about
Planck 2013 results. I. Overview of products and scientific resultsJoint analysis of BICEP2/keck array and Planck DataPlanck 2013 results. XVI. Cosmological parametersPlanck early results. III. First assessment of the Low Frequency Instrument in-flight performancePlanck early results. XXII. The submillimetre properties of a sample of Galactic cold clumpsPlanck early results. XXVI. Detection with Planck and confirmation by XMM-Newton of PLCK G266.6–27.3, an exceptionally X-ray luminous and massive galaxy cluster at z ~ 1Cosmology and Fundamental Physics with the Euclid Satellite.Backreaction during inflation: a physical gauge invariant formulation.Planck intermediate results XXV. The Andromeda galaxy as seen by PlanckPlanck intermediate results XXIII. Galactic plane emission components derived from Planck with ancillary dataPlanck 2013 results. XXIII. Isotropy and statistics of the CMBProbing Inflation with CMB PolarizationPlanck2013 results. XXVII. Doppler boosting of the CMB: Eppur si muovePlanck intermediate results XIII. Constraints on peculiar velocitiesPlanck 2013 results. XXV. Searches for cosmic strings and other topological defectsSPACE: the spectroscopic all-sky cosmic explorerPlanckearly results. V. The Low Frequency Instrument data processingPlanck pre-launch status: The Planck missionPlanckpre-launch status: ThePlanck-LFI programmePlanck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulaePlanck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dustPlanck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visiblePlanck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarizationPRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paperPlanck 2013 results. II. Low Frequency Instrument data processingPlanck 2013 results. III. LFI systematic uncertaintiesPlanck 2013 results. IV. Low Frequency Instrument beams and window functionsPlanck 2013 results. IX. HFI spectral responsePlanck 2013 results. V. LFI calibrationPlanck 2013 results. VI. High Frequency Instrument data processingPlanck 2013 results. VII. HFI time response and beamsPlanck 2013 results. VIII. HFI photometric calibration and mapmakingPlanck 2013 results. X. HFI energetic particle effects: characterization, removal, and simulationPlanck 2013 results. XI. All-sky model of thermal dust emissionPlanck 2013 results. XII. Diffuse component separationPlanck 2013 results. XIII. Galactic CO emissionPlanck 2013 results. XIV. Zodiacal emissionPlanck 2013 results. XIX. The integrated Sachs-Wolfe effectPlanck 2013 results. XV. CMB power spectra and likelihoodPlanck 2013 results. XVII. Gravitational lensing by large-scale structure
P50
Q15217920-9D5C471E-1497-4595-A03A-0F175C75ACA6Q27012165-6CB1CA49-4B2A-48C2-883A-1BE72FB2D248Q27016861-FE2FE1B2-E19A-4326-8518-63DD2E3098AFQ27019766-C4428B74-AC86-4CD0-879B-D51A53CB93A6Q27019812-9ECD2125-03B1-4761-9BAD-35812E881A52Q27019857-0ADF9EA2-2287-4D03-9A73-E6709D2BA216Q47098810-6077E6A7-FFC5-4073-92B7-7D2711405E7EQ51575982-F61339D0-BC1F-44D1-9F9C-B73D8597B73CQ55691065-17AAF869-AF3E-460A-AF07-18786B302100Q55691144-7604365C-7551-454D-9A30-66899ECA2245Q55980389-2CC09909-A282-4139-B5E9-6C68ECC5BDEBQ56039944-57323176-9430-4958-801C-775A22D7BD4DQ56041097-C354C01D-86BF-4F17-A0D4-88649E2FE36AQ56057757-4FF83005-A1A7-4D8C-873B-B92C793AEFDAQ56224847-4034FD50-2C51-453F-9A78-14CBF5DF77F0Q56555882-1AA2F4F9-DBCF-4515-97AC-D1771C75AC5CQ56933869-463D841A-C636-4CCD-9EE8-D88F254BCB31Q56934014-00135627-4FA4-46A2-BF04-5FA8943DE4B7Q56934020-0CE817C2-5B65-42A5-8921-5B556B93224AQ57548959-57F98E53-90CD-4B83-9A5C-51E3603A9025Q57548961-F094C5B4-89F3-49CE-A2E8-E99B02EE3D0BQ57548963-F17AD61A-FC77-4873-A5A5-A3B08E7BDE95Q57548965-14D1131F-72BA-4F4D-8E8D-A4B14096BF2AQ57548976-EDAFB6FE-9503-4EB7-A22A-D77AB0425B56Q57548977-39050F5C-4048-4469-A009-A6533CAA15ACQ57548978-BA2A932D-EFD6-4943-AB09-E8ACD5EEC287Q57548980-C4E11BEA-3F6D-4A74-B03A-0C111F8BF645Q57548981-936B23DD-E855-4B4A-96F9-5E3D86693446Q57548983-3C224A94-C464-479A-A1BB-75E516B98F32Q57548986-A7750BCC-83BC-44E3-B75A-00273EEA5B45Q57548989-C6180BFF-A0D9-48A6-BB87-CA99D238AC89Q57548991-552DADE6-2138-49C0-B77C-9C3CB7CC535AQ57548994-16446AC9-5814-4B96-BF6C-D3A5391B14E3Q57548996-5A3BE546-6C81-4E0F-ABB9-07DB93238B05Q57549000-A4076CB3-458C-4C31-8008-0DCF17C23212Q57549002-C9270364-DFAC-40F0-B271-C59D92DE346EQ57549005-283149BA-65E1-4F12-B163-3E796C6D0D2DQ57549007-7325AED9-8FCE-4C12-B913-7794C9EA1216Q57549010-1D473A6D-1A22-48CA-B3A6-A4C8CA5D8595Q57549013-D91F5482-75A7-4EA9-B2DA-D0D3512A13BE
P50
description
hulumtues
@sq
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
F. Finelli
@nl
F. Finelli
@sl
Fabio Finelli
@en
Fabio Finelli
@es
type
label
F. Finelli
@nl
F. Finelli
@sl
Fabio Finelli
@en
Fabio Finelli
@es
altLabel
F. Finelli
@en
prefLabel
F. Finelli
@nl
F. Finelli
@sl
Fabio Finelli
@en
Fabio Finelli
@es
P106
P21
P31
P496
0000-0002-6694-3269