A dataset provided by the European Space Agency

Name DUST_SED
Title DUST IN SPIRAL GALAXIES ENERGY DISTRIBUTION AND TEMPERATURE
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=642005130

DOI https://doi.org/10.5270/esa-zyfa9ky
Author TREWHELLA, MATTHEW
Description =========================================================================== ==> this proposal is an extension of the grade 2 open time proposal jidavies.dustygal =========================================================================== our aim is to measure the spectral energy distribution of dust at several positions in spiral disks. we will be able to accurately determine the mass fraction of dust at different temperatures, the total mass of dust, the fraction of energy emitted by dust of different temperatures and the total energy output of dust. we will also see how these properties vary with position in the disk. this information will allow us to further investigate our initial findings from iso 200 micron observations of ngc 6946 which imply that strong radial dust temperature gradients are present in disk galaxies which cannot be detected using data from the iras satellite. by comparing the total energy output accurately measured with lws to that measured using iras hires and iso (isophot) observations at 12,25,60,100 and 200 microns we will be in position to create a set of template. spectra corresponding to a wide range of physical conditions encountered in galactic disks.these will significantly increase the accuracy of our measurements of the internal extinction in spiral galaxies with the jidavies.dustygal program. the total dust mass (and therefore dust-to-gas ratio) will be measured accurately as a function of position. current estimates of dust mass, based on iras data, span over an order of magnitude.
Instrument LWS01
Temporal Coverage 1997-05-01T10:12:14Z/1997-08-23T20:29:39Z
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 1998-08-31T00:00:00Z
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, TREWHELLA et al., 1998, 'DUST IN SPIRAL GALAXIES ENERGY DISTRIBUTION AND TEMPERATURE', 1.0, European Space Agency, https://doi.org/10.5270/esa-zyfa9ky