A dataset provided by the European Space Agency

Name SN1987A
Title IRON-GROUP SPECTROSCOPY OF SN1987A
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=236010020

DOI https://doi.org/10.5270/esa-ozf6six
Author WOODEN, DIANE H.
Description we propose observations of the heavy-element interior of supernova sn1987a utilizing the [nii] (7.51 microns), [niii] (6.64 microns), [fei] (24.04, 34.71 and 51.29 microns), [feii] (25.99, 35.34 and 51.68 microns), and [feiii] (22.93, 33.04 and 54.31 microns) lines. these measurements are a followon to our successful iron and nickel line studies from the kuiper airborne observatory (erickson etal. 1988; haas etal. 1990; wooden etal. 1993; colgan etal. 1994). utilizing the increased sensitivity of iso, we will continue to probe the evolution of the ionization states, densities, and temperatures of the iron-rich regions of the ejecta, and ascertain the existence of a central energy source (i.e. a pulsar).
Instrument LWS02 , SWS06
Temporal Coverage 1996-07-10T08:41:02Z/1996-07-10T10:24:28Z
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 1999-02-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, WOODEN, DIANE H., 1999, SN1987A, 1.0, European Space Agency, https://doi.org/10.5270/esa-ozf6six