A dataset provided by the European Space Agency

Name 078452
Title X-ray large scale survey of the nearby galaxy cluster Abell2199
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784520101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521701

DOI https://doi.org/10.5270/esa-be2o7em
Author Dr Takayuki Tamura
Description We use XMM to map the cluster Abell 2199 intermediate region (<3/4 virial
radius) and search X-ray faint substructures in a wide spacial range from a
galaxy to a cluster and larger sizes. We observed this area with SUZAKU and
found a number of structures and a hint of asymmetric large scale emission.
These substructures along with unresolved background sources should be resolved
spatially and covered fully with XMM imaging. Errors of the EPIC background will
be reduced by our SUZAKU deep spectra. These X-ray maps will be compared with
our wide area weak-lensing data observed with SUBARU Hyper suprime-Cam. The XMM
observations provide uniquely a direct comparison among structures of galaxies,
ICM, and dark matter.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-03-03T07:00:31Z/2017-03-22T10:50:54Z
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 2018-04-19T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Takayuki Tamura, 2018, 078452, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-be2o7em