The 10 parsec sample
Revised census of the 10 parsecs sample. The catalogue contains 540 stars, brown dwarfs, and exoplanets in 339 systems, within 10 pc from the Sun. This list is as volume-complete as possible from current knowledge and it provides benchmark stars that can be used, for instance, to define calibration ...
MEDUSA: Marine benthic Ecological Data from Underwater imagery Surveys of sub-Antarctic Crozet environments
Inscribed on the UNESCO World Heritage list, the sub-Antarctic Crozet archipelago is located in a region facing significant environmental changes impacting a poorly known marine biodiversity. Underwater imagery constitutes a valuable non-invasive approach for gathering ecological data and improving ...
PROTEKER: a near-shore submarine observatory in the Kerguelen Islands for the long-term monitoring of benthic habitats
PROTEKER is a pilot program that aims at establishing a baseline for assessing the impact of climate change on near-shore marine ecosystems of the Kerguelen Islands by implementing an ecological and genetic monitoring at reference sites. The high diversity of coastal marine ecosystems is usually ...
Gaia Data Release 3
Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006. Both the spacecraft and the payload were built by European industry. The involvement of the scientific community focusses on data processing for which the ...
Gaia early Data Release 3
Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006. Both the spacecraft and the payload were built by European industry. The involvement of the scientific community focusses on data processing for which the ...
Gaia Data Release 2
Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006,. Both the spacecraft and the payload were built by European industry. The involvement of the scientific community focusses on data processing for which the ...
Gaia Data Release 1
Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original interferometric concept was changed to a direct-imaging approach. Both the spacecraft and the payload were built by ...
Carbonate dissolution by euendolithe cyanobacterium
Bioerosion is the process of destruction of rocks by living organisms. The bioerosion of biogenic carbonates by so-called "euendolithic" cyanobacteria (which live in rocks) is a major but poorly quantified process, causing, among other things, the disintegration of coral reefs. Euendolitic ...
Satellite images of cloud types products in West Africa from March to August in 2017
It is products developped by Meteo France through the SAF application, showing the types of clouds in function of their elevation.
SISMEAUCLIM
This project is based on three disciplines: seismology, hydrogeology and climatology. It aims to develop a new approach to monitor hydrogeological reservoirs, in particular karst aquifers, subject to extreme climatic events. The objective is to carry out 4D imaging during floods in a watershed ...
Mesures urbaines de la température dans l’agglomération du Grand Dijon (MUSTARDijon)
Air temperature and monitoring in the Dijon agglomeration for high-resolution monitoring of the urban heat island (50 stations, record sampling every 20 minutes, period June 2014 onwards)
Mobile temperature measurements of air temperature in Dijon
Air temperature and monitoring in the Dijon agglomeration by bike (one measurement every 5m) to characterize the urban heat island at very high resolution along constant transects
The Gaia catalogue of nearby stars
We provide the community with a large, well-characterised catalogue of objects in the solar neighbourhood. This is a primary benchmark for measuring and understanding fundamental parameters and descriptive functions in astronomy. We have produced a catalogue of 331 312 objects that we estimate ...
Pollen analysis - Montlebon (F-25), Sur la Vigne 1 (Morteau A)
Natural site: wet meadow. 99 palynological samples + 4 radiocarbon datings. Drilling of 28.10 meters length.
Pollen analysis - Montlebon (F-25), La Vigne 2
Natural site: wet meadow. 22 palynological samples. From 3,90 to 18,85 meters length: extension of Morteau Stade and Sur la Seigne transect lines.
Pollen analysis - Lavancia-Epercy (F-39), Dortan travertine quarry
Natural site: travertine quarry ("Tuff of Dortan"). 3 palynological samples + 1 radiocarbon dating: 9100 ± 180 BP.
Pollen analysis - Montlebon (F-25), Transect S4
Natural site: wet meadow. 6 palynological samples. From 10.20 to 13.20 meters. Atypical results. Extension of Morteau Stade et Sur la Seigne transect lines.
Pollen analysis - Montlebon (Morteau-Montlebon) (F-25), Transects II-6, II-7 et III-7
Natural site; wet meadow. 14 palynological samples. Approximate geographical coordinates: 3 transect lines.
Pollen analysis - Montlebon (F-25), Sur La Seigne
Natural site: wet meadow. 58 palynological samples + 2 radiocarbon datings. 10,40 meters length.
Pollen analysis - Montlebon (F-25), Transect S3
Natural site: wet meadow. 24 palynological samples. From 4.40 to 25,70 meters length: extension of Morteau Stade and Sur la Seigne transect lines.
Pollen analysis - Morteau (F-25), Moulin Bournez
Natural site; weat meadow. 126 palynological samples + 2 radiocarbon datings. 33,57 meters length drilling.
Pollen analysis - Morteau (F-25), Transect S2
Natural site; weat meadow. 16 palynological samples. Many drillings along a transect ligne: 6.0 to 12.45 meters length.
Pollen analysis - Morteau (F-25), Transect S1
Natural site; weat meadow. 18 palynological samples. Many drillings along a transect ligne: 4.20 to 12.30 meters length.
Pollen analysis - Morteau (F-25), Stade
Natural site; weat meadow. 62 palynological samples. 12 meters length drilling.
Accurate SB2 orbits for 10 binaries and masses of the components of 5 binaries
Double-lined spectroscopic binaries (SB2s) are one of the main sources of stellar masses, as additional observations are only needed to give the inclinations of the orbital planes in order to obtain the individual masses of the components. For this reason, we are observing a selection of SB2s using ...
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