A dataset provided by the European Space Agency

Name: XMM-Newton Observations of G330.2+1.0
Published: 2016-04-01T22:00:00Z

Proposal ID	074205
Title	XMM-Newton Observations of G330.2+1.0
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742050101
DOI	https://doi.org/10.5270/esa-v6xcqlo
Principal Investigator, PI	Dr Brian Williams
Abstract	G330.2+1.0 is one of only a few remnants in the Galaxy dominated by synchrotronradiation, and it is the only one of those to show hints of thermal emission aswell. Previous short {it XMM-Newton} and {it Chandra} observations areinsufficient to verify and characterize this result, and we propose here for adeeper observation to constrain both the thermal and nonthermal physics in theremnant. These observations will also allow us to constrain the amount ofparticle acceleration taking place around the periphery of the shell, which isentirely dominated by synchrotron emission, as well as reveal the nature of thecentral compact object as a neutron star, pulsar, or pulsar wind nebula.
Publications	A Deep X-Ray View of the Synchrotron-dominated Supernova Remnant G330.2+1.0 \|Williams, Brian J., Hewitt, John W., et al. \| ApJ \| 855-118 \| 2018 \| 2018ApJ...855..118W \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...855..118W CXOU J160103.1-513353: another central compact object with a carbon atmosphere? \|Doroshenko, V., Suleimanov, V., \| A&A \| 618-76 \| 2018 \| 2018A&A...618A..76D \| http://ui.adsabs.harvard.edu/#abs/2018A&A...618A..76D Anisotropic winds in a Wolf-Rayet binary identify a potential gamma-ray burst progenitor \|Callingham, J. R., Tuthill, P. G., et al. \| NatAs \| 3-82 \| 2019 \| 2019NatAs...3...82C \| http://ui.adsabs.harvard.edu/#abs/2019NatAs...3...82C Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z What causes the absence of pulsations in Central Compact Objects in supernova remnants? \|Wu, Qi, Pires, Adriana M., et al. \| RAA \| 21-294 \| 2021 \| 2021RAA....21..294W \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21..294W Do Central Compact Objects have Carbon Atmospheres? \|Alford, J. A. J., Halpern, J. P., \| ApJ \| 944-36 \| 2023 \| 2023ApJ...944...36A \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...944...36A Evidence for non-thermal X-ray emission from the double Wolf-Rayet colliding-wind binary Apep \|del Palacio, S., Garc\\u00eda, F., et al. \| A&A \| 672-109 \| 2023 \| 2023A&A...672A.109D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A.109D Mapping thermal emission in the synchrotron-dominated supernova remnants G330.2+1.0, 3C58, and RX J1713.7-3946 \|Picquenot, A., Williams, B. J., et al. \| A&A \| 683-A197 \| 2024 \| 2024A&A...683A.197P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...683A.197P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2015-03-08T05:50:30Z/2015-03-09T20:58:49Z
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2016-04-01T22:00:00Z
Keywords	"particle acceleration taking", "synchrotron emission", "XMM", "neutron star", "galaxy dominated", "G330.2", "central compact object", "XMM-Newton", "synchrotron radiation", "pulsar wind nebula", "thermal emission", "nonthermal physics", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Brian Williams, 2016, 'XMM-Newton Observations of G330.2+1.0', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-v6xcqlo