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.
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
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
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
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
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.
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
