The Daily Brew
Selected astro-ph abstracts for Friday June 18
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How accurately can suborbital experiments measure the CMB?
Angelica de Oliveira-Costa, Max Tegmark, Mark Devlin, Lyman Page,
Amber Miller, Barth Netterfield, Yongzhong Xu
astro-ph/0406375
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Galaxy-Galaxy Flexion: Weak Lensing to Second Order
David M. Goldberg (Drexel University), David J. Bacon (IfA, Edinburgh)
astro-ph/0406376
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Far Ultraviolet Observations of Molecular Hydrogen in the Diffuse
Interstellar Medium of Starburst Galaxies
C. G. Hoopes (1), K. R. Sembach (2), T. M. Heckman (1), G. R. Meurer
(1), A. Aloisi (2), D. Calzetti (2), C. Leitherer (2), and C. L. Martin (3)
((1) JHU, (2) STScI, (3)UCSB)
astro-ph/0406378
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Spatial Distribution of Warm Dust in Early-Type Galaxies
M. A. Pahre, M. L. N. Ashby, G. G. Fazio, and S. P. Willner (CfA)
astro-ph/0406379
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Phase light curves for extrasolar Jupiters and Saturns
Ulyana A. Dyudina, Penny D. Sackett, Daniel D. R. Bayliss, Sara
Seager, Carolyn C. Porco, Henry B. Throop, and Luke Dones
astro-ph/0406390
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An ISOCAM survey through gravitationally lensing galaxy clusters. II.
The properties of infrared galaxies in the A2218 field
A. Biviano, L. Metcalfe, B. McBreen, B. Altieri, D. Coia, M.F.
Kessler, J-P. Kneib, K. Leech, K. Okumura, S. Ott, R. Perez-Martinez, C.
Sanchez-Fernandez, B. Schulz
astro-ph/0406391
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Velocity trends in the debris of Sagittarius and the shape of the
dark-matter halo of the Galaxy
Amina Helmi (Kapteyn Institute)
astro-ph/0406396
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Improved Baade-Wesselink surface-brightness relations
Martin Groenewegen
astro-ph/0406397
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Molecular Hydrogen and [FeII] in Active Galactic Nuclei
Alberto Rodriguez-Ardila (1), Miriani G. Pastoriza (2), Sueli Viegas
(3), T. A. A. Sigut (4), Anil K. Pradhan (5) ((1) Laboratorio Nacional de
Astrofisica - Brazil, (2) UFRGS - Brazil, (3) Instituto de Astronomia,
Geofisica e Ciencias Atmosfericas-USP - Brazil, (4) Department of Physics and
Astronomy, The University of Western Ontario - Canada, (5) Department of
Astronomy, The Ohio State University - USA.)
astro-ph/0406402
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