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19982018
most citedThe USNO-B Catalog

2.1k citations · 2.9k across the 9 of their papers we have counts for

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9 papers

astro-ph.SR2018★ 24 cited

Distant White Dwarfs in the US Naval Observatory Flagstaff Station Parallax Sample

S. K. Leggett, P. Bergeron, John P. Subasavage +18

This paper presents new trigonometric parallaxes and proper motions for 214 stars. The measurements were made at the US Naval Observatory Flagstaff Station (NOFS) between 1989 and…

astro-ph.SR2018★ 10 cited

Distances of Dwarf Carbon Stars

Hugh C. Harris, Conard C. Dahn, John P. Subasavage +8

Parallaxes are presented for a sample of 20 nearby dwarf carbon stars. The inferred luminosities cover almost two orders of magnitude. Their absolute magnitudes and tangential velo…

astro-ph.SR2017★ 36 cited

CCD Parallaxes for 309 Late-type Dwarfs and Subdwarfs

Conard C. Dahn, Hugh C. Harris, John P. Subasavage +16

New, updated, and/or revised CCD parallaxes determined with the Strand Astrometric Reflector at the Naval Observatory Flagstaff Station (NOFS) are presented. Included are results f…

astro-ph.SR2013★ 12 cited

The Binary White Dwarf LHS 3236

Hugh Harris, Conard Dahn, Trent Dupuy +13

The white dwarf LHS 3236 (WD1639+153) is shown to be a double-degenerate binary, with each component having a high mass. Astrometry at the U.S. Naval Observatory gives a parallax a…

astro-ph2008★ 44 cited

Trigonometric Parallaxes for Two Late-Type Subdwarfs: LSR1425+71 (sdM8.0) and the Binary LSR1610-00 (sd?M6pec)

C. C. Dahn, H. C. Harris, S. E. Levine +9

Trigonometric parallax astrometry and BVI photometry are presented for two late-type subdwarf candidates, LSR1425+71 (sdM8.0) and LSR1610-00 (sd?M6pec). For the former we measure a…

astro-ph2007★ 17 cited

The nearby young visual binary HIP 115147 and its common proper motion companion LSPM J2322+7847

V. V. Makarov, N. Zacharias, G. S. Hennessy +2

We report a late M-type, common proper motion companion to a nearby young visual binary HIP 115147 (V368 Cep), separated by 963 arcseconds from the primary K0 dwarf. This optically…