A dataset provided by the European Space Agency

Name 085261
Title A survey of NGC55: a holistic view of a low metallicity X-ray binary population
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852610101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852610201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852610301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852610401

DOI https://doi.org/10.57780/esa-p7r6z2p
Author European Space Agency
Description With NuSTAR, it is possible for the first time to determine the compact object
type and accretion state of large samples of X-ray binaries (XRBs) in nearby
galaxies. This classification, based on hard X-ray luminosity and hardness
ratios, can provide valuable insights into how XRB properties vary with
variables such as metallicity (Z), age, and specific star formation rate (sSFR).
Vulic et al. (2018) classified 90 XRBs in nearby galaxies observed by NuSTAR,
but the sample contains few galaxies with low-Z or low sSFR. Furthermore,
variability studies of XRB populations have been limited to M31. We propose
joint NuSTAR-XMM observations of the NGC 55 to expand studies of the compact
objects, accretion states, and variability of XRBs to lower luminosities in a low-Z galaxy.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-11-27T19:19:37Z/2020-05-19T11:12:28Z
Version 18.02_20200221_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 2021-05-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021, A Survey Of Ngc55: A Holistic View Of A Low Metallicity X-Ray Binary Population, 18.02_20200221_1200, European Space Agency, https://doi.org/10.57780/esa-p7r6z2p