A dataset provided by the European Space Agency

Name CYGNUSX3
Title INFRARED OBSERVATIONS OF CYGNUS X-3: WHAT IS THE ORIGIN OF THE INFRARED FLARES? - I AUTUMN TARGET LIST
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=130012060
DOI https://doi.org/10.5270/esa-yfvg8gq
Author Barr, Paul
Description we propose a long uninterrupted observation of the x-ray binary system cygnus x-3, lasting for 4,8hours (the period of the system), in order to study the colour evolution of the infrared flares seen in this exotic object. in particular we wish to test the predictions of the relativistic jet model regarding the spectral behaviour during the flares this proposal is identical to proposal ii (propid=cygnusx4) except that this proposal contains the autumn launch target list while proposal ii contain the spring launch target list
Instrument CAM01
Temporal Coverage 1996-03-26T15:36:02Z/1996-03-26T16:55:16Z
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 1999-03-31T00:00:00Z
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Barr et al., 1999, 'INFRARED OBSERVATIONS OF CYGNUS X-3: WHAT IS THE ORIGIN OF THE INFRARED FLARESquestionMark - I AUTUMN TARGET LIST', 1.0, European Space Agency, https://doi.org/10.5270/esa-yfvg8gq