A dataset provided by the European Space Agency

Name ULT_QD_1
Title PHOTOMETRY AND SPECTROSCOPY OF ULTRALUMINOUS IRAS GALAXIES: THE QDOT SAMPLE
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=216003160

DOI https://doi.org/10.5270/esa-d6g5nyp
Author ROWAN-ROBINSON, MICHAEL
Description we propose to carry out multiwavelength photometry at 4-200 mu of a complete all-sky sample of ultraluminous iras galaxies from the qdot survey, and to perform spectroscopy with lws and sws on a few of the brighter galaxies in the sample. the discovery of ultraluminous infrared galaxies was one of the major results of the iras mission. subsequent study of these galaxies has been hampered by lack of access to most of the infrared waveband. detailed radiative transfer models for starbursts and agn contributions to the far infrared continuum are porrly constrained by the iras fluxes. in most cases only 60 and 100 mu fluxes were detected by iras. although there is a concensus that interactions and mergers play a major role in generating ultraluminous infrared galaxies, there is major controversy about whether massive starbursts or shrouded quasars are the principal contributors to the emission. detailed spectral energy distributions over a wide spectral range will be a powerful tool in resolving the controversy. study of a complete sample is essentail for statistical and quantitative conclusions to be reached. spectroscopy of a smaple of the brighter galaxies at 4-200 mu will allow us to assess the contribution of line emission to the broad band fluxes, provide diagnostic evidence of the presence of starbursts, and give the contribution of broad features from very small grains or pahs (and the magnitude of depletion of these features) in a variety of environments. the 10 mu silicate feature and its shape is an especially important constraint on radiative transfer models.
Instrument CAM01 , PHT22
Temporal Coverage 1996-06-20T04:16:53Z/1996-08-09T01:06:41Z
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 1999-04-29T00:00:00Z
Last Update 2026-03-02
Keywords Infrared Space Observatory data, ESA ISO mission dataset, ISO infrared observations, mid-infrared astronomy data, far-infrared spectroscopy dataset, ISOCAM imaging data, ISOPHOT photometry data, SWS short wavelength spectrometer data, LWS long wavelength spectrometer data, infrared spectral line observations, infrared imaging survey data, dust emission infrared observations, star formation infrared dataset, interstellar medium spectroscopy data, polycyclic aromatic hydrocarbons PAH features data, active galactic nuclei infrared observations, circumstellar envelope infrared data, planetary nebula infrared spectroscopy, extragalactic infrared survey data, calibrated ISO data products, FITS files infrared astronomy, spectral energy distribution infrared data, continuum photometry dataset, infrared spectral cubes, flux-calibrated infrared maps, ESA ISO Data Archive, legacy infrared space mission dataset
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, ROWAN-ROBINSON et al., 1999, 'PHOTOMETRY AND SPECTROSCOPY OF ULTRALUMINOUS IRAS GALAXIES: THE QDOT SAMPLE', 1.0, European Space Agency, https://doi.org/10.5270/esa-d6g5nyp