ALMA Band 3 polarimetric follow-up of a complete sample of faint PACO sources

We present Atacama Large Millimeter/submillimiter Array (ALMA) high sensitivity (\(\sigma_P \simeq 0.4\,\)mJy) polarimetric observations at \(97.5\,\)GHz (Band 3) of a complete sample of \(32\) extragalactic radio sources drawn from the faint Planck-ATCA Co-eval Observations (PACO) sample (\(b

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Bibliographic Details
Published in:arXiv.org 2019-06
Main Authors: Galluzzi, Vincenzo, Puglisi, Giuseppe, Burkutean, Sandra, Liuzzo, Elisabetta, Bonato, Matteo, Massardi, Marcella, Paladino, Rosita, Gregorini, Loretta, Ricci, Roberto, Trombetti, Tiziana, Toffolatti, Luigi, Burigana, Carlo, Bonaldi, Anna, Bonavera, Laura, Casasola, Viviana, De Zotti, Gianfranco, Ekers, Ronald David, Sperello di Serego Alighieri, López-Caniego, Marcos, Tucci, Marco
Format: Article
Language:English
Subjects:
Arrays
Cosmic dust
Extragalactic radio sources
Frequency ranges
Galaxies
Polarimetry
Polarization
Radio telescopes
Sky surveys (astronomy)
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Summary:We present Atacama Large Millimeter/submillimiter Array (ALMA) high sensitivity (\(\sigma_P \simeq 0.4\,\)mJy) polarimetric observations at \(97.5\,\)GHz (Band 3) of a complete sample of \(32\) extragalactic radio sources drawn from the faint Planck-ATCA Co-eval Observations (PACO) sample (\(b
ISSN:2331-8422
DOI:10.48550/arxiv.1907.00299