A dataset provided by the European Space Agency

Name CFREP305
Title Photometric Calibration of chopped observations.
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=734018030

DOI https://doi.org/10.5270/esa-l6nyx7v
Author Ulrich Klaas
Description the following program is carried out in order to consolidate the pht calibration of chopped measurements and derive signal losses due to the high chopper frequency compared to signal stabilization time. - observation of standard calibration stars: background and star staring plus chopped measurements. we intend to use well known calibration stars with a consolidated spectral energy distribution. the star is sufficiently bright to be used as a standard at wavelengths longward of 60 micron. several filters are taken to have several contrast levels between background and source. a second set of measurements is taken using shorter reset interval, in order to increase the chopper frequency. to do this we have to increase the fluxes to the double of its value. .history 23/06/97 ja first version. standard star is hr5340 26/08/97 ja standard star is hr6705 27/10/97\t ja standard star is hr7980 using detector p3 .ott .tdt
Instrument PHT03
Temporal Coverage 1997-11-19T03:27:37Z/1997-11-19T05:17:35Z
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 2024-10-31T19:44:17Z
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Ulrich Klaas, 2024, 'Photometric Calibration of chopped observations.', 1.0, European Space Agency, https://doi.org/10.5270/esa-l6nyx7v