output
19932026
most citedThe Gaia mission

7.1k citations

Showing 2013 · astro-ph.IMShow all

7 papers · 2 filters

astro-ph.IM2013★ 221 cited

The First Fermi-LAT Catalog of Sources Above 10 GeV

LAT Collaboration

We present a catalog of gamma-ray sources at energies above 10 GeV based on data from the Large Area Telescope (LAT) accumulated during the first three years of the Fermi Gamma-ray…

astro-ph.IM2013★ 276 cited

RadioAstron -- a Telescope with a Size of 300 000 km: Main Parameters and First Observational Results

N. S. Kardashev, V. V. Khartov, RadioAstron collaboration

The Russian Academy of Sciences and Federal Space Agency, together with the participation of many international organizations, worked toward the launch of the RadioAstron orbiting…

astro-ph.IM2013★ 188 cited

Planck 2013 results. IX. HFI spectral response

Planck Collaboration, P. A. R. Ade, N. Aghanim +217

The Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground based tests conducted with the HFI focal plane in a cryogenic environment pri…

astro-ph.IM2013★ 111 cited

Planck 2013 results. VII. HFI time response and beams

Planck Collaboration, P. A. R. Ade, N. Aghanim +220

This paper characterizes the effective beams,the effective beam window functions and the associated errors for the Planck HFI detectors. The effective beam is the angular response…

astro-ph.IM2013★ 78 cited

Planck 2013 results. V. LFI calibration

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +217

We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the Orbital D…

astro-ph.IM2013★ 97 cited

Planck 2013 results. II. Low Frequency Instrument data processing

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +229

We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5…

astro-ph.IM2013★ 31 cited

VLBI imaging throughout the primary beam using accurate UV shifting

John S. Morgan, F. Mantovani, A. T. Deller +5

For Very Long Baseline Interferometry (VLBI), the fringe spacing is extremely narrow compared to the field of view imposed by the primary beam of each element. This means that an e…