tipa -- 3/31/2015

Dust production 680-850 million years after the Big Bang

• Michał J. Michałowski (IfA, Edinburgh)

The first gamma-ray detection of the narrow-line Seyfert 1 FBQS J1644+2619

• F. D'Ammando (DIFA - University of Bologna, INAF-IRA Bologna), M. Orienti (INAF-IRA Bologna), J. Larsson (KTH, Dep. of Physics, and the Oskar Klein Centre), M. Giroletti (INAF-IRA Bologna)

Cosmic Reionization after Planck: The Derived Growth of the Ionizing Background now matches the Growth of the Galaxy UV Luminosity Density

• R. J. Bouwens, G. D. Illingworth, P. A. Oesch, J. Caruana, B. Holwerda, R. Smit, S. Wilkins

A Hero's Dark Horse: Discovery of an Ultra-Faint Milky Way Satellite in Pegasus

• Dongwon Kim, Helmut Jerjen, Dougal Mackey, Gary S. Da Costa, Antonino P. Milone

X-ray flares from dense shells formed in gamma-ray burst explosions

• R. Hascoet (1), A. M. Beloborodov (1), F. Daigne (2), R. Mochkovitch (2) ((1) Columbia University, (2) UPMC-CNRS, Institut d'Astrophysique de Paris)

Radio flares from gamma-ray bursts

• D. Kopac, C.G. Mundell, S. Kobayashi, F.J. Virgili, R. Harrison, J. Japelj, C. Guidorzi, A. Melandri, A. Gomboc

The Milky Way system in LCDM cosmological simulations

• Qi Guo, Andrew Cooper, Carlos Frenk, John Helly, Wojciech Hellwing

Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA

• S. Dye, C. Furlanetto, A. M. Swinbank, C. Vlahakis, J. W. Nightingale, L. Dunne, S. A. Eales, Ian Smail, I. Oteo-Gomez, T. Hunter, M. Negrello, H. Dannerbauer, R. J. Ivison, R. Gavazzi, A. Cooray, P. van der Werf

Nature of the Extreme Ultraluminous X-ray Sources

• Grzegorz Wiktorowicz, Malgorzata Sobolewska, Aleksander Sadowski, Krzysztof Belczynski

Reply to Comment on "Evidence for dark matter in the inner Milky Way"

• Fabio Iocco, Miguel Pato, Gianfranco Bertone

Measurement of the Electron Neutrino Charged-current Interaction Rate on Water with the T2K ND280 pi-zero Detector

• T2K Collaboration

Measurement of a false electric dipole moment signal from $^{199}$Hg atoms exposed to an inhomogeneous magnetic field

• S. Afach, C. A. Baker, G. Ban, G. Bison, K. Bodek, Z. Chowdhuri, M. Daum, M. Fertl, B. Franke, P. Geltenbort, K. Green, M. G. D. van der Grinten, Z. Grujic, P. G. Harris, W. Heil, V. Hélaine, R. Henneck, M. Horras, P. Iaydjiev, S. N. Ivanov, M. Kasprzak, Y. Kermaïdic, K. Kirch, P. Knowles, H.-C. Koch, S. Komposch, A. Kozela, J. Krempel, B. Lauss, T. Lefort, Y. Lemière, A. Mtchedlishvili, O. Naviliat-Cuncic, J. M. Pendlebury, F. M. Piegsa, G. Pignol, P. N. Prashant, G. Quéméner, D. Rebreyend, D. Ries, S. Roccia, P. Schmidt-Wellenburg, N. Severijns, A. Weis, E. Wursten, G. Wyszynski, J. Zejma, J. Zenner, G. Zsigmond