cPbL. August 12 2000

 Find TITLE-PHRASE THIRTEEN-COLOR PHOTOMETRY of 1380 OR  TITLE-PHRASE LIBRARY OF STELLAR SPECTRA   


2 citations



/usr/tmp/citation.tmp.27059
@ARTICLE{JacobyOct84,
	author={Jacoby, G.H. and Hunter, D.A. and Christian, C.A.},
	title={
A library of stellar spectra
	},
	journal={Astrophysical Journal Supplement Series},
	volume={56},
	number={2},
	year={1984},
	month={Oct},
	pages={257-81},
	abstract={
Spectra for 161 stars having spectral classes O-M and luminosity classes V,
III, and I have been incorporated into a library available on magnetic
tape. The spectra extend from 3510 to 7427 AA at a resolution of
approximately 4.5 AA. The typical photometric uncertainty of each
resolution element in the spectra is on the order of 1%, while broad-band
variations are smaller than 3%. Potential uses for the library include
population synthesis of galaxies and clusters, tests of stellar atmosphere
models, spectral classification, and the generation of color indices having
arbitrary wavelength and bandpass
	},
	keywords={
		astronomical catalogues
		stellar photometry
		stellar spectra
		ultraviolet astronomical observations
		visible astronomical observations
		visible
		UV
		nm 0351 to 0742
		spectrophotometry
		AD 1980 12 to 1981 12
		stellar spectra
		spectral classes
		luminosity classes
		magnetic tape
		population synthesis
		galaxies
		clusters
		stellar atmosphere models
		spectral classification
		color indices
		},
	mynotes={UNREAD},
}
@ARTICLE{JohnsonSep75,
	author={Johnson, H.L. and Mitchell, R.I.},
	title={
Thirteen-color photometry of 1380 bright stars
	},
	journal={Revista Mexicana de Astronomia y Astrofisica},
	volume={1},
	number={3},
	year={1975},
	month={Sep},
	pages={299-324},
	abstract={
Presents the final data from an extended program of 13-color
medium-narrow-band photometry. The observations include essentially all of
the stars brighter than the fifth visual magnitude north of declination -20
degrees , essentially all of the stars brighter than the fourth visual
magnitude south of declination -20 degrees . A new absolute calibration,
based upon all of the available data is derived. This photometric system
should be useful for the standardization of other photometric systems, as
well as for narrow-band spectrophotometry
	},
	keywords={
		stellar radiation
		stellar spectrophotometry
		bright stars
		absolute calibration
		standardization
		13 colour photometry
		medium narrow band photometry
		},
	mynotes={UNREAD},
}