activity
19982003
most citedObservations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes

2 citations · 4 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph2003

Maps of the millimetre sky from the BOOMERanG experiment

P. de Bernardis, P. A. R. Ade, A. Balbi +38

In the 1998-99 flight, BOOMERanG has produced maps of of the sky at high Galactic latitudes, at frequencies of 90, 150, 240 and 410 GHz, with resolution $\simgt 10'$. Th…

astro-ph20032 cited

The MAXIMA Experiment: Latest Results and Consistency Tests

R. Stompor, S. Hanany, M. E. Abroe +10

The MAXIMA cosmic microwave background anisotropy experiment had a significant impact on cosmology. Results from the program have played a significant role in determining the geome…

astro-ph20032 cited

Observations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes

K. Coble, P. A. R. Ade, J. J. Bock +32

We present millimeter-wave observations of three extra-galactic and six Galactic sources in the Southern sky. Observations were made at 90, 150, 240 and 400 GHz with resolutions of…

astro-ph2001

Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data

S. Prunet, P. A. R. Ade, J. J. Bock +35

We describe here an iterative method for jointly estimating the noise power spectrum from a CMB experiment's time-ordered data, together with the maximum-likelihood map. We test th…

astro-ph2000

From the time-ordered data to the Maximum-Likelihood temperature maps of the Cosmic Microwave Backgorund anisotropy

R. Stompor, A. Balbi, J. Borrill +10

We review selected methods of the Cosmic Microwave Background data analysis appropriate for the analysis of the largest currently available data sets. We focus on techniques of the…

astro-ph2000

Detection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment

P. de Bernardis, P. A. R. Ade, J. J. Bock +35

BOOMERanG has recently resolved structures on the last scattering surface at redshift 1100 with high signal to noise ratio. We review the technical advances which made this…