Journal club Astro-particules

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Prochaine séance : vendredi 26/4/2013 - 11h - N.B.: Salle de cours à côté de la salle 9 !

• ​http://arxiv.org/abs/1304.4279 | Dark Matter Search Results Using the Silicon Detectors of CDMS II | Jabob Lamblin
• ​http://arxiv.org/abs/1303.5062 | Planck 2013 results. I. Overview of products and scientific results + comments on Fig.A.4(b)​, Fig.2 and Fig.21 of the ​Cosmological parameters paper | Laurence & Celine

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FAQ (about the Journal-Club)

• its goal is to allow us to discuss recent papers, taking advantage of the many topics and expertises developed in the lab.
• it's an opportunity for students to 'give' talks and ask questions.
• feel free to attend and contribute in English (but be aware that French is the default language)
• it is open to everybody and any subject, though the focus is on astroparticle physics

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/ (ou ​http://slac.stanford.edu/spires/ si vous préférez). 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 (la date du Journal Club à venir apparaît toujours en bleu/gras ci-dessous)
• Comment ? Dès que la date de la séance suivante est affichée, éditez ce Wiki et ajoutez un lien vers le papier désiré (suivre les instructions ici si vous ne pouvez pas éditer ce Wiki) :
  1. Cliquez sur connexion (haut à droite)
  2. Cliquez sur Modifier la page (bas à gauche) pour éditer ce Wiki et ajouter votre lien
  3. Cliquez sur Enregistrer les modifications (bas au milieu)... c'est fini !
• 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, nous choisirons délibérément de donner la priorité aux doctorants. Venez nombreux !

Contact : David Maurin (bureau 341, tél 40 82), Juan Macias-Perez (bureau 331B, tél 41 52)

Trac : TracWiki (documentation Trac), WikiFormatting (règles de formatage)

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Précédentes éditions

Année 2012-2013

Vendredi 15/02/2013

• ​http://arxiv.org/abs/1212.5018 | A novel approach in the WIMP quest: Cross-Correlation of Gamma-Ray Anisotropies and Cosmic Shear | Marco Regis
• Herbst et al., ApJ 76, 761 (2012)​| The Local Interstellar Spectrum beyond the Heliopause: What can be Learned from Voyager in the Inner Heliosheath? | David Maurin

Vendredi 25/01/2013

• ​http://arxiv.org/abs/1301.0512 | Giant Magnetized Outflows from the Centre of the Milky Way (*)​ (**)​ (***)​| Marco Regis
• ​http://arxiv.org/abs/1301.3820 | Determination of the Cosmic Antideuteron Flux in a Monte Carlo approach | David Maurin

Vendredi 11/01/2013

• ​http://arxiv.org/abs/1207.5645 | Observing the dynamics of super-massive black hole binaries with Pulsar Timing Arrays | Rémi Adam
• ​http://arxiv.org/abs/1301.0446 | A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy (see also ​0907.3831 and ​1204.5176 for a complementary view on tidal dwarf galaxies)| David Maurin

Vendredi 14/12/2012

• ​http://arxiv.org/abs/1211.1787 | Nuclear proton and neutron distributions in the detection of weak interacting massive particles | Quentin Riffard
• ​http://arxiv.org/abs/1211.6905 | Low energy cosmic ray positron fraction explained by charge-sign dependent solar modulation | Laurent Derome

Vendredi 9/11/2012

• ​http://arxiv.org/abs/1109.6322 | Searching for dark matter in the CMB: A compact parametrization of energy injection from new physics (*)​| Lilian Sanselme
• ​http://arxiv.org/abs/1211.0536 | Dwarf galaxies and the cosmic web | Céline Combet

Vendredi 26/10/2012

• ​http://arxiv.org/abs/1210.6031 | A measurement of the intrahalo light fraction with near- infrared background anisotropies | Juan Macias-Perez
• ​PRL 109, 071101 (2012) | Local Magnetic Turbulence and TeV–PeV Cosmic Ray Anisotropies | David Maurin

Année 2011-2012

Vendredi 15/6/2012

• ​http://arxiv.org/abs/1204.6305 | Closing the Loop: A Self-Consistent Model of Optical, X-ray, and SZ Scaling Relations for Clusters of Galaxies | Barbara Comis
• ​PRL (2007) + ​(2012) | Experimental Observation of Spatially Localized Dynamo Magnetic Fields + reversal ​(*)| David Maurin

Vendredi 8/6/2012

• ​1103.5222 + ​1107.2886 + ​1204.2507 | Support for the thermal origin of the Pioneer anomaly (*)​| David Maurin

Vendredi 1/6/2012

• ​1205.2154 | Polar Field Reversal Observation With Hinode ​Solar Magnetic Field (*)​| William Gillard
• ​1204.2797 + ​1205.2739 | A Tentative Gamma-Ray Line + Search for DM in Gamma-ray Lines and the Inclusive Photon Spectrum from DM Annihilation at the Fermi-LAT | David Maurin

Vendredi 27/4/2012

• ​http://arxiv.org/abs/1204.5122 | Entropy of Non-Extremal Black Holes from Loop Gravity | Francesca Vidotto
• ​http://arxiv.org/abs/1204.3622 | Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation | Quentin Le Boulc'h

