At the compromise distance of 570 light years, the star has a total bolometric luminosity some 85,000 times that of the.    From Wordnik.com.  [Conservapedia - Recent changes [en]] Reference

Its visible portion covers a range of about one octave; bolometric indications already in 1884 comprised between three and four.    From Wordnik.com.  [A Popular History of Astronomy During the Nineteenth Century Fourth Edition] Reference

Because of their intrinsically red colors and dusty circumstellar envelopes, tracking the numbers and bolometric fluxes of AGB stars requires the NIR observations we propose here.    From Wordnik.com.  [SpaceRef Top Stories] Reference

As to the eye, we have reason to believe, from the bolometric observations of LANGLEY (1888), that the mean wave-length of the visual curve of intensity nearly coincides with that of the true intensity-curve, a conclusion easily understood from.    From Wordnik.com.  [Lectures on Stellar Statistics] Reference

Confirmatory evidence of the extraordinary promptitude with which our satellite parts with heat already to some extent appropriated, was afforded by Professor Langley's bolometric observations at Allegheny of the partial eclipse of September 23.    From Wordnik.com.  [A Popular History of Astronomy During the Nineteenth Century Fourth Edition] Reference