A dataset provided by the European Space Agency

Name 088199
Title A Survey of Late-Time X-ray Emission in VLASS Detected Supernovae
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881990101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881990201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881990701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881990901

DOI https://doi.org/10.57780/esa-f8hfkyi
Author Dr Michael Stroh
Description Radio and X-ray observations of supernovae (SNe) acquired in the poorly sampled
phase of years to decades post-explosion are necessary to drive progress in
several fundamental areas of explosive transient research. Bright emission
virgulyears to decades post explosion of extragalactic SNe may be due to A)
shock-interaction with the circumstellar medium; or B) the emergence of
radiation from a pulsar wind nebula. A solid identification of the scenarios
above would lead to significant advances in our understanding of the physics of
stellar explosions, their progenitors, and their remnants. We propose the first
systematic late-time X-ray survey of SNe with bright detected radio emission.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-05-26T02:56:55Z/2022-03-19T12:32:41Z
Version 19.17_20220121_1250
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 2023-04-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Michael Stroh, 2023, 088199, 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-f8hfkyi