org/10.5270/esa-cttuza4
Principal Investigator, PI	Dr Fred Jansen XMM-Newton MM
Abstract	EPIC Routine Calibration: spectral capabilities and contamination monitoringPA=102 shall be used as default (was proposal 015976).obs1: exceptionally pointed at RA 08:49:30.0 Dec -45:35:00 (req. by K. Dennerl) (normally at RA 08:48:49.05 Dec -45:38:26.1)obs6: coord. changed to RA 08:48:49 Dec -45:38:27 (req. by K. Dennerl)
Publications	Is Vela Jr. a young supernova remnant? \|Katsuda Satoru Tsunemi Hiroshi \| AdSpR \| 43-895 \| 2009 \| 2009AdSpR..43..895K \| http://ui.adsabs.harvard.edu/#abs/2009AdSpR..43..895K The X-ray spectral signatures from the complex circumnuclear regions in the Compton thick AGN NGC 424 \|Marinucci A. Bianchi S. et al. \| A&A \| 526-36 \| 2011 \| 2011A&A...526A..36M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..36M 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 Nonthermal emission properties of the northwestern rim of supernova remnant RX J0852.0-4622 \|Kishishita T. Hiraga J. \| A&A \| 551-132 \| 2013 \| 2013A&A...551A.132K \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A.132K 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 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 The Slow X-Ray Expansion of the Northwestern Rim of the Supernova Remnant RX J0852.0-4622 \|Katsuda S. Tsunemi H. \| ApJ \| 678-35 \| 2008 \| 2008ApJ...678L..35K \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...678L..35K 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 SRG/eROSITA and XMM-Newton observations of Vela Jr \|Camilloni Francesco Becker Werner et al. \| A&A \| 673-45 \| 2023 \| 2023A&A...673A..45C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..45C 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2006-11-09T00:38:22Z/2017-10-31T09:44:04Z
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	2017-11-06T23:00:00Z
Keywords	"epic gain", "05 dec", "EPIC", "vela supernova remnant", "ra 08", "epic routine calibration", "00 req"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton MM, 2017, 'EPIC Gain, contamination and CTI monitoring-Vela SNR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cttuza4