A dataset provided by the European Space Agency

Name: TRACE SPECIES DETECTED THROUGH PDR EMISSION A STUDY OF DEPLETION IN THE GAS PHASE
Published: 1998-08-31T00:00:00Z

Name	PDR_TRAC
Title	TRACE SPECIES DETECTED THROUGH PDR EMISSION A STUDY OF DEPLETION IN THE GAS PHASE
URL	http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=555008230
DOI	https://doi.org/10.5270/esa-eue8jwn
Author	STUTZKI, JUERGEN
Description	we propose to measure infrared fine structure lines of the elements fe, cl, f, p, and ti in bright pdrs using the sws and lws in fabry-perot mode. this data can be used to derive the abundances of these elements in the dense interstellar medium. iso will be the only instrument capable of studying depletions in this phase of the interstellar mediumm in the foreseable future.
Instrument	LWS01 , LWS04 , SWS07
Temporal Coverage	1997-05-09T11:41:45Z/1997-08-01T03:58:38Z
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, STUTZKI et al., 1998, 'TRACE SPECIES DETECTED THROUGH PDR EMISSION A STUDY OF DEPLETION IN THE GAS PHASE', 1.0, European Space Agency, https://doi.org/10.5270/esa-eue8jwn