Searching for benchmark systems containing ultra-cool dwarfs and white dwarfs by Pinfield D.J., Gomes J.I.

“…We cross-matched L dwarf candidates from the surveys with Hipparcos and Gliese stars, finding two new systems. …”
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On the mass distribution of stars in the solar neighborhood by Ninković S., Trajkovska V.

“…The present authors analyze samples consisting of Hipparcos stars. Based on the corresponding HR diagrams they estimate masses of Main-Sequence stars from their visual magnitudes. …”
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BV CCD Photometry of M71: Distance and Age by Hong-Suh Yim, Mun-Suk Chun, Yong-Ik Byun, Young-Jong Sohn

“…Based on our color-magnitude diagram (CMD), we derive the distance to M71 using a sample of Hipparcos subdwarfs of similar metallicity. Our distance modulus is (m-M)V=13.46(± 0.17). …”
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MODERN CCD OBSERVATIONS OF SELECTED MINOR PLANETS FOR THE CONNECTION OF DYNAMIC AND KINEMATIC COORDINATE SYSTEMS by A. Pomazan, N. Maigurova

“…The comparison of the obtained results with observations of the some ground based observatories and Hipparcos satellite shows high accuracy and uniformity of Nikolaev asteroid observations.…”
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Modelling the Galaxy in the era of Gaia by Binney, J

“…The body of photometric and astrometric data on stars in the Galaxy has been growing very fast in recent years (Hipparcos/Tycho, OGLE-3, 2-Mass, DENIS, UCAC2, SDSS, RAVE, Pan Starrs, Hermes, ...) and in two years ESA will launch the Gaia satellite, which will measure astrometric data of unprecedented precision for a billion stars. …”

Dynamics of the solar neighborhood by Binney, J

“…The Hipparcos mission has prompted a thorough reanalysis of the kinematics of the Solar neighborhood. …”

Space-Based Photometry of Binary Stars: From Voyager to TESS by John Southworth

“…This review traces the binary stars observed and the scientific results obtained from the early days of ultraviolet missions (OAO-2, Voyager, ANS, IUE), through a period of diversification (<i>Hipparcos</i>, WIRE, MOST, BRITE), to the current era of large planetary transit surveys (<i>CoRoT</i>, <i>Kepler</i>, TESS). …”
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A New Estimate of the Local Standard of Rest from Data on Young Objects by Bobylev V. V., Bajkova A. T.

“…These objects include the nearest Hipparcos O–B2.5 type stars, masers with VLBI trigonometric parallaxes, and two samples consisting of the youngest and middle-aged Cepheids. …”
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On the Component Masses of Visual Binaries by Ninkovic, S., Cvetkovic, Z.

“…Their total masses were obtained dynamically, i.e. they were calculated using the orbital elements and the new Hipparcos parallaxes. For the same pairs the total mass was also found astrophysically - by applying the mass-luminosity relation. …”
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The abundance of brown dwarfs by Binney, J

“…If these power-law mass functions are truncated at 0.001Msun, the contribution to the local density of stars lies between 0.016 and 0.039 Msun pc^-3, in conformity with the density measured dynamically from Hipparcos stars. If the mass function is generalized from a power law to a low-order polynomial in log(M), the mass in stars with M&lt;0.1Msun is either negligible or strongly divergent, depending on the order of the polynomial adopted.…”

Spectral analysis of the He-enriched sdO-star HD 127493 by Dorsch Matti, Latour Marilyn, Heber Ulrich

“…A comparison between the parallax distance measured by Hipparcos and the derived spectroscopic distance indicate that the derived atmospheric parameters are realistic. …”
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Visual Binaries: Cross-Matching and Compiling of a Comprehensive List by Isaeva A. A., Kovaleva D. A., Malkov O. Yu.

“…The resulting list1 contains 130 873 pairs, and we also provide trigonometric parallaxes for 14 319 of them drawn mostly from the Hipparcos catalogue.…”
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The Lower Main Sequence of Stars in the Solar Neighborhood: Model Predictions Versus Observation by Bartašiūtė S., Deveikis V., Raudeliūnas S., Sperauskas J.

“…We have used the Simbad database and VizieR catalogue access tools to construct the observational color-absolute magnitude diagrams of nearby K-M dwarfs with precise Hipparcos parallaxes (σπ/π ≤ 0:05). Particular attention has been paid to removing unresolved double/multiple stars and variables. …”
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Calibration of the Strömvil Photometric System by Kazlauskas A., Straižys V., Boyle R. P., Philip A. G. Davis, Laugalys V., Černis K., Sperauskas J.

“…The distances were taken from the Hipparcos catalog, and Te, log g, [Fe/H]) were collected from several literature sources and averaged.…”
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The Age of the Solar Neighbourhood by Binney, J, Dehnen, W, Bertelli, G

“…High-quality Hipparcos data for a complete sample of nearly 12000 main-sequence and subgiant stars, together with Padua isochrones, are used to constrain the star-formation history of the solar neigbourhood and the processes that stochastically accelerate disk stars. …”

The age of the solar neighbourhood by Binney, J, Dehnen, W, Bertelli, G

“…High-quality Hipparcos data for a complete sample of nearly 12 000 main-sequence and subgiant stars, together with Padua isochrones, are used to constrain the star formation history of the solar neigbourhood and the processes that stochastically accelerate disc stars. …”

Distance determination for RAVE stars using stellar models III: The nature of the RAVE survey and Milky Way chemistry by Burnett, B, Binney, J, Sharma, S, Williams, M, Zwitter, T, Bienayme, O, Bland-Hawthorn, J, Freeman, K, Fulbright, J, Gibson, B, Gilmore, G, Grebel, E, Helmi, A, Munari, U, Navarro, J, Parker, Q, Seabroke, G, Siebert, A, Siviero, A, Steinmetz, M, Watson, F, Wyse, R

“…Subsamples of stars that either have Hipparcos parallaxes or belong to well-studied clusters, inspire confidence in the formal errors. …”

Dynamics of quadruple system Finsen 332 = ADS 11640 = HIP 92027 = WDS 18455+0530 by Olević Dragomir M., Cvetković Zorica D.

“…The dynamical parallax from the obtained period and the semi major axis for pair FIN 332 Bb agrees completely with that obtained from the Hipparcos program. In the case of FIN 332 Aa a somewhat higher parallax but within the error limits following from the errors of the period and semimajor axis, is obtained and it agrees with the parallax for FIN 332 Bb. …”
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On the component masses of visual binaries by Cvetković Zorica, Ninković S.

“…Their total masses were obtained dynamically, i.e. they were calculated using the orbital elements and the new Hipparcos parallaxes. For the same pairs the total mass was also found astrophysically - by applying the mass-luminosity relation. …”
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Analysis and improvement of star identification algorithm based on singular value decomposition for star sensor by Mona Zahednamazi, Alireza toloui

“…The simulations were performed based on the Hipparcos star catalog for stars brighter than magnitude 6.5 and using MATLAB software.…”
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