A dataset provided by the European Space Agency

Name 088205
Title Investigating new super-soft sources in the Magellanic Cloud System
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882050301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882050401

DOI https://doi.org/10.57780/esa-qzq0ky9
Author European Space Agency
Description The Magellanic Clouds are an ideal site to study super-soft X-ray sources given
their moderate and well known distances with low Galactic foreground absorption.
In the course of the eROSITA all-sky surveys the MCs are scanned frequently.
This provides the unique opportunity to detect new SSS in the full Magellanic
System as already demonstrated during the first survey. We propose three
triggered XMM observations of 20 ks each of new or unexplored SSS in the MS. Our
goal is to study their spectral and temporal properties in detail and identify
their nature by combining the existing multi-wavelength follow-up facilities we
have with the SALT transients collaboration and the GROND on the ESO/MPG
telescope.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-12-23T13:43:18Z/2022-01-22T01:55:01Z
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 2023-02-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Investigating New Super-Soft Sources In The Magellanic Cloud System, 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-qzq0ky9