A dataset provided by the European Space Agency

Name 050622
Title X-ray Spectrometry of SN1987A
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506220101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506220201

DOI 10.5270/esa-mamnqze
Author Dr Frank Haberl
Description The X-ray luminosity of SN1987A rapidly increased over the last four years, such that in a single 100 ks XMM-Newton obervation spectra can be taken with excellent counting statistics up to energies of 10 keV and more. In reference to our accepted 100 ksec AO5 observation another observation ~1 year later will allow to study the time evolution of the shock conditions and abundance profiles of N, O, Fe and Ne with RGS. At high energies EPIC-pn can help to clarify the extremely low Fe abundance of 0.04, observed so far. Is the Fe completely swallowed by the central compact object or is the emission from the inner sections of the progenitor star still absorbed? Because of the high number of counts a sensitive search for pulses from the pulsar limited to high energy photons will be possible.
Publication Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 735-68 . 2011 . 2011ApJ...735...68K ,
A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 747-107 . 2012 . 2012ApJ...747..107K ,
Evolution and Hydrodynamics of the Very Broad X-Ray Line Emission in SN 1987A . Dewey, D., Dwarkadas, V. V., et all. . ApJ . 752-103 . 2012 . 2012ApJ...752..103D ,
Suzaku Observations of SN 1987A . Sturm, Richard, Haberl, Frank, et all. . PASJ . 61-895 . 2009 . 2009PASJ...61..895S ,
High resolution X-ray spectroscopy of SN 1987 A: monitoring with XMM-Newton . Sturm, R., Haberl, F., et all. . A&A . 515-5 . 2010 . 2010A&A...515A...5S ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
XMM-Newton observations of SNR 1987A. II. The still increasing X-ray light curve and the properties of Fe K lines . Maggi, P., Haberl, F., et all. . A&A . 548-3 . 2012 . ...,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
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 ,
XMM-Newton study of 30 Doradus C and a newly identified MCSNR J0536-6913 in the Large Magellanic Cloud* . Kavanagh, P. J., Sasaki, M., et all. . A&A . 573-73 . 2015 . 2015A&A...573A..73K ,
A New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys . Terashima, Yuichi, Hirata, Yoshitaka, et all. . ApJ . 814-11 . 2015 . 2015ApJ...814...11T ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
Chandra Observes the End of an Era in SN 1987A . Frank, Kari A., Zhekov, Svetozar A., et all. . ApJ . 829-40 . 2016 . 2016ApJ...829...40F ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* . van Jaarsveld, N., Buckley, D. A. H., et all. . MNRAS . 475-3253 . 2018 . 2018MNRAS.475.3253V ,
X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC . Ou, Po-Sheng, Chu, You-Hua, et all. . ApJ . 863-137 . 2018 . 2018ApJ...863..137O ,
A Spatially Resolved Study of X-Ray Properties in Superbubble 30 Dor C with XMM-Newton . Babazaki, Yasunori, Mitsuishi, Ikuyuki, et all. . ApJ . 864-12 . 2018 . 2018ApJ...864...12B ,
3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission . Orlando, S., Miceli, M., et all. . A&A . 622-73 . 2019 . 2019A&A...622A..73O ,
Evidence of Particle Acceleration in the Superbubble 30 Doradus C with NuSTAR . Lopez, Laura A., Grefenstette, Brian W., et all. . ApJ . 893-144 . 2020 . 2020ApJ...893..144L ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-01-11T17:50:57Z/2008-01-13T04:14:44Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2009-02-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-02-07T00:00:00Z, 050622, 17.56_20190403_1200. https://doi.org/10.5270/esa-mamnqze