output
20022013
most citedSpectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

1.4k citations

Showing 2008Show all

31 papers · 1 filter

astro-ph200841 cited

Heating in an Extended Accretion Disk Corona along the Z-Pattern in Cyg X-2

N. S. Schulz, D. P. Huenemoerder, L. Ji +3

We observed at very high spectral resolution the prototype Z-source Cyg x-2 twice along its entire X-ray spectral variation pattern. In this preliminary analysis we find an extende…

astro-ph200817 cited

Photometric properties of resolved and unresolved magnetic elements

Serena Criscuoli, Mark Rast

We investigate the photometric signature of magnetic flux tubes in the solar photosphere. We developed two dimensional, static numerical models of isolated and clustered magnetic f…

astro-ph2008414 cited

Science with ASKAP - the Australian Square Kilometre Array Pathfinder

S. Johnston, R. Taylor, M. Bailes +47

[ABRIDGED VERSION] The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be…

astro-ph200837 cited

New Observations and a Possible Detection of Parameter Variations in the Transits of Gliese 436b

Jeffrey L. Coughlin, Guy S. Stringfellow, Andrew C. Becker +3

We present ground-based observations of the transiting Neptune-mass planet Gl 436b obtained with the 3.5-meter telescope at Apache Point Observatory and other supporting telescopes…

astro-ph200849 cited

Cluster Abell 520: a perspective based on member galaxies. A cluster forming at the crossing of three filaments?

M. Girardi, R. Barrena, W. Boschin +1

The connection of cluster mergers with the presence of extended, diffuse radio sources in galaxy clusters is still debated. An interesting case is the rich, merging cluster Abell 5…

astro-ph200829 cited

A dynamical perspective on additional planets in 55 Cancri

Sean N. Raymond, Rory Barnes, Noel Gorelick

Five planets are known to orbit the star 55 Cancri. The recently-discovered planet f at 0.78 AU (Fischer et al. 2008) is located at the inner edge of a previously-identified stable…