A dataset provided by the European Space Agency

Name TOOCOMBA
Title TOO: ISOPHOT OBSERVATIONS OF A BRIGHT COMET COMA COMPOSITION AND DUST PRODUCTION
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=129017090

DOI https://doi.org/10.5270/esa-shp4j0k
Author Gruen, E.
Description long-period comets comprise even more primitive material than short-period comets. observations of their composition are diagnostic of the environment during their formation. there is a more than 50% chance that a bright long-period comet will be observable during the time of iso observations. this comet should be observed by a similar program as comet p/kopff in guaranteed time observations. this program includes three observation sequences at three different heliocentric distances in order to observe the development of cometray activity and of coma composition. for estimation of the integration time it is assumed that this comet is as bright as comet p/kopff.
Instrument PHT03 , PHT04 , PHT22
Temporal Coverage 1996-03-25T17:31:25Z/1996-10-10T17:04:14Z
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 1999-07-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Gruen, E., 1999, TOOCOMBA, 1.0, European Space Agency, https://doi.org/10.5270/esa-shp4j0k