A dataset provided by the European Space Agency

Name: A Deep XMM-Newton Legacy Survey of M33
Published: 2013-02-14T00:00:00Z

Proposal ID	067219
Title	A Deep XMM-Newton Legacy Survey of M33
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672190301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672190401
DOI	https://doi.org/10.5270/esa-gkhanmn
Principal Investigator, PI	Dr Benjamin Williams
Abstract	We request 190 ks of additional XMM-Newton time to complete our accepted 700 ksAO-9 Legacy program survey of M33. Rather than pad our AO-9 request to accountfor high background periods, we decided to proceed nominally and assess thebackground in the actual data. Four of the fields lost from 30 to 80 ks of theirplanned 100 ks time. We propose observations of these significantly impactedfields to bring the overall depth of exposure on each field to a similar level,thus improving the analysis. The complete survey will cover the entire regionenclosed by the D25 isophote, providing extensive information on the timing ofXRBs, the spectra of the largest known population of extragalactic SNRs, and theconnections between star formation and the hot component of the ISM.
Publications	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 Deep XMM-Newton Survey of M33: Point-source Catalog Source Detection and Characterization of Overlapping Fields \|Williams Benjamin F. Wold Brian et al. \| ApJS \| 218-9 \| 2015 \| 2015ApJS..218....9W \| http://ui.adsabs.harvard.edu/#abs/2015ApJS..218....9W Supernova remnants in M33: X-ray properties as observed by XMM-Newton \|Garofali Kristen Williams Benjamin F. et al. \| MNRAS \| 472-308 \| 2017 \| 2017MNRAS.472..308G \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472..308G Point and Compact Halpha Sources in the Interior of M33 \|Moody J. Ward Hintz Eric G. et al. \| AJ \| 154-268 \| 2017 \| 2017AJ....154..268M \| http://ui.adsabs.harvard.edu/#abs/2017AJ....154..268M MMT Spectroscopy of Supernova Remnant Candidates in M33 \|Long Knox S. Blair William P. et al. \| ApJ \| 855-140 \| 2018 \| 2018ApJ...855..140L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...855..140L On the Nature of the X-Ray Emission from the Ultraluminous X-Ray Source M33 X-8: New Constraints from NuSTAR and XMM-Newton \|West Lacey A. Lehmer Bret D. et al. \| ApJ \| 869-111 \| 2018 \| 2018ApJ...869..111W \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...869..111W A New Deep JVLA Radio Survey of M33 \|White Richard L. Long Knox S. et al. \| ApJS \| 241-37 \| 2019 \| 2019ApJS..241...37W \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..241...37W The First Candidate Colliding-wind Binary in M33 \|Garofali Kristen Levesque Emily M. et al. \| ApJ \| 880-8 \| 2019 \| 2019ApJ...880....8G \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...880....8G Formation time-scales for high-mass X-ray binaries in M33 \|Garofali Kristen Williams Benjamin F. et al. \| MNRAS \| 479-3526 \| 2018 \| 2018MNRAS.479.3526G \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.479.3526G Revealing Efficient Dust Formation at Low Metallicity in Extragalactic Carbon-rich Wolf-Rayet Binaries \|Lau Ryan M. Hankins Matthew J. et al. \| ApJ \| 909-113 \| 2021 \| 2021ApJ...909..113L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..113L 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 Young Black Hole and Neutron Star Systems in the Nearby Star-forming Galaxy M33: The NuSTAR View \|Yang Jun Wik Daniel R. et al. \| ApJ \| 930-64 \| 2022 \| 2022ApJ...930...64Y \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...64Y Monitoring the X-Ray Variability of Bright X-Ray Sources in M33 \|Kyer Rebecca Albrecht Shelby et al. \| ApJ \| 961-168 \| 2024 \| 2024ApJ...961..168K \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..168K 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	2012-01-10T14:13:30Z/2012-01-12T03:49:12Z
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	2013-02-14T00:00:00Z
Last Update	2025-01-27
Keywords	"impacted fields", "overall depth", "complete survey", "proceed nominally", "d25 isophote", "star formation", "M33", "region enclosed", "fields lost", "XMM-Newton", "program survey", "actual data", "hot component", "XMM", "extragalactic supernova remnant", "deep xmm newton", "background periods", "extensive information"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Benjamin Williams, 2013, 'A Deep XMM-Newton Legacy Survey of M33', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gkhanmn