A dataset provided by the European Space Agency

Name 1236
Title COULD EMISSION FROM DUST IN CLUSTERS OF GALAXIES CONFUSE OBSERVATIONS OF THE SUNYAEV-ZELDOVICH EFFECT?
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=573032070

DOI https://doi.org/10.5270/esa-b77hby2
Author MCHARDY, IAN M
Description as the microwave background (mwb) photons travel towards us through rich clusters of galaxies, they are scattered to higher energies by the hot gas in the clusters. the resulting spectral distortion is called the sunyaev-zeldovich (sz) effect and consists of a decrement in the mwb intensity in the direction of the cluster relative to the general background at wavelengths >1.4mm and an increment at wavelengths <1.4mm. the cosmological importance of the sz effect is that, when coupled with x-ray observations of the hot scattering gas, it is possible to deduce the scale size of the universe, ie the hubble constant, h_0. with the advent of the imaging sub-millimetre array, scuba, on the james clerk maxwell telescope (jcmt) it will soon be possible to make observations of the sz effect in the increment regime, where the spectral distortion should be large. however there have recently been some indications that clusters of galaxies may contain large amounts (10^9 solar massess) of very cool dust (temperatures of 10-30 k). such dust would dominate the cluster emission at 200 microns and, although largely undetectable by iras, could also radiate noticeably in the sub-millimetre waveband and so could confuse observations of the sz increment. we therefore propose isophot 200 observations, through 3 filters, to search for possible dust emission from a sample of sz candidate clusters, and to measure its temperature, in order to determine whether dust may confuse future determinations of h_0.
Instrument PHT32
Temporal Coverage 1997-06-11T13:19:15Z/1997-06-11T14:48:39Z
Version 1.0
Mission Description The Infrared Space Observatory (ISO) was the world's first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
Creator Contact https://support.cosmos.esa.int/iso/
Date Published 1999-04-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, MCHARDY, IAN M, 1999, 1236, 1.0, European Space Agency, https://doi.org/10.5270/esa-b77hby2