activity
19942003
most citedAdvanced pseudo-correlation radiometers for the Planck-LFI instrument

8 citations · 10 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph2003

The CMB Power Spectrum from the Background Emission Anisotropy Scanning Telescope (BEAST) Experiment

Ian J. O'Dwyer, Marco Bersanelli, Jeffrey Childers +19

The Background Emission Anisotropy Scanning Telescope (BEAST) is a 2.2m off-axis telescope with an 8 element mixed Q (38-45GHz) and Ka (26-36GHz) band focal plane, designed for bal…

astro-ph20038 cited

Advanced pseudo-correlation radiometers for the Planck-LFI instrument

A. Mennella, M. Bersanelli, R. C. Butler +34

The LFI (Low Frequency Instrument) on board the ESA Planck satellite is constituted by an array of radiometric detectors actively cooled at 20 K in the 30-70 GHz frequency range in…

astro-ph20032 cited

A Map of the Cosmic Microwave Background from the BEAST Experiment

Peter R. Meinhold, Marco Bersanelli, Jeffrey Childers +24

We present the first sky maps from the BEAST (Background Emission Anisotropy Scanning Telescope) experiment. BEAST consists of a 2.2 meter off axis Gregorian telescope fed by a cry…

astro-ph1999

Cosmic Microwave Background Observations in the Post-Planck Era

J. B. Peterson, J. E. Carlstrom, E. S. Cheng +5

The Microwave Anisotropy Probe and Planck missions will provide low noise maps of the temperature of the cosmic microwave background (CMB). These maps will allow measurement of the…

astro-ph1997

Cosmic microwave background maps from the HACME experiment

Max Tegmark, Angelica de Oliveira-Costa, John Staren +9

We present Cosmic Microwave Background (CMB) maps from the Santa Barbara HACME balloon experiment (Staren etal 2000), covering about 1150 square degrees split between two regions i…

astro-ph1994

Degree Scale Anisotropy: SP94 Results

J. Gundersen, M. Lim, J. Staren +8

We present results from 2 observations of the CMB performed from the South Pole during the 93-94 austral summer. Each observation employed a 3 peak to peak sinusoidal, si…