The Daily Brew
Selected astro-ph abstracts for Tuesday March 15
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The Stellar Mass Evolution of Galaxies in the NICMOS Ultra Deep Field
S. D. J. Gwyn and F. D. A. Hartwick
astro-ph/0503275
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Metric Tests for Curvature from Weak Lensing and Baryon Acoustic
Oscillations
G. Bernstein (University of Pennsylvania)
astro-ph/0503276
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TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR
1806-20
Kunihito Ioka, Soebur Razzaque, Shiho Kobayashi, Peter Meszaros
astro-ph/0503279
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A Variable Infrared Counterpart to the Soft Gamma-ray Repeater SGR
1806-20
George Kosugi, Ryusuke Ogasawara, Hiroshi Terada
astro-ph/0503280
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Detecting Intracluster Gas Motion in Galaxy Clusters: Mock Astro-E2
Observations
Andrew Pawl, August E. Evrard, Renato A. Dupke
astro-ph/0503281
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Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with
Weak Gravitational Lensing
David E. Johnston
astro-ph/0503282
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High-redshift quasar host galaxies with adaptive optics
B. Kuhlbrodt (1 and 2), E. Orndahl (3 and 4), L. Wisotzki (1 and 5)
and K. Jahnke (1 and 2) ((1) Astrophysikalisches Institut Potsdam, (2)
Hamburger Sternwarte, (3) Tuorla Observatory, (4)Department of Astronomy and
Space Physics, Uppsala University, (5) Institut fuer Physik, Potsdam
University)
astro-ph/0503284
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The Connection between Ultraviolet and X-ray Outflows in AGN: the case
of PDS 456
Paul T. O'Brien (University of Leicester), James N. Reeves
(JHU/NASA-GSFC), Chris Simpson (University of Durham), Martin J. Ward
(University of Durham)
astro-ph/0503293
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Mass estimates from stellar proper Motions: The mass of $\omega$
Centauri
Richard D'Souza, Hans-Walter Rix
astro-ph/0503299
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X-ray Lighthouses of the High-Redshift Universe. II. Further Snapshot
Observations of the Most Luminous z>4 Quasars with Chandra
C. Vignali (Dipartimento di Astronomia, Universita` di Bologna;
INAF-Osservatorio Astronomico di Bologna, Italy), W.N.Brandt, D.P. Schneider
(Department of Astronomy and Astrophysics, The Pennsylvania State University,
USA), S. Kaspi (School of Physics and Astronomy, Raymond and Beverly Sackler
Faculty of Exact Sciences, Tel-Aviv University; Physics Department, Technion,
Haifa, Israel)
astro-ph/0503301
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