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USNO Bright Star Catalog (UBSC) is a new astrometric catalog of 1423 brightest stars covering the entire sky, which is published online. It is nearly complete to $V=3$ mag except for three stellar systems. A combined astrometric solution of…

Solar and Stellar Astrophysics · Physics 2022-07-20 Norbert Zacharias , Valeri V. Makarov , Charles T. Finch , Hugh C. Harris , Jeffrey A. Munn , John P. Subasavage

The proper motions of 15 nearby (d < 1 kpc) open clusters were recalculated using data from the UCAC4 catalog. Only evolved or main sequence stars inside a certain radius from the center of the cluster were used. The results differ…

Solar and Stellar Astrophysics · Physics 2016-12-22 Alexander Kurtenkov , Nadezhda Dimitrova , Alexander Atanasov , Teodor D. Aleksiev

The StarScan machine at the U.S. Naval Observatory (USNO) completed measuring photographic astrograph plates to allow determination of proper motions for the USNO CCD Astrograph Catalog (UCAC) program. All applicable 1940 AGK2 plates, about…

USNO-B1.0 and 2MASS are the most widely used full-sky surveys. However, 2MASS has no proper motions at all, and USNO-B1.0 published only relative, not absolute (i.e. on ICRS) proper motions. We performed a new determination of mean…

Astrophysics of Galaxies · Physics 2015-05-18 Siegfried Roeser , Markus Demleitner , Elena Schilbach

Most future surveys designed to discover transiting exoplanets, including TESS and PLATO, will target bright (V<13) and nearby solar-type stars having a spectral type later than F5. In order to enhance the probability of identifying…

We present mean proper motions and membership probabilities of individual stars for optically visible open clusters, which have been determined using data from the UCAC5 catalog. This follows our previous studies with the UCAC2 and UCAC4…

Solar and Stellar Astrophysics · Physics 2018-06-13 W. S. Dias , H. Monteiro , M. Assafin

A key science driver for the next generation of wide-field optical and radio surveys is the exploration of the time variable sky. These surveys will have unprecedented sensitivity and areal coverage, but will be limited in their ability to…

Astrophysics of Galaxies · Physics 2013-12-04 G. J. Madsen , B. M. Gaensler

The Lick Northern Proper Motion (NPM) program, a two-epoch (1947-1988) photographic survey of the northern two-thirds of the sky (Dec. > -23 deg), has measured absolute proper motions, on an inertial system defined by distant galaxies, for…

Astrophysics · Physics 2009-11-10 Robert B. Hanson , Arnold R. Klemola , Burton F. Jones , David G. Monet

The U.S. Naval Observatory Robotic Astrometric Telescope (URAT) is observing the northern sky since April 2012 for an astrometric survey. Multiple overlaps per year are performed in a single bandpass (680$-$750 nm) using the "redlens" 20 cm…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 Norbert Zacharias

We present the third installment of the Yale/San Juan Southern Proper Motion Catalog, SPM3. Absolute proper motions, positions, and photographic B,V photometry are given for roughly 10.7 million objects, primarily stars, down to a magnitude…

Astrophysics · Physics 2009-11-10 T. M. Girard , D. I. Dinescu , W. F. van Altena , I. Platais , D. G. Monet , C. E. Lopez

We present a catalog of 345,000 stars with proper motions \mu > 20 mas/yr and magnitudes r' <20, drawn from the intersection of the SDSS Data Release One and USNO-B. We first use SDSS quasars to correct the proper motions in each of the two…

Astrophysics · Physics 2010-03-01 Andrew Gould , Juna A. Kollmeier

Proper motions are computed and collected in a catalog using the Hipparcos positions (epoch 1991.25) and URAT1 positions (epoch 2012.3 to 2014.6). The goal is to obtain a significant improvement on the proper motion accuracy of single stars…

Solar and Stellar Astrophysics · Physics 2015-10-14 Julien Frouard , Bryan N. Dorland , Valeri V. Makarov , Norbert Zacharias , Charlie T. Finch

The results of 4,747 intensified CCD observations of double stars, made with the 26-inch refractor of the U.S. Naval Observatory, are presented. Each observation of a system represents a combination of over two thousand short-exposure…

Solar and Stellar Astrophysics · Physics 2017-10-18 Brian D. Mason , William I. Hartkopf

The historic plates of the "Carte du Ciel", an international cooperative project launched in 1887, offer valuable first-epoch material for the determination of absolute proper motions. We present the CdC-SF, an astrometric catalogue of…

Astrophysics of Galaxies · Physics 2015-05-14 Belen Vicente , Carlos Abad , Francisco Garzon , Terrence M. Girard

We combine Gaia DR1, PS1, SDSS and 2MASS astrometry to measure proper motions for 350 million sources across three-fourths of the sky down to a magnitude of $m_r\sim20$\,. Using positions of galaxies from PS1, we build a common reference…

The results of 3,989 intensified CCD observations of double stars, made with the 26-inch refractor of the U.S. Naval Observatory, are presented. Each observation of a system represents a combination of over two thousand short-exposure…

Solar and Stellar Astrophysics · Physics 2018-11-07 Brian D. Mason , William I. Hartkopf , Sean E. Urban , Jordan D. Josties

Completion of the SUPERBLINK proper motion survey in the southern celestial hemisphere has turned up 170 new stars with proper motion 0.45 arcsec/yr < pm < 2.0 arcsec/yr. This fourth and final installment completes the all-sky, data-mining…

Astrophysics · Physics 2009-11-13 Sebastien Lepine

This paper examines a subset of objects from the USNO-B1 catalogue with listed proper motions between 1.0 and 5.0 arcseconds per year. We look at the degree of contamination within this range of proper motions, and point out the major…

Astrophysics · Physics 2008-11-26 Stephen E. Levine

Using the USNO CCD Astrograph all-sky Catalog (UCAC2), we measure the mean proper motion of the two Magellanic Clouds. Appropriately selected LMC populations show a proper motion (<\mu RA>, <\mu DEC>) ~ (+0.84,+4.32) that is significantly…

Astrophysics · Physics 2009-11-11 Y. Momany , S. Zaggia

We describe the final product of the North Celestial Cap Survey (NCC Survey, NCCS) - the optical-UV-IR merged catalogue for the region within 10 deg of the North Celestial Pole. The NCC region at DEC > 80 deg is poorly covered by modern…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 Evgeny Gorbikov , Noah Brosch