Obs 1: The MOC wants to do a thruster torque calibration.Obs 2: NRCO 86 (Evaluating the short term stability of EPIC-pn Timing Modeoffset mapsObs 3:NRCO 87 (Assessing the quality of energy reconstruction in EPIC-pn TimingMode on Mkn 3)Obs 4: NRCO 89 (XB1254-690)Obs 5: NRCO 90 (GX13+1)Obs 6: NRCO 91 (Circinus Galaxy and EPIC-pn resolution at 6 keV) Obs 7: NRCO 92 (Simultaneous Chandra/Swift/XMM-Newton observation ofCygX-3: redistribution in timing modes)
Periodic signals from the Circinus region: two new cataclysmic variables and the ultraluminous X-ray source candidate GC X-1 |Esposito, P., Israel, G. L., et al. | MNRAS | 452-1112 | 2015 | 2015MNRAS.452.1112E | http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.1112E
Unveiling the Physics of Low-luminosity AGNs through X-Ray Variability: LINER versus Seyfert 2 |Hernandez-Garcia, L., Masegosa, J., et al. | ApJ | 824-7 | 2016 | 2016ApJ...824....7H | http://ui.adsabs.harvard.edu/#abs/2016ApJ...824....7H
The exceptional X-ray evolution of SN 1996cr in high resolution |Quirola-V\\u00e1squez, J., Bauer, F. E., et al. | MNRAS | 490-4536 | 2019 | 2019MNRAS.490.4536Q | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.490.4536Q
Long-term X-ray spectral evolution of ultraluminous X-ray sources: implications on the accretion flow geometry and the nature of the accretor |G\\u00farpide, A., Godet, O., et al. | A&A | 649-104 | 2021 | 2021A&A...649A.104G | http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.104G
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
2010-04-14T09:05:39Z/2014-06-25T14:56:34Z
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, 2014, 'Non routine calibration observations', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y0xj2r9
