A dataset provided by the European Space Agency

Name: A Deep XMM-Newton Legacy Survey of M33
Published: 2011-09-11T00:00:00Z

Proposal ID	065051
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=0650510101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650510201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650510301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650510401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650510501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650510601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650510701
DOI	https://doi.org/10.5270/esa-r6nli1b
Principal Investigator, PI	Dr Benjamin Williams
Abstract	We propose a deep XMM-Newton legacy survey of M33 covering the entire D25isophote with a total of 700 ks of exposure. These data will allow us todetermine how the temperature and energetics of the hot interstellar medium areaffected by star formation, constrain the nature and dynamical masses of newpulsating and eclipsing X-ray binaries, and perform detailed statistical andspectral studies on the largest extragalactic population of X-ray supernovaremnants. As the deepest and most complete X-ray census of an entire spiralgalaxy possible with current technology, our survey will test the physics ofdiffuse hot gas and the evolution of X-ray source populations at luminositiesnever before available for such a sample.
Publications	The ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion \|Sutton, Andrew D., Roberts, Timothy P., \| MNRAS \| 435-1758 \| 2013 \| 2013MNRAS.435.1758S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.1758S XMM-Newton discovery of transient 285.4 s X-ray pulsar XMMU J013359.5+303634 in M33 \|Trudolyubov, S. P., \| MNRAS \| 435-3326 \| 2013 \| 2013MNRAS.435.3326T \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.3326T 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 Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson, Michael E., Churazov, Eugene, \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 Crossing the Eddington Limit: Examining Disk Spectra at High Accretion Rates \|Sutton, Andrew D., Swartz, Douglas A., et al. \| ApJ \| 836-48 \| 2017 \| 2017ApJ...836...48S \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...836...48S The Wolf-Rayet Content of M33 \|Neugent, Kathryn F., Massey, Philip, \| ApJ \| 733-123 \| 2011 \| 2011ApJ...733..123N \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...733..123N 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	2010-07-09T07:04:52Z/2010-08-15T14:04:03Z
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	2011-09-11T00:00:00Z
Keywords	"xray supernova remnant", "star formation", "deep xmm newton", "eclipsing xray binary", "largest extragalactic population", "XMM", "dynamical masses", "hot interstellar medium", "M33", "spiral galaxy", "XMM-Newton", "xray source populations", "diffuse hot gas", "complete xray census", "d25 isophote"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Benjamin Williams, 2011, 'A Deep XMM-Newton Legacy Survey of M33', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-r6nli1b