output
20032026
Showing 2013 · astro-ph.IMShow all

7 papers · 2 filters

astro-ph.IM2013★ 69 cited

First Searches for Optical Counterparts to Gravitational-wave Candidate Events

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +904

During the LIGO and Virgo joint science runs in 2009-2010, gravitational wave (GW) data from three interferometer detectors were analyzed within minutes to select GW candidate even…

astro-ph.IM2013★ 39 cited

The camera of the fifth H.E.S.S. telescope. Part I: System description

J. Bolmont, P. Corona, P. Gauron +54

In July 2012, as the four ground-based gamma-ray telescopes of the H.E.S.S. (High Energy Stereoscopic System) array reached their tenth year of operation in Khomas Highlands, Namib…

astro-ph.IM2013★ 3 cited

The NectarCAM camera project

J-F. Glicenstein, M. Barcelo, J-A. Barrio +57

In the framework of the next generation of Cherenkov telescopes, the Cherenkov Telescope Array (CTA), NectarCAM is a camera designed for the medium size telescopes covering the cen…

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…