A dataset provided by the European Space Agency

Name: Search for central compact stars in two Galactic SNRs and their first X-ray char
Published: 2017-11-29T23:00:00Z

Proposal ID	078146
Title	Search for central compact stars in two Galactic SNRs and their first X-ray char
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781460101
DOI	https://doi.org/10.5270/esa-nw783wm
Principal Investigator, PI	Dr Dmitry Klochkov
Abstract	We propose to observe two Galactic supernova remnants (SNRs) G94.0+1.0 andG96.0+2.0 which have so far not been characterized in X-rays. We plan to searchfor possible central neutron stars (NS) associated with the remnants, i.e. toincrease the small but diverse class of isolated NSs associated with SNRs, andto perform the first morphological and spectral study of the remnants in X-rays.The target SNRs are located relatively far from the Galactic center resulting inlow absorption, their size does not exceed the XMM-Newton FoV and distanceestimates exist for both remnants making them ideal targets for the proposedstudies.
Publications	XMM-Newton and Fermi/LAT view on the supernova remnant 3C434.1 \|Doroshenko V. Malyshev D. et al. \| A&A \| 631-179 \| 2019 \| 2019A&A...631A.179D \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.179D 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-11-07T12:59:28Z/2016-11-07T22:09:28Z
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	2017-11-29T23:00:00Z
Last Update	2025-01-27
Keywords	"target supernova remnant", "isolated nss", "ideal targets", "galactic supernova remnant", "located relatively", "supernova remnant", "XMM-Newton", "diverse class", "low absorption", "XMM", "xmm newton fov", "central compact stars", "xray char", "galactic center", "G94.0"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Dmitry Klochkov, 2017, 'Search for central compact stars in two Galactic SNRs and their first X-ray char', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-nw783wm