A dataset provided by the European Space Agency

Name: EPIC Routine Calibration: Tycho SNR
Published: 2008-01-04T00:00:00Z

Proposal ID	051118
Title	EPIC Routine Calibration: Tycho SNR
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511180101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511180201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511180301
DOI	https://doi.org/10.5270/esa-6pz48mc
Principal Investigator, PI	Dr Arvind Parmar XMM-Newton MM
Abstract	EPIC Non Routine Calibration (NRCO#71): Tycho SNRCTE Calibration using CAL source and SNRPA fixed to 45 degr (i.e. to be scheduled in August)(if not possible, PA=225)(original proposal was 31059 - PI F. Jansen)
Publications	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 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 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 Discovery of a 3.5 keV line in the Galactic Centre and a critical look at the origin of the line across astronomical targets \|Jeltema Tesla Profumo Stefano \| MNRAS \| 450-2143 \| 2015 \| 2015MNRAS.450.2143J \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.450.2143J Spatial Distribution of X-Ray Emitting Ejecta in Tychos SNR: Indications of Shocked Titanium \|Miceli M. Sciortino S. et al. \| ApJ \| 805-120 \| 2015 \| 2015ApJ...805..120M \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805..120M Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus \|Carlson Eric Jeltema Tesla \| JCAP \| 2-9 \| 2015 \| 2015JCAP...02..009C \| http://ui.adsabs.harvard.edu/#abs/2015JCAP...02..009C 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 Three-dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tychos Supernova Remnant \|Uchida Hiroyuki Kasuga Tomoaki et al. \| ApJ \| 962-159 \| 2024 \| 2024ApJ...962..159U \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...962..159U 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	2007-12-30T19:32:51Z/2008-01-03T08:12:15Z
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	2008-01-04T00:00:00Z
Last Update	2025-01-27
Keywords	"tycho supernova remnant", "EPIC", "cal source", "routine calibration nrco", "epic routine calibration", "225 original", "31059 pi"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Arvind Parmar XMM-Newton MM, 2008, 'EPIC Routine Calibration: Tycho SNR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6pz48mc