A dataset provided by the European Space Agency

Name M16_CVF
Title ISOCAM M16 IMAGING FOLLOW-UP: CVF SPECTRO-IMAGING
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=703014010

DOI https://doi.org/10.5270/esa-b9pohhf
Author PILBRATT, GORAN
Description the objective of this supplementary discretionary time proposal is to perform isocam cvf spectro-imaging of (most of) the field in the m16 eagle nebula which we earlier mapped in lw2 and lw3. the goal is to establish the physical nature of the emission, including in a mysterious extended feature discovered in our lw3 image located near (but outside the extent of) the main elephant trunk in the hubble field in m16.
Instrument CAM04
Temporal Coverage 1997-10-19T01:45:58Z/1997-10-19T03:06:38Z
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 1999-01-20T00:00:00Z
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, PILBRATT et al., 1999, 'ISOCAM M16 IMAGING FOLLOW-UP: CVF SPECTRO-IMAGING', 1.0, European Space Agency, https://doi.org/10.5270/esa-b9pohhf