A dataset provided by the European Space Agency

Name DUST_Z
Title THE DUST COMPOSITION IN DISTANT GALAXIES
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=443003060

DOI https://doi.org/10.5270/esa-ldn6kpa
Author GERIN, MARYVONNE
Description ===================================================================== == in this proposal, more time is being requested for mgerin.dust_hiz == the sample has been enlarged and the instrumental configuration changed. ===================================================================== we propose in this proposal to investigate the dust properties of distant iras galaxies (z =0.3, 0.6, 0.93 and 2.6) by looking for the presence of the uibs in their spectrum. the presence of these features and the detailed spectrum will give a good assessment on the nature of dust grains in these distant galaxies. we shall also measure the overall shape of the spectrum in the infrared, a very important ingredient in the interpretation of faint galaxy counts and in the prediction of the extragalactic background in the infrared.
Instrument CAM04
Temporal Coverage 1997-02-01T11:46:09Z/1997-02-07T09:15:39Z
Version 1.0
Mission Description The Infrared Space Observatory (ISO) was the worlds 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 1998-09-06T00:00:00Z
Last Update 2025-01-24
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, GERIN et al., 1998, 'THE DUST COMPOSITION IN DISTANT GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-ldn6kpa