about
Joint 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 ~ 1Planck 2015 results. XIII. Cosmological parametersPlanck intermediate results XXXI. Microwave survey of Galactic supernova remnantsPlanck intermediate results XXV. The Andromeda galaxy as seen by PlanckPlanck intermediate results XXIII. Galactic plane emission components derived from Planck with ancillary dataPlanck intermediate results XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudesPlanck 2013 results. XXIII. Isotropy and statistics of the CMBPlanck 2015 resultsPlanck2013 results. XXVII. Doppler boosting of the CMB: Eppur si muovePlanck intermediate results XIII. Constraints on peculiar velocitiesPlanck 2015 resultsPlanck 2013 results. XXV. Searches for cosmic strings and other topological defectsESPRESSO: The next European exoplanet hunterPlanckearly 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. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulencePlanck 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 polarizationPlanck 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 likelihood
P50
Q27012165-F455A13E-0E76-4A90-BCE7-6B62F602F2E1Q27016861-5750B3FE-F0ED-4964-AE9E-26060D76DA1CQ27019766-9EF61B5E-A913-4926-AA0C-BDA8F7AAAF81Q27019812-5417F49C-7803-4360-B3FE-0D605E91445EQ27019857-402B14C8-6B52-4374-813F-03A9CE1AF3ACQ54001693-2EB35662-EF68-451A-B0C4-926EB7616B1AQ55691015-2CEA4F1F-93EF-4A27-BB6E-402EEE157D73Q55691065-B4AD0A30-8A2E-4610-B781-880DEA3CB371Q55691144-20BAC176-DC27-491A-90D9-A04FAF37B9DCQ55877492-F532FC91-8E01-45AD-8E15-3512A14C9360Q55980389-2E8DBDEC-4B35-4B38-B8D3-FE1557910262Q56039962-BB39A621-D96F-4722-A9F3-45EF4445B951Q56041097-37DC3156-A31F-4A74-A54F-F11ABDF9A47CQ56057757-83D5F46B-8384-4005-9A2E-1E1102657DA5Q56069928-74C9C8D9-3CE6-40CF-822C-995B9B14C70EQ56224847-E788AF39-4EF3-4C12-B350-9B5430B98B8EQ56672877-BB403FE4-D6CF-4C18-B6DF-79BAC766CE30Q56933869-16EC6661-6E11-4890-BDFA-57300FCF2EC0Q56934014-B59D289A-0D17-479F-B49E-A7430F71C0C7Q56934020-5142082C-94B6-4155-8AEF-A4818DE60808Q57548959-F992DAE2-8702-4A1F-94F6-9CB042061493Q57548961-AC6EDA16-8572-49CB-BB3D-7B780487A047Q57548962-57174B6D-BBB2-4817-AAFA-C5B1D815E51CQ57548963-D638875A-8079-41D4-A28D-4BC57A3D991DQ57548965-44BA8A15-1A00-4346-BDC6-C24BCD2E29B1Q57548977-4463BAD2-3547-4538-A8D1-5FB3577CD7AEQ57548978-A41D9958-0556-4C6B-986C-81D88FAE2D66Q57548980-916839C6-50F3-4CD5-B920-719ADD477172Q57548981-A55B9023-7B60-4ABF-8FF1-529BD31E1E51Q57548983-508FC0E0-E757-4E00-81C1-40C062FCBAFFQ57548986-8783FB97-AC13-48F4-95D0-6E22F4A83E57Q57548989-370BBCD2-EED4-4BFE-A9CC-32B5A6F909EBQ57548991-F30FFF04-251D-4C4D-BBC5-ABF022578E9AQ57548994-4751407F-6819-4C5D-BE75-63392BC9D12AQ57548996-01D7F1A3-9798-451F-A6CD-C20F25B71DABQ57549000-E7E8503C-B947-4498-8A6E-6D792C937443Q57549002-97392A6F-B1B4-459D-87CD-C074482A907CQ57549005-AB3986FC-CFA2-4951-8B68-FEAEE274D6E3Q57549007-93B86334-4C6C-4014-AAD1-187413EB8CE1Q57549010-96E2E09D-B2DB-4195-8CB5-A1623C1CC9D0
P50
description
hulumtues
@sq
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
S. Galeotta
@nl
S. Galeotta
@sl
Samuele Galeotta
@en
Samuele Galeotta
@es
type
label
S. Galeotta
@nl
S. Galeotta
@sl
Samuele Galeotta
@en
Samuele Galeotta
@es
altLabel
S. Galeotta
@en
prefLabel
S. Galeotta
@nl
S. Galeotta
@sl
Samuele Galeotta
@en
Samuele Galeotta
@es
P106
P1153
14630273900
P21
P31
P496
0000-0002-3748-5115