guest ::
| Home > Private Collections > >DESY > >FH > L > Planck 2015 Cosmological Results > print |
| Home > Private Collections > >DESY > >FH > L > Planck 2015 Cosmological Results > print |
| 001 | 315079 | ||
| 005 | 20211110140029.0 | ||
| 020 | _ | _ | |a 978-3-945931-08-0 |
| 024 | 7 | _ | |2 datacite_doi |a 10.3204/DESY-PROC-2016-05/19 |
| 024 | 7 | _ | |2 ISSN |a 1435-8077 |
| 037 | _ | _ | |a PUBDB-2016-05614 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |0 P:(DE-HGF)0 |a Paoletti, Daniela |b 0 |
| 111 | 2 | _ | |0 C16-03-17 |2 inspire |a Magellan Workshop |c Hamburg |d 2016-03-17 - 2016-03-18 |w Germany |
| 245 | _ | _ | |a Planck 2015 Cosmological Results |
| 260 | _ | _ | |a Hamburg |b Verlag Deutsches Elektronen-Synchrotron |c 2016 |
| 295 | 1 | 0 | |a Paoletti, Daniela "Planck 2015 Cosmological Results" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg |
| 300 | _ | _ | |a 71-86 |
| 336 | 7 | _ | |2 ORCID |a CONFERENCE_PAPER |
| 336 | 7 | _ | |0 33 |2 EndNote |a Conference Paper |
| 336 | 7 | _ | |2 BibTeX |a INPROCEEDINGS |
| 336 | 7 | _ | |2 DRIVER |a conferenceObject |
| 336 | 7 | _ | |2 DataCite |a Output Types/Conference Paper |
| 336 | 7 | _ | |0 PUB:(DE-HGF)8 |2 PUB:(DE-HGF) |a Contribution to a conference proceedings |b contrib |m contrib |s 1480068969_1407 |
| 336 | 7 | _ | |0 PUB:(DE-HGF)7 |2 PUB:(DE-HGF) |a Contribution to a book |m contb |
| 490 | 0 | _ | |0 PERI:(DE-600)2450075-6 |a DESY-PROC |
| 520 | _ | _ | |a The {\it Planck} satellite has observed the full sky at nine frequencies between 30 GHz and 1 THz from 2009 to 2013. It represents the third generation of satellites dedicated to the observation of the Cosmic Microwave Background radiation (CMB). The CMB anisotropies represent the picture of primordial cosmological perturbations that originated the present structures of the Universe and {\it Planck} has performed their measurement with unprecedented accuracy in both temperature and polarization. In 2015 the {\it Planck} full mission data and results have been released to the public , here we will present some of the main cosmological results. |
| 700 | 1 | _ | |0 P:(DE-HGF)0 |a Planck Collaboration |b 1 |e Collaboration author |
| 787 | 0 | _ | |0 PUBDB-2016-05604 |a Dahmke, Stefan K.G. et. al. |d Deutsches Elektronen-Synchrotron, DESY |i isPartOf |r DESY-PROC-2016-05 |t Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy: Hamburg, Germany, March 17-18, 2016 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/315079/files/fulltext.pdf |y OpenAccess |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:315079 |p openaire |p open_access |p driver |p dnbdelivery |
| 910 | 1 | _ | |0 I:(DE-HGF)0 |6 P:(DE-HGF)0 |a IASF, Bologna |b 0 |
| 910 | 1 | _ | |0 I:(DE-HGF)0 |6 P:(DE-HGF)0 |a INFN, Bologna |b 0 |
| 915 | _ | _ | |0 StatID:(DE-HGF)0510 |2 StatID |a OpenAccess |
| 915 | _ | _ | |0 StatID:(DE-HGF)10000 |2 StatID |a Hosted Content |
| 915 | _ | _ | |0 LIC:(DE-HGF)CCBY4 |2 HGFVOC |a Creative Commons Attribution CC BY 4.0 |
| 980 | _ | _ | |a contrib |
| 980 | _ | _ | |a contb |
| 980 | _ | _ | |a I:(DE-H253)L-20120731 |
| 980 | 1 | _ | |a UNRESTRICTED |
| 980 | 1 | _ | |a FullTexts |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|