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HD 54683


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Classification of Spectra from the Infrared Space Observatory PHT-S Database
We have classified over 1500 infrared spectra obtained with the PHT-Sspectrometer aboard the Infrared Space Observatory according to thesystem developed for the Short Wavelength Spectrometer (SWS) spectra byKraemer et al. The majority of these spectra contribute to subclassesthat are either underrepresented in the SWS spectral database or containsources that are too faint, such as M dwarfs, to have been observed byeither the SWS or the Infrared Astronomical Satellite Low ResolutionSpectrometer. There is strong overall agreement about the chemistry ofobjects observed with both instruments. Discrepancies can usually betraced to the different wavelength ranges and sensitivities of theinstruments. Finally, a large subset of the observations (~=250 spectra)exhibit a featureless, red continuum that is consistent with emissionfrom zodiacal dust and suggest directions for further analysis of thisserendipitous measurement of the zodiacal background.Based on observations with the Infrared Space Observatory (ISO), aEuropean Space Agency (ESA) project with instruments funded by ESAMember States (especially the Principle Investigator countries: France,Germany, Netherlands, and United Kingdom) and with the participation ofthe Institute of Space and Astronautical Science (ISAS) and the NationalAeronautics and Space Administration (NASA).

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Observation and Astrometry data

Constellation:テーブルさん座
Right ascension:07h01m23.64s
Declination:-75°37'15.3"
Apparent magnitude:8.902
Distance:302.115 parsecs
Proper motion RA:6.8
Proper motion Dec:12.5
B-T magnitude:10.952
V-T magnitude:9.072

Catalogs and designations:
Proper Names
HD 1989HD 54683
TYCHO-2 2000TYC 9380-1052-1
USNO-A2.0USNO-A2 0075-01299664
HIPHIP 33830

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