A dataset provided by the European Space Agency

Name 014422
Title THE COMPOSITE SNR G0.9+0.1
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0144220101

DOI 10.5270/esa-wir3j7k
Author Dr Lara Sidoli
Description We propose an XMM-Newton observation of the composite supernova remnant G0.9+0.1, located in the Galactic Center region, from which we discovered X-rays with BeppoSAX. The main goals of the proposal are to perform a spatially resolved spectroscopy of the diffuse synchrotron nebula, to assess the likely presence of a young neutron star, and to detect X-rays from the radio shell.
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Spatially resolved X-ray spectroscopy and modeling of the nonthermal emission of the pulsar wind nebula in G0.9+0.1 . Holler, M., Schock, F. M., et all. . A&A . 539-24 . 2012 . 2012A&A...539A..24H ,
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High resolution radio study of the pulsar wind nebula within the supernova remnant G0.9+0.1 . Dubner, G., Giacani, E., . A&A . 487-1033 . 2008 . 2008A&A...487.1033D ,
XMMU J174716.1-281048: a ''quasi-persistent.. very faint X-ray transient? . Del Santo, M., Sidoli, L., et all. . A&A . 468-17 . 2007 . 2007A&A...468L..17D ,
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Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
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The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
The XMM-Newton view of the central degrees of the Milky Way . Ponti, G., Morris, M. R., et all. . MNRAS . 453-172 . 2015 . 2015MNRAS.453..172P ,
A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars . Pye, J. P., Rosen, S., et all. . A&A . 581-28 . 2015 . 2015A&A...581A..28P ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
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Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
An X-ray survey of the central molecular zone: Variability of the Fe Kalpha emission line . Terrier, R., Clavel, M., et all. . A&A . 612-102 . 2018 . 2018A&A...612A.102T ,
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X-ray chimneys in the Galactic Centre . Chernyakova, Masha, . Natur . 567-318 . 2019 . 2019Natur.567..318C ,
An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre . Ponti, G., Hofmann, F., et all. . Natur . 567-347 . 2019 . 2019Natur.567..347P ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2003-03-12T01:23:56Z/2003-03-12T15:57:30Z
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 2004-04-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-04-04T00:00:00Z, 014422, 17.56_20190403_1200. https://doi.org/10.5270/esa-wir3j7k