Routine CAL - During periods of low visibility, the primary target 1es0102 willbe supplemented by observations of the bright LMC supernova remnant N132D. Normally pn shall be in sw mode.New coords and PA constraints to be defined by M. Ehleobs20 (in previous proposal 12934) had PA=247 and corresponding sw coords. thatshould be used for all future monitoring in February.
Publications
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue |Watson, M. G., Schroder, A. C., et al. | A&A | 493-339 | 2009 | 2009A&A...493..339W | http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras |Mateos, S., Saxton, R. D., et al. | A&A | 496-879 | 2009 | 2009A&A...496..879M | http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M
A systematic cross-search for radio/infrared counterparts of XMM- Newton sources |Combi, J. A., Albacete Colombo, J. F., et al. | Ap&SS | 331-53 | 2011 | 2011Ap&SS.331...53C | http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C
Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* |van Jaarsveld, N., Buckley, D. A. H., et al. | MNRAS | 475-3253 | 2018 | 2018MNRAS.475.3253V | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V
Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D |Sharda, Piyush, Gaetz, Terrance J., et al. | ApJ | 894-145 | 2020 | 2020ApJ...894..145S | http://ui.adsabs.harvard.edu/#abs/2020ApJ...894..145S
New optically identified supernova remnants in the Large Magellanic Cloud |Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. | MNRAS | 500-2336 | 2021 | 2021MNRAS.500.2336Y | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y
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
2007-02-05T10:10:50Z/2017-02-18T01:22:42Z
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 Fred Jansen XMM-Newton MM, 2017, 'EPIC GAIN comma CTE AND CONTAMINATION MONITORING-N132D', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-swadq8y
