about
Joint analysis of BICEP2/keck array and Planck DataPlanck intermediate results: XXXII. The relative orientation between the magnetic field and structures traced by interstellar dustPlanck 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 latitudesThe second-generation guide star catalog: description and propertiesPlanck 2013 results. XXIII. Isotropy and statistics of the CMBPlanckpre-launch status: Design and description of the Low Frequency InstrumentPlanck 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 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. 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 effect
P50
Q27012165-BAB0A61C-F4C1-4E54-AC32-5C3E3370D4E7Q27016153-D627246D-9FED-4CEE-90B1-5C778B542289Q27016861-E4B7DC16-87BD-4723-84A9-1A828362AB28Q27019766-7DF19578-48FD-48ED-BE6D-689D5704B2DBQ27019812-10C8D2C0-D9A2-4A29-9758-5B3D58FF1D41Q27019857-B666B4F6-4548-4E3E-8E26-9B92706673C4Q54001693-7694ACF4-9A0D-491A-9921-329D77B29873Q55691015-EC603B13-EF78-4CD6-9FFB-F68B8CF3F6C2Q55691065-3F5D9C02-C00D-43B9-BD8E-CC62EB39D47AQ55691144-D71464D6-336C-4949-A749-385D52C1CAF1Q55877492-C18D44B3-5DBC-4BDD-BA38-7B698CEAAF80Q55966655-BAF46D6B-B3F2-4F88-95AB-5EA4DCBBD7FFQ55980389-1BEB7BCB-8E22-412A-B837-B7A06D2041DAQ55983318-A0B89D06-BBCF-4591-8723-01FB4C6B9EBDQ56039962-2286BD26-A25B-464A-925D-932E2B56D50FQ56041097-2513315D-511A-447E-8646-53665EBF65EFQ56057757-0460417D-1DEF-4358-9638-79B317C91953Q56069928-DC24EBFB-35AB-4D3E-80D5-7F735FD19376Q56224847-BAF94F64-E03E-4D5E-84A7-1B43DAE73886Q56555882-32682BA2-39E2-483C-ACA1-322A446C93C8Q56933869-A73E27C6-1EAB-43C5-8E7E-B317200932E3Q56934014-D4AC0C55-12EB-44B7-8E7C-773A6542A79DQ56934020-A5EE04C3-774D-4D87-8E38-A8622B3DC2B7Q57548959-C8A3AD91-7213-4C07-9662-32D59C07DA6CQ57548961-7E353FC5-1516-4AB9-8098-BD227910234EQ57548965-6ABEFDCD-1EA7-41AE-B4A3-B9AA6CF34019Q57548977-8D070CCA-73D2-4131-8F80-93D16F9A86DBQ57548978-0C29ACF2-3CC3-4D9A-B6AC-EDA4D92CC527Q57548980-D44775F2-EA34-4A3D-B3E1-A94A75BDAC9CQ57548981-BFFD6861-351C-4764-9BA0-F5550DBEB717Q57548983-8E495B9F-8863-48F0-BC00-6244D6DF9396Q57548986-6066EF4C-F21C-480A-980C-98A640D71E2FQ57548989-1CC2A3E8-B0D7-4962-AB63-A8D3F718EAE5Q57548991-E44C3F07-CCA4-4D8B-9B09-EC45ACF80344Q57548994-B71E2226-CC53-45D1-8A78-B65BD38B274AQ57548996-339B931B-565E-4A91-8426-E28F0E3A9444Q57549000-E99971EC-25EB-460C-9B9B-577151EAB0C3Q57549002-0E094E31-7E2A-47B1-9476-562ED6874222Q57549005-8060982E-517E-46EC-8098-DB41EF9880E5Q57549007-DC337942-5A8B-4C42-98E3-5B259545F1EC
P50
description
hulumtues
@sq
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
A. Zacchei
@nl
A. Zacchei
@sl
Andrea Zacchei
@en
Andrea Zacchei
@es
type
label
A. Zacchei
@nl
A. Zacchei
@sl
Andrea Zacchei
@en
Andrea Zacchei
@es
altLabel
A. Zacchei
@en
prefLabel
A. Zacchei
@nl
A. Zacchei
@sl
Andrea Zacchei
@en
Andrea Zacchei
@es
P106
P1153
56273947300
P21
P31
P496
0000-0003-0396-1192