Institution
Collège de France
Education•Paris, France•
About: Collège de France is a education organization based out in Paris, France. It is known for research contribution in the topics: Population & Receptor. The organization has 6541 authors who have published 11983 publications receiving 648742 citations. The organization is also known as: College de France.
Topics: Population, Receptor, Dopamine, Dopaminergic, Neural crest
Papers published on a yearly basis
Papers
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TL;DR: In this paper, the temporal relationship between meltwater pulse 1a (mwp-1a) and the climate history of the last deglaciation remains a subject of debate.
Abstract: The temporal relationship between meltwater pulse 1a (mwp-1a) and the climate history of the last deglaciation remains a subject of debate. By combining the Greenland Ice Core Project d18O ice core record on the new Greenland ice core chronology 2005 timescale with the U/Th-dated Barbados coral record, we conclusively derive that mwp-1a did not coincide with the sharp Bolling warming but instead with the abrupt cooling of the Older Dryas. To evaluate whether there is a relationship between meltwater injections, North Atlantic Deep Water (NADW) formation, and climate change, we present a high-resolution record of NADW flow intensity from Eirik Drift through the last deglaciation. It indicates only a relatively minor 200-year weakening of NADW flow, coincident with mwp-1a. Our compilation of records also indicates that during Heinrich event 1 and the Younger Dryas there were no discernible sea level rises, and yet these periods were characterized by intense NADW slowdowns/shutdowns. Clearly, deepwater formation and climate are not simply controlled by the magnitude or rate of meltwater addition. Instead, our results emphasize that the location of meltwater pulses may be more important, with NADW formation being particularly sensitive to surface freshening in the Arctic/Nordic Seas.
204 citations
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TL;DR: Functional imaging data on humans reveal a network of cortical areas that respond to polymodal stimuli conveying motion information and it is suggested that this area constitutes the human equivalent of monkey area VIP.
204 citations
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TL;DR: A new measurement of the 1S-3S two-photon transition frequency of hydrogen is presented, realized with a continuous-wave excitation laser at 205 nm on a room-temperature atomic beam, with a relative uncertainty of 9×10^{-13}.
Abstract: We present a new measurement of the $1S\ensuremath{-}3S$ two-photon transition frequency of hydrogen, realized with a continuous-wave excitation laser at 205 nm on a room-temperature atomic beam, with a relative uncertainty of $9\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}13}$. The proton charge radius deduced from this measurement, ${r}_{p}=0.877(13)\text{ }\text{ }\mathrm{fm}$, is in very good agreement with the current CODATA-recommended value. This result contributes to the ongoing search to solve the proton charge radius puzzle, which arose from a discrepancy between the CODATA value and a more precise determination of ${r}_{p}$ from muonic hydrogen spectroscopy.
204 citations
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University of Geneva1, Sapienza University of Rome2, Queen Mary University of London3, Jet Propulsion Laboratory4, California Institute of Technology5, University of California, Berkeley6, Lawrence Berkeley National Laboratory7, University of California, Santa Barbara8, CERN9, Instituto Superior Técnico10, Collège de France11, University of Rome Tor Vergata12, University of Massachusetts Amherst13, University of Toronto14
TL;DR: The angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, is used to constrain the geometry of the universe and new constraints on the fractional matter density and the cosmological constant are obtained.
Abstract: We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Ω is constrained to be 0.85 ≤ Ω ≤ 1.25 at the 68% confidence level. Combined with the COBE measurement, the data on degree scales from the Microwave Anisotropy Telescope in Chile, and the high-redshift supernovae data, we obtain new constraints on the fractional matter density and the cosmological constant.
204 citations
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Lawrence Livermore National Laboratory1, University of California, Berkeley2, Australian National University3, University of California, Davis4, University of Paris-Sud5, DSM6, Collège de France7, University of Washington8, University of Notre Dame9, University of La Serena10, Institut d'Astrophysique de Paris11, University of California, San Diego12, University of Sheffield13, Massachusetts Institute of Technology14, European Southern Observatory15, Max Planck Society16, University of Oxford17
TL;DR: The EROS and MACHO collaborations have each published upper limits on the amount of planetary-mass dark matter in the Galactic halo obtained from gravitational microlensing searches as discussed by the authors.
Abstract: The EROS and MACHO collaborations have each published upper limits on the amount of planetary-mass dark matter in the Galactic halo obtained from gravitational microlensing searches. In this Letter, the two limits are combined to give a much stronger constraint on the abundance of low-mass MACHOs. Specifically, objects with masses 10−7 Mm10−3 M make up less than 25% of the halo dark matter for most models considered, and less than 10% of a standard spherical halo is made of MACHOs in the 3.5×10−7 M
204 citations
Authors
Showing all 6597 results
Name | H-index | Papers | Citations |
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Pierre Chambon | 211 | 884 | 161565 |
Irving L. Weissman | 201 | 1141 | 172504 |
David R. Williams | 178 | 2034 | 138789 |
Kari Alitalo | 174 | 817 | 114231 |
Pierre Bourdieu | 153 | 592 | 194586 |
Stanislas Dehaene | 149 | 456 | 86539 |
Howard L. Weiner | 144 | 1047 | 91424 |
Alain Fischer | 143 | 770 | 81680 |
Yves Agid | 141 | 669 | 74441 |
Michel Foucault | 140 | 499 | 191296 |
Jean-Pierre Changeux | 138 | 672 | 76462 |
Jean-Marie Tarascon | 136 | 853 | 137673 |
K. Ganga | 132 | 272 | 99004 |
Jacques Delabrouille | 131 | 354 | 94923 |
G. Patanchon | 128 | 241 | 87233 |