Vendredi 13/4/2012

• ​http://arxiv.org/abs/1203.0570 | A common solution to the cosmic ray anisotropy and gradient problems| Laurent Derome
• ​1110.3230 + ​1202.6403 | First evidence of pep solar neutrinos by direct detection in Borexino + Cosmic-muon flux and annual modulation in Borexino at 3800 m water-equivalent depth (suppl.)​| David Maurin

Vendredi 30/3/2012

• ​http://arxiv.org/abs/1105.3207 | The Contribution of Supernovae to Cosmic Reionization | Lilian Sanselme
• ​http://arxiv.org/abs/1203.4097 | The Missing Massive Satellites of the Milky Way (Aquarius)​(Millenium)​ | Céline Combet

Vendredi 16/3/2012

• ​http://arxiv.org/abs/1203.2612 | An extremely primitive halo star | David Maurin
• ​http://arxiv.org/abs/1203.3277 | An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data | J.F. Macias-Perez

Vendredi 10/2/2012

• ​http://arxiv.org/abs/1202.0554 | Cuspy No More: How Outflows Affect the Central Dark Matter and Baryon Distribution in Lambda CDM Galaxies | Laurent Derome
• ​http://prl.aps.org/abstract/PRL/v108/i6/e061304 | Axion Dark Matter and Cosmological Parameters (*)​ David Maurin

Vendredi 3/2/2012

• ​http://arxiv.org/abs/1201.5114 | Observations of dark and luminous matter: the radial distribution of satellite galaxies around massive red galaxies Aq-D-2.jpg (*)​millenium.jpg (*)​ | Céline Combet
• ​http://arxiv.org/abs/1112.3264 | A gas cloud on its way towards the super-massive black hole in the Galactic Centre | David Maurin

Vendredi 27/1/2012

• ​http://arxiv.org/abs/1105.0419 | Evidence for dark energy from the CMB alone using the Atacama Cosmology Telescope lensing measurements (*)​ | Laurence Perotto
• ​http://arxiv.org/abs/1201.4491 | Magnetic substructure in the northern Fermi Bubble revealed by polarized WMAP emission (*)​| Celine Combet

Vendredi 13/1/2012

• ​http://arxiv.org/abs/1103.2124 | Detection of the Power Spectrum of CMB Lensing by the Atacama Cosmology Telescope (*)​ | Laurence Perotto
• ​http://arxiv.org/abs/1109.5871 | Cosmic ray transport in galaxy clusters: implications for radio halos and gamma-rays | David Maurin
• ​http://arXiv.org/abs/1108.3003 | Stable Lorentzian Wormholes in Dilatonic Einstein-Gauss-Bonnet Theory | Aurélien Barrau

Vendredi 16/12/2011

• ​http://arxiv.org/abs/1111.6386v1 | CMB constraints on duration and timing from SPT | Lilian Sanselme
• ​http://arxiv.org/abs/1112.3020 | Nearby supernova remnants and the cosmic-ray spectral hardening at high energies | Benoît Coste
• ​http://arxiv.org/pdf/1112.3590v1(*)​ | Sudden intensity increase and radial gradiant changes of cosmic ray MeV electrons and protons observed at voyager 1 beyond 111 AU in the heliosheath | William Gillard

Vendredi 09/12/2011

• ​http://arxiv.org/abs/1110.1529 | Probing DM Decay and Annihil. with Fermi Observ. of Nearby Galaxy Clusters ((+ ​1001.0644 for spectral features from Decay in X-rays) | David Maurin

Vendredi 25/11/2011

• ​http://arxiv.org/abs/1111.1004 | Constraints on Modified Gravity from Sunyaev-Zeldovich Cluster Surveys | Guillaume Hurier
• ​http://arxiv.org/abs/1111.5127 | Fermi Bubble as a Source of Cosmic Rays in the Energy Range > 10E15 eV | Mathieu Tartare et/ou Guilhem Bernard
• ​2011APh....35...21M (*)​ | An high resolution FDIRC for the measurement of cosmic-ray isotopic abundances | William Gillard
• ​1111.0075 and ​1111.3983| How will astronomy archives survive the data tsunami? (some tools ​here and ​there) + The ADS All-Sky Survey | David Maurin

Vendredi 18/11/2011

• ​http://cdsads.u-strasbg.fr/abs/2011ApJ...735..128S | On Cosmic Ray Modulation beyond the Heliopause: Where is the Modulation Boundary? (suppl.)​| David Maurin
• ​http://arxiv.org/abs/1111.3075 | Anisotropy of TeV Cosmic Rays and the Outer Heliospheric Boundaries | Céline Combet
• ​http://arxiv.org/abs/1110.0857 | DAMA vs. the annually modulated muon background (*)​ | Frédéric Mayet

Vendredi 4/11/2011

• ​http://arxiv.org/abs/1109.4897 | Superluminic neutrinos @ OPERA ? | Laurent Derome
• ​http://arxiv.org/abs/1107.1916 | Where will SUSY dark matter first be seen in gamma-rays? (suppl.)​ | David Maurin
• ​http://arxiv.org/abs/1103.0303 | Likelihood Approach to the First Dark Matter Results from XENON100 | Julien Billard
• ​http://arxiv.org/abs/1109.0521 | Measurement of separate cosmic-ray electron and positron spectra with the Fermi Large Area Telescope | William Gillard