Context. The winter seeing at Concordia is bimodal, i.e. either excellent or quite poor, depending on the altitude above the snow surface. We study the temporal behavior of the good seeing sequences. Efficient exploitation of extremely good seeing conditions with an adaptive optics system requires long integrations.Aims: We examine the temporal...
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July 2010 (v1)Journal articleUploaded on: December 4, 2022
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2009 (v1)Conference paper
The optical turbulence above Dome C in winter is mainly concentrated in the first tens of meters above the ground. The properties of this so-called surface layer were investigated during the last two winterover by a set of sonics anemometers placed on a 45 m high tower. These anemometers provide measurements of the temperature and the wind...
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June 2009 (v1)Journal article
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August 2014 (v1)Journal article
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November 2013 (v1)Journal article
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August 2012 (v1)Conference paper
We present long term site testing statistics based on DIMM and GSM data obtained at Dome C, Antarctica. These data have been collected on the bright star Canopus since the end of 2003. We give values of the integrated turbulence parameters in the visible (wavelength 500 nm). The median value we obtained for the seeing are 1.2 arcsec, 2.0 arcsec...
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2009 (v1)Conference paper
So as to prepare future observations of terrestrial extrasolar planets liable to shelter life, we attempt to detect the life on the Earth seen as a dot. We use the Moon Earthshine, in which any place reflects the totality of the enlightened part of Earth facing the Moon. Observing from OHP and from ESO, we detected terrestrial chlorophyll in...
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December 2015 (v1)Journal articleMonitoring the optical turbulence in the surface layer at Dome C, Antarctica, with sonic anemometers
The optical turbulence above Dome C in winter is mainly concentrated in the first tens of metres above the ground. Properties of this so-called surface layer (SL) were investigated during the period 2007–2012 by a set of sonic anemometers placed on a 45 m high tower. We present the results of this long-term monitoring of the refractive index...
Uploaded on: February 28, 2023 -
November 2018 (v1)Journal article
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2016 (v1)Conference paper
International audience
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2009 (v1)Journal article
Astronomy and Astrophysics, 511, p. 36 (2009)
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2012 (v1)Conference paper
The ASTEP program is dedicated to exo-planet transit search from the Concordia Station located at Dome C, Antarctica. It comprises two instruments: a fixed 10cm refractor pointed toward the celestial South Pole, and a 400mm Newton telescope with a 1x1 degree field of view. This work focuses on the latter instrument. It has been installed in...
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2016 (v1)Conference paper
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Uploaded on: December 4, 2022