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Extreme coronagraphy with an adaptive hologram. Simulations of exo-planet imagingEstimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometryA detailed census of variable stars in the globular cluster NGC 6333 (M9) from CCD differential photometry★The transiting system GJ1214: high-precision defocused transit observations and a search for evidence of transit timing variationTransits and starspots in the WASP-6 planetary systemHigh-precision photometry by telescope defocussing – VI. WASP-24, WASP-25 and WASP-26★MOA-2010-BLG-328Lb: a Sub-Neptune orbiting very late M dwarf?Physical properties, transmission and emission spectra of the WASP-19 planetary system from multi-colour photometry★High-precision photometry by telescope defocusing – V. WASP-15 and WASP-16★MOA-2010-BLG-311: a planetary candidate below the threshold of reliable detectionMicrolensing discovery of a population of very tight, very low mass binary brown dwarfsA giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251Flux and color variations of the doubly imaged quasar UM673MOA-2010-BLG-523: "Failed planet" = RS CVn starMOA-2010-BLG-073L: an m-dwarf with a substellar companion at the Planet/Brown dwarf boundaryMicrolensing binaries with candidate brown dwarf companionsA brown dwarf orbiting an M-dwarf: MOA 2009–BLG–411LHigh-precision photometry by telescope defocusing - IV. Confirmation of the huge radius of WASP-17 bA new type of ambiguity in the planet and binary interpretations of central perturbations of high-magnification gravitational microlensing eventsCharacterizing low-mass binaries from observation of long-timescale caustic-crossing gravitational microlensing eventsOGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly -- brown dwarf or stellar binary?MOA 2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion, and detection of blended lightCharacterizing lenses and lensed stars of high-magnification single-lens gravitational microlensing events with lenses passing over source starsMicrolensing binaries discovered through high-magnification channelDiscovery and mass measurements of a cold, 10 earth mass planet and its host starMOA-2009-BLG-387Lb: a massive planet orbiting an M dwarfFlux and color variations of the quadruply imaged quasar HE 0435-1223A much lower density for the transiting extrasolar planet WASP-7A Sub-Saturn mass planet, MOA-2009-BLG-319LbHigh-precision photometry by telescope defocusing - III. The transiting planetary system WASP-2★OGLE-2009-BLG-092/MOA-2009-BLG-137: a dramatic repeating event with the second perturbation predicted by real-time analysisFrequency of solar-like systems and of ice and gas giants beyond the snow line from high-magnification microlensing events in 2005-2008OGLE 2008-BLG-290: an accurate measurement of the limb darkening of a galactic bulge K giant spatially resolved by microlensingRealisation of a fully-deterministic microlensing observing strategy for inferring planet populationsERRATUM: “PHYSICAL PROPERTIES OF THE 0.94 DAY PERIOD TRANSITING PLANETARY SYSTEM WASP-18” (2009, ApJ, 707, 167)Physical properties of the 0.94-Day period transiting planetary system WASP-18High-precision photometry by telescope defocussing - II. The transiting planetary system WASP-4High-precision photometry by telescope defocusing - I. The transiting planetary system WASP-5The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classesManaging GRB afterglows optical/IR observations in the web 2.0 era
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description
Italiaans onderzoeker
@nl
forsker
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researcher
@en
հետազոտող
@hy
name
D. Ricci
@ast
D. Ricci
@nl
D. Ricci
@sl
Davide Ricci
@en
Davide Ricci
@es
Davide Ricci
@nb
Davide Ricci
@sq
type
label
D. Ricci
@ast
D. Ricci
@nl
D. Ricci
@sl
Davide Ricci
@en
Davide Ricci
@es
Davide Ricci
@nb
Davide Ricci
@sq
altLabel
D. Ricci
@en
prefLabel
D. Ricci
@ast
D. Ricci
@nl
D. Ricci
@sl
Davide Ricci
@en
Davide Ricci
@es
Davide Ricci
@nb
Davide Ricci
@sq
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P1153
7005630862
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0000-0002-9790-0552