A dataset provided by the European Space Agency

Name 010264
Title Deep survey of M33 TS33
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102640901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102641001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102641101
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102641201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102641701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102641801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102642001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102642101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102642201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102642301

DOI https://doi.org/10.5270/esa-yv5rspi
Author Dr Bernd Aschenbach
Description GT-We propose a raster observation of the bright local group spiral galaxy M33 to perform an unbiased study of its population of X-ray sources (SNRs, XRBs, supershells) down to a luminosity limit of 1e35 erg-s (a factor of 10 deeper than earlier ROSAT observations). EPIC spectra will be used to separate between different source classes. Short term time variability of brighter sources (pulsations of the order of sec) will be investigated as well as long term variability of the brighter sources (binary light curves, transients, variability of nuclear source). We also will be able to spectrally characterize the diffuse component that is correlated with the inner spiral arms. Observations are ordered to allow timing analysis on different time scales.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-08-02T00:23:43Z/2002-01-27T13:18:01Z
Version 17.56_20190403_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 2002-12-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-12-16T00:00:00Z, 010264, 17.56_20190403_1200. https://doi.org/10.5270/esa-yv5rspi