-
Mathieu Servillat (LUTH, Observatoire de Paris)07/09/2020 14:00
-
Mireille Louys07/09/2020 14:10
-
Mathieu Servillat (LUTH, Observatoire de Paris)07/09/2020 14:20
-
Mathieu Servillat (LUTH, Observatoire de Paris)07/09/2020 14:40
-
Mme Michèle Sanguillon (LUPM)07/09/2020 14:55
-
François Bonnarel (CDS ObAS CNRS Université de Strasbourg)07/09/2020 15:10
-
Mathieu Servillat (LUTH, Observatoire de Paris)07/09/2020 15:25
-
Gilles Landais (CDS)07/09/2020 16:00
-
Vincenzo Galluzzi (INAF - Osservatorio Astronomico di Trieste)07/09/2020 16:20
The high-frequency (> 20 GHz), bright flux density (> 200 mJy) extragalactic radio sources (ERSs) population is dominated by blazars. Multi-frequency (and multi-epoch) polarimetry is invaluable to study magnetic fields and plasma in the inner and unresolved regions of their relativistic jets. Moreover, as ERSs constitute an important foreground for CMB, such studies are also crucial for...
Go to contribution page -
Jutta Schnabel (Friedrich-Alexander Universität Erlangen-Nürnberg), Tamas Gal (ECAP / FAU)07/09/2020 16:40
-
Jose Enrique Ruiz08/09/2020 09:30
-
Jean Aboudarham (LESIA/PADC - Observatoire de Paris/PSL)08/09/2020 09:50
-
Veronique Delouille (STCE/Royal Observatory of Belgium)08/09/2020 10:10
The SPoCA-suite provide two modules, one for Active Region (AR) detection, and one for Coronal Holes(CH) detection, to the SDO Event Detection System (EDS). It runs in near-real times at Lockheed Martin Solar and Astrophysics Laboratory. Every four hours, the EDS generates and uploads the SPoCA entries into the AR and CH Catalogs of the HEK or Heliophysics Events Knowledgebase.
The VOEvent...
Go to contribution page -
Alan Loh, M. Baptiste Cecconi (Observatoire de Paris)08/09/2020 10:30
-
Mattia Mancini, M. Yan Grange (ASTRON, the Netherlands Institute for Radio Astronomy)08/09/2020 11:10
-
Des Small (JIVE), Harro Verkouter (Joint Institute for VLBI ERIC), Mark Kettenis (JIVE)08/09/2020 11:30
In this use-case presentation the EVN Archive and its provenance challenges will be presented.
The EVN is a proposal-driven open-access instrument for VLBI astronomy. There is considerable interest -- not least from funding agencies -- about the conversion of the data taken into papers published in the scientific literature (which in our case can be restricted to those registered in the...
Go to contribution page -
Alessandra Zanichelli08/09/2020 11:50
Choisissez le fuseau horaire
Le fuseau horaire de votre profil: