GRETSI 2005, n/a, pp. 257-260 (2005)
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2005 (v1)Conference paperUploaded on: December 3, 2022
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2005 (v1)Conference paper
PSIP 2005, Paper 01-03, (2005)
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2003 (v1)Conference paper
Impacts on Earth, The Spring School of Astronomy and Astrophysics of Goutelas, Lecture Notes in Physics 505, pp. 3-30 (2003)
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2011 (v1)Journal article
International audience
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2011 (v1)Journal article
International audience
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2010 (v1)Journal article
International audience
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2004 (v1)Journal article
Icarus, 168, pp. 374-384 (2004)
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2004 (v1)Conference paper
35th COSPAR Scientific Assembly, 2205, n/a, (2004)
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2005 (v1)Journal article
Icarus, 179, pp. 304-324 (2005)
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2007 (v1)Journal article
EAS Publications Series, 25, pp. 339-342 (2007)
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2007 (v1)Conference paper
We present the results of the first light of CORONA obtained during the summer campaign 2005 at Dome C. The CORONA experiment uses an automated 14primeprime antarctized telescope for its remote operation from the Concordia station. The instrument includes an Achromatized Phase Knife Coronagraph (APKC) with no tip-tilt correction. The high...
Uploaded on: December 4, 2022 -
2007 (v1)Conference paper
We present the results of the first light of CORONA obtained during the summer campaign 2005 at Dome C. The CORONA experiment uses an automated 14primeprime antarctized telescope for its remote operation from the Concordia station. The instrument includes an Achromatized Phase Knife Coronagraph (APKC) with no tip-tilt correction. The high...
Uploaded on: February 22, 2023 -
2011 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2007 (v1)Publication
n/a, pages (2007)
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2006 (v1)Journal article
Icarus, 180, pp. 565-567 (2006)
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2006 (v1)Conference paper
SF2A - Scientific Highlights 2005, eds. F. Casoli, T. Contini, J.-M. Hameury and L. Pagani, EDP Sciences - Conference Series n/a, pp. 277-278 (2006)
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2005 (v1)Journal article
Icarus, 179, pp. 297-303 (2005)
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2011 (v1)Journal article
International audience
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2022 (v1)Journal article
This paper presents orbits and masses for 22 visual double stars, partly derived using their last observations made with the speckle camera PISCO. For 13 of them we have determined their first-time orbits. Masses were calculated from Hipparcos and Gaia parallaxes when available, and from dynamical parallaxes otherwise. They are compared with...
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2007 (v1)Publication
n/a, pages (2007)
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2006 (v1)Conference paper
Advances in Stellar Interferometry, eds. J. D. Monnier, M. Schöller and W. C. Danchi, SPIE 6269, p. 170 (2006)
Uploaded on: December 4, 2022