guest ::
| Home > Publications database > Very-high-energy quasars hint at ALPs > print |
| 001 | 408339 | ||
| 005 | 20211110151242.0 | ||
| 010 | _ | _ | |a |
| 020 | _ | _ | |a 978-3-935702-83-6 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2013-04/roncadelli_marco |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 037 | _ | _ | |a PUBDB-2018-02792 |
| 041 | _ | _ | |a English |
| 088 | 1 | _ | |a DESY-PROC-2013-04 |
| 088 | _ | _ | |a DESY-PROC-2013-04 |2 DESY |
| 100 | 1 | _ | |a Roncadelli, M. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 9th Patras Workshop on Axions, WIMPs and WISPs |c Mainz |d 2013-06-24 - 2013-06-28 |g AXION-WIMP 2013 |0 C13-06-24.5 |2 inspire |w Germany |
| 245 | _ | _ | |a Very-high-energy quasars hint at ALPs |
| 260 | _ | _ | |a Hamburg |c 2013 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Roncadelli, M. "Very-high-energy quasars hint at ALPs" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz |
| 300 | _ | _ | |a 89-92 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a Report |0 PUB:(DE-HGF)29 |2 PUB:(DE-HGF) |m report |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1533892981_17297 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a Contribution to a book |0 PUB:(DE-HGF)7 |2 PUB:(DE-HGF) |m contb |
| 490 | 0 | _ | |a DESY-PROC |0 PERI:(DE-600)2450075-6 |
| 520 | _ | _ | |a One of the mysteries of very-high-energy (VHE) astrophysics is the observatio of flat spectrum radio quasars (FSRQs) above about 30 GeV, because at those energies their broad line region should prevent photons produced by the central engine to escape. Although a few astrophysical explanations have been put forward, they are totally ad hoc. We show that a natural explanation emerges within the conventional models of FSRQs provided that photon-ALP oscillations take place inside the source for the model parameters within an allowed range. |
| 536 | _ | _ | |a 899 - ohne Topic (POF3-899) |0 G:(DE-HGF)POF3-899 |c POF3-899 |f POF III |x 0 |
| 588 | _ | _ | |a Dataset connected to GVK |
| 650 | _ | 7 | |a Hypothetisches Teilchen |0 (DE-588)4220935-3 |2 gnd |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a Galanti, G. |0 P:(DE-HGF)0 |b 1 |
| 700 | 1 | _ | |a Tavecchio, F. |0 P:(DE-HGF)0 |b 2 |
| 700 | 1 | _ | |a Bonnoli, G. |0 P:(DE-HGF)0 |b 3 |
| 787 | 0 | _ | |a Oberlack, Uwe et. al. |0 PUBDB-2015-05816 |r DESY-PROC-2013-04 |i isPartOf |t Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/408339/files/fulltext.pdf |y OpenAccess |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:408339 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 913 | 1 | _ | |a DE-HGF |b Programmungebundene Forschung |l ohne Programm |1 G:(DE-HGF)POF3-890 |0 G:(DE-HGF)POF3-899 |2 G:(DE-HGF)POF3-800 |v ohne Topic |x 0 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF3 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 4.0 |0 LIC:(DE-HGF)CCBY4 |2 HGFVOC |
| 920 | 1 | _ | |0 I:(DE-H253)L-20120731 |k L |l Bibliothek und Dokumentation |x 0 |
| 980 | _ | _ | |a contrib |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | _ | _ | |a report |
| 980 | _ | _ | |a contb |
| 980 | _ | _ | |a I:(DE-H253)L-20120731 |
| 980 | 1 | _ | |a FullTexts |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|