A dataset provided by the European Space Agency

Name 078338
Title A SHALLOW SURVEY OF THE AQUARUIS SUPECLUSTER FIELD
URL

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DOI https://doi.org/10.5270/esa-icxyfmo
Author Dr Maxim Markevitch
Description There is a place in the sky where the projected density of galaxy clusters is
factor 6 above average - a chain of superclusters spanning z=0.08-0.2, or 500
Mpc along the line of sight. Such fortuitous natural stacking of matter
concentrations improves our chances to detect signatures of the intergalactic
medium (WHIM). Intriguingly, our preliminary analysis of the public Planck data
hints at faint SZ signal from regions beyond known individual clusters. We
propose a shallow XMM survey of this scarcely observed area in order to detect
all clusters down to 1e43 erg/s, to be followed up with deeper observations for
accurate SZ modeling. We will then model away the cluster SZ contribution and
see if anything is left that can be attributed to WHIM in this giant filament.
Publication No observations found associated with the current proposal
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2016-12-15T08:44:58Z/2016-12-16T23:54:54Z
Version PPS_NOT_AVAILABLE
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 2018-01-13T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Maxim Markevitch, 2018, 078338, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-icxyfmo