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Journal club Astro-particules
A quoi ça sert ? L'idée du journal club est de se tenir au courant de l'actualité scientifique par le biais de discussions autour d'articles vus sur http://arxiv.org/. Il s'agit donc d'encourager la prise de parole dans une atmosphère conviviale, d'échanger, de partager nos expertises, nos questions... afin de faire vivre encore plus la vie scientifique au labo !
Mode opératoire :
- Quand ? Tous les vendredis à 11h00
- Comment ? A n'importe quel moment, ajoutez simplement un lien vers le papier que vous souhaitez présenter/discuter (voir ci-dessous, il suffit d'éditer ce wiki).
- Et ensuite ? Une séance dure au plus 1h. Chaque papier pourra être présenté/discuté pendant 10-15 mn (en fonction du nombre). L'idée est de faire ressortir les idées principales du papier, montrer les courbes les plus importantes et nous dire pourquoi ce papier vous a interpelé (libre à chacun d'être plus ambitieux). Il peut s'agir d'un résultat expérimental/observationnel, d'une simulation, de phéno/théorie, de méthodes/outils...
- Modalité d'inscription Le Journal Club est ouvert à tous, mais notez bien qu'il s'agira de discuter de sujets reliés aux astro-particules (sauf événement scientifique exceptionnel). Pour les prises de parole/questions, la priorité sera donnée aux doctorants. Bref, venez nombreux !
Contact : David Maurin (bureau 341, extension 40 82), Juan Macias-Perez (bureau 331, extension 41 52), Fred Mayet (bureau 319, extension 41 82)
Trac : TracWiki (documentation Trac), WikiFormatting (règles de formatage)
Vendredi 21/10/2011 (?) - 11h - Salle XXX
- http://arxiv.org/abs/ | Titre | Orateur [pour modifier la page, copier/coller le modèle ci-dessous avec votre ref.]
- http://arxiv.org/abs/1109.4897 | Superluminic neutrinos @ OPERA ? | David Maurin
- http://arxiv.org/abs/1107.1916 | Where will supersymmetric dark matter first be seen in gamma-rays? | David Maurin
Précédentes éditions
Vendredi 14/10/2011
- Sans doute rien
- Toujours rien
Vendredi 07/10/2011
- Rien
- Rien
Attachments (55)
- 2011-11_JClubSupplement.pdf (1.4 MB ) - added by 13 years ago.
- toto (5 bytes ) - added by 13 years ago.
- Mayet-dama-muons.pdf (494.3 KB ) - added by 13 years ago.
- 2011-11_JClubSupplementSolMod.pdf (731.4 KB ) - added by 13 years ago.
- marrocchesi2011.pdf (853.6 KB ) - added by 13 years ago.
- ArXiv1112.3590v1.pdf (1.6 MB ) - added by 13 years ago.
- JC_ACT.pdf (2.1 MB ) - added by 13 years ago.
- jc_fermi.pdf (425.8 KB ) - added by 13 years ago.
- Aq-D-2jpg (637.0 KB ) - added by 13 years ago.
- Aq-D-2.jpg (637.0 KB ) - added by 13 years ago.
- millenium.jpg (617.0 KB ) - added by 13 years ago.
- 2012-01_JC_BBNaxionsCosmo.pdf (222.3 KB ) - added by 13 years ago.
- 2012-04_JClubBorexino.pdf (1.2 MB ) - added by 13 years ago.
-
CRDrift.png
(32.9 KB
) - added by 12 years ago.
Drift streamlines for positively charged cosmic rays. The directions correspond to the 1975 sunspot minimum (when the polar solar magnetic field was directed outward from the Sun) and would be reversed in alternate minima. The heavy wavy line is the interplanetary current sheet, along which particles drift extremely rapidly. Similarly, the arrows would be reversed for negatively charged particles.
- 2012-06_JClubPioneer.pdf (935.6 KB ) - added by 12 years ago.
- journal_club_9_nov_2012.pdf (260.4 KB ) - added by 12 years ago.
- nature11734.pdf (3.0 MB ) - added by 12 years ago.
- nature11734-s1.pdf (1.1 MB ) - added by 12 years ago.
- 1005.5480.pdf (1.5 MB ) - added by 12 years ago.
- LIS_Herbst+12.pdf (3.7 MB ) - added by 12 years ago.
- JClub-260413-Fig2-Fig4.pdf (418.6 KB ) - added by 12 years ago.
- JClub-260413-Fig21.pdf (405.7 KB ) - added by 12 years ago.
- JClub-260413-Fig2-Fig4.2.pdf (418.6 KB ) - added by 12 years ago.
- JClub-260413-figA4b.pdf (127.9 KB ) - added by 12 years ago.
- PlosOne.8.0054847.2013.pdf (882.0 KB ) - added by 12 years ago.
- phys.rev.D.84.103501-Nelson.pdf (241.2 KB ) - added by 12 years ago.
- Fermi_13.pdf (812.9 KB ) - added by 11 years ago.
- gaps_flight_a.pdf (2.1 MB ) - added by 11 years ago.
- gaps_flight_b.pdf (2.9 MB ) - added by 11 years ago.
- 2014-02_JClubGAPS.pdf (1.6 MB ) - added by 11 years ago.
- Note_MaBert.pdf (179.2 KB ) - added by 10 years ago.
- 1403.1612v2.pdf (1.2 MB ) - added by 10 years ago.
- fig30.png (80.7 KB ) - added by 10 years ago.
- nature14616.pdf (6.9 MB ) - added by 9 years ago.
- naturev0.pdf (962.2 KB ) - added by 9 years ago.
- 2015-11_JClub-3.5keVLine.pdf (2.7 MB ) - added by 9 years ago.
- stream.jpg (147.1 KB ) - added by 9 years ago.
- hotgas.jpg (258.5 KB ) - added by 9 years ago.
- 2016-03_JClubPopIII.pdf (3.9 MB ) - added by 9 years ago.
- 2016-03_PlanetNine.pdf (1.4 MB ) - added by 9 years ago.
- 2016-05_JClubPDFDM.pdf (1.7 MB ) - added by 9 years ago.
- Slides_Journal_Club_Covariance_SZ_lensing.pdf (5.8 MB ) - added by 9 years ago.
- jclub_sidm.pdf (668.5 KB ) - added by 8 years ago.
- Mangeard2016JGRA..121.7435M.pdf (963.3 KB ) - added by 8 years ago.
- 2016-11_JclubNM.pdf (6.0 MB ) - added by 8 years ago.
- Slides_Journal_Club_CLASH.pdf (10.4 MB ) - added by 8 years ago.
- jclub_20170120.pdf (645.1 KB ) - added by 8 years ago.
- 2017-01_JClubErrorMatrix.pdf (1.1 MB ) - added by 8 years ago.
- 2017-03_DarkClumps.pdf (11.2 MB ) - added by 8 years ago.
- R_process.pdf (1.6 MB ) - added by 8 years ago.
- myJC_02.pdf (1.2 MB ) - added by 7 years ago.
- 2017-10_JClubGW170817.pdf (1.3 MB ) - added by 7 years ago.
-
2017-12_Florian_JClub_Missing_Baryons.pdf
(11.7 MB
) - added by 7 years ago.
Slide_Florian
- DD_ID_CMB.pdf (11.7 MB ) - added by 7 years ago.
- Genolini.pdf (6.1 MB ) - added by 7 years ago.