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ALMACAL IV: a catalogue of ALMA calibrator continuum observations

Bonato, M.; Liuzzo, E.; Giannetti, A.; Massardi, M.; De Zotti, G.; Burkutean, S.; Galluzzi, V.; Negrello, M.; Baronchelli, I.; Brand, J.; Zwaan, MA.; Rygl, K.L.J.; Marchili, N.; Klitsch, A.; Oteo, I.

ALMACAL IV: a catalogue of ALMA calibrator continuum observations Thumbnail


Authors

M. Bonato

E. Liuzzo

A. Giannetti

M. Massardi

G. De Zotti

S. Burkutean

V. Galluzzi

M. Negrello

I. Baronchelli

J. Brand

MA. Zwaan

K.L.J. Rygl

N. Marchili

A. Klitsch

I. Oteo



Abstract

We present a catalogue of ALMA flux density measurements of 754 calibrators observed between 2012 August and 2017 September, for a total of 16263 observations in different bands and epochs. The flux densities were measured by reprocessing the ALMA images generated in the framework of the ALMACAL project, with a new code developed by the Italian node of the European ALMA Regional Centre. A search in the online data bases yielded redshift measurements for 589 sources (∼78 per cent of the total). Almost all sources are flat spectrum, based on their low-frequency spectral index, and have properties consistent with being blazars of different types. To illustrate the properties of the sample, we show the redshift and flux density distributions as well as the distributions of the number of observations of individual sources and of timespans in the source frame for sources observed in bands 3 (84−116 GHz) and 6 (211−275 GHz). As examples of the scientific investigations allowed by the catalogue, we briefly discuss the variability properties of our sources in ALMA bands 3 and 6 and the frequency spectra between the effective frequencies of these bands. We find that the median variability index steadily increases with the source-frame time lag increasing from 100 to 800  d, and that the frequency spectra of BL Lacs are significantly flatter than those of flat-spectrum radio quasars. We also show the global spectral energy distributions of our sources over 17 orders of magnitude in frequency.

Journal Article Type Article
Acceptance Date Apr 20, 2018
Online Publication Date May 5, 2018
Publication Date Aug 1, 2018
Deposit Date Jul 5, 2018
Publicly Available Date Jul 5, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 478
Issue 2
Pages 1512-1519
DOI https://doi.org/10.1093/mnras/sty1173
Public URL https://durham-repository.worktribe.com/output/1327008

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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





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