Between 2007 and 2012, our yearly XMM-Newton monitoring of SN1987A yielded EPICand RGS spectra of unprecedented quality. The fluxes and broadening of thenumerous emission lines provide information on the evolution of the X-rayemitting plasma and its dynamics. The soft X-ray light curve shows a mildflattening after 2006. To further monitor the evolution of the X-ray flux andlook for a possible turn-over we propose to continue our monitoring. This willallow us to further study the time evolution of the shock conditions andabundance profiles. At high energies EPIC-pn can help to clarify the extremelylow observed Fe abundance by following the evolution of the detected Fe-K line.
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
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
BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary |Janssens, S., Shenar, T., et al. | A&A | 646-33 | 2021 | 2021A&A...646A..33J | http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..33J
The Post-impact Evolution of the X-Ray-emitting Gas in SNR 1987A as Viewed by XMM-Newton |Sun, Lei, Vink, Jacco, et al. | ApJ | 916-41 | 2021 | 2021ApJ...916...41S | http://ui.adsabs.harvard.edu/#abs/2021ApJ...916...41S
Thermal Emission and Radioactive Lines, but No Pulsar, in the Broadband X-Ray Spectrum of Supernova 1987A |Alp, Dennis, Larsson, Josefin, | ApJ | 916-76 | 2021 | 2021ApJ...916...76A | http://ui.adsabs.harvard.edu/#abs/2021ApJ...916...76A
Associated Molecular and Atomic Clouds with X-Ray Shell of Superbubble 30 Doradus C in the LMC |Yamane, Y., Sano, H., et al. | ApJ | 918-36 | 2021 | 2021ApJ...918...36Y | http://ui.adsabs.harvard.edu/#abs/2021ApJ...918...36Y
SN 1987A: Tracing the flux decline and spectral evolution through a comparison of SRG/eROSITA and XMM-Newton observations |Maitra, C., Haberl, F., et al. | A&A | 661-30 | 2022 | 2022A&A...661A..30M | http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..30M
Thermal X-ray emission in the western half of the LMC superbubble 30 Dor C |Chi, Yi-Heng, Chen, Han-Xiao, et al. | MNRAS | 530-4219 | 2024 | 2024MNRAS.530.4219C | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.4219C
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
2015-11-15T04:00:52Z/2015-11-15T22:37:32Z
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 Frank Haberl, 2016, 'X-ray Spectrometry of SN1987A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-s5goxsq
