Science Feed Posts - TopicsExpress

C-Band All-Sky Survey: A First Look at the Galaxy.
C-Band All-Sky Survey: A First Look at the Galaxy. (arXiv:1501.06069v1 [astro-ph.GA]) M.O. Irfan, C. Dickinson, R.D. Davies, C. Copley, R.J. Davis, P....

The Third Catalog of Active Galactic Nuclei Detected by the Fermi
The Third Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope. (arXiv:1501.06054v1 [astro-ph.HE]) M. Ackermann, M. Ajello, W....

The Bolocam Galactic Plane Survey. XI. Temperatures and
The Bolocam Galactic Plane Survey. XI. Temperatures and Substructure of Galactic Clumps Based on 350 micron Observations. (arXiv:1501.05965v1 [astro-p...

Hadronic models of blazars require a change of the accretion
Hadronic models of blazars require a change of the accretion paradigm. (arXiv:1501.06124v1 [astro-ph.HE]) Andrzej A. Zdziarski, Markus Boettcher We s...

A Continuum of Planet Formation Between 1 and 4 Earth Radii.
A Continuum of Planet Formation Between 1 and 4 Earth Radii. (arXiv:1501.05953v1 [astro-ph.EP]) Kevin C. Schlaufman It has long been known that stars...

Design of the Front End Electronics for the Infrared Camera of
Design of the Front End Electronics for the Infrared Camera of JEM-EUSO, and manufacturing and verification of the prototype model. (arXiv:1501.06183v...

ALMA Multi-line Imaging of the Nearby Starburst Galaxy NGC 253.
ALMA Multi-line Imaging of the Nearby Starburst Galaxy NGC 253. (arXiv:1501.05694v1 [astro-ph.GA]) David S. Meier (1,2,3), Fabian Walter (4,2), Albert...

A spin-down clock for cool stars from observations of a
A spin-down clock for cool stars from observations of a 2.5-billion-year-old cluster. (arXiv:1501.05651v1 [astro-ph.SR]) Soren Meibom, Sydney A. Barne...

Optical technologies for the observation of low Earth orbit
Optical technologies for the observation of low Earth orbit objects. (arXiv:1501.05736v1 [astro-ph.IM]) Daniel Hampf, Paul Wagner, Wolfgang Riede In ...

Formation of Super-Earth Mass Planets at 125-250 AU from a
Formation of Super-Earth Mass Planets at 125-250 AU from a Solar-type Star. (arXiv:1501.05659v1 [astro-ph.EP]) S. J. Kenyon, B. C. Bromley We investi...