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Scientific paper - Original scientific paper
The faint radio sky: VLBA observations of the COSMOS field
Astronomy and Astrophysics, 607 (2017); A132. https://doi.org/10.1051/0004-6361/201731163
Herrera Ruiz, N.; Middelberg, E.; Deller, A.; Norris, R. P.; Best, P. N.; Brisken, W.; Schinnerer, E.; Smolčić, Vernesa; Delvecchio, I.; Momjian, E.; Bomans, D.; Scoville, N. Z.; Carilli, C.

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Herrera Ruiz, N., Middelberg, E., Deller, A., Norris, R. P., Best, P. N., Brisken, W. ... Carilli, C. (2017). The faint radio sky: VLBA observations of the COSMOS field. Astronomy and Astrophysics, 607.. doi: 10.1051/0004-6361/201731163

Herrera Ruiz, N., et al. "The faint radio sky: VLBA observations of the COSMOS field." Astronomy and Astrophysics, vol. 607, 2017. https://doi.org/10.1051/0004-6361/201731163

Herrera Ruiz, N., E. Middelberg, A. Deller, R. P. Norris, P. N. Best, W. Brisken, E. Schinnerer, et al. "The faint radio sky: VLBA observations of the COSMOS field." Astronomy and Astrophysics 607 (2017). https://doi.org/10.1051/0004-6361/201731163

Herrera Ruiz, N., et al. (2017) 'The faint radio sky: VLBA observations of the COSMOS field', Astronomy and Astrophysics, 607. doi: 10.1051/0004-6361/201731163

Herrera Ruiz N, Middelberg E, Deller A, Norris RP, Best PN, Brisken W, and sur.. The faint radio sky: VLBA observations of the COSMOS field. Astronomy and Astrophysics [Internet]. 2017 [cited 2024 November 08];607. doi: 10.1051/0004-6361/201731163

N. Herrera Ruiz, et al., "The faint radio sky: VLBA observations of the COSMOS field", Astronomy and Astrophysics, vol. 607, 2017. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:783968. [Accessed: 08 November 2024]

Metadata
Title (english)The faint radio sky: VLBA observations of the COSMOS field
AuthorN. Herrera Ruiz
AuthorE. Middelberg
AuthorA. Deller
AuthorR. P. Norris
AuthorP. N. Best
AuthorW. Brisken
AuthorE. Schinnerer
AuthorVernesa Smolčić
MBZ: 336180
AuthorI. Delvecchio
AuthorE. Momjian
AuthorD. Bomans
AuthorN. Z. Scoville
AuthorC. Carilli
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract (english)
Context. Quantifying the fraction of active galactic nuclei (AGN) in the faint radio population and understanding their relation with star-forming activity are fundamental to studies of galaxy evolution. Very long baseline interferometry (VLBI) observations are able to identify AGN above relatively low redshifts (z> 0.1) since they provide milli-arcsecond resolution. Aims: We have created an AGN catalogue from 2865 known radio sources observed in the Cosmic Evolution Survey (COSMOS) field, which has exceptional multi- wavelength coverage. With this catalogue we intend to study the faint radio sky with statistically relevant numbers and to analyse the AGN - host galaxy co-evolution, making use of the large amount of ancillary data available in the field.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleAstronomy and Astrophysics
Numberingvol. 607, A132
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201731163
URN:NBNurn:nbn:hr:217:783968
Publication2017
Document URLhttps://www.aanda.org/articles/aa/abs/2017/11/aa31163-17/aa31163-17.html
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2017 ESO. Received: 12 May 2017. Accepted: 13 July 2017. Published online: 28 November 2017. Acknowledgements. N.H.R. acknowledges support from the Deutsche Forschungsgemeinschaft through project MI 1230/4-1. V.S. and I.D. acknowledge the European Union’s Seventh Framework programme under grant agreement 337595 (ERC Starting Grant, “CoSMass”). P.N.B. is grateful for support from STFC via grant ST/M001229/1. We wish to thank the anonymous referee for the helpful comments, which have improved this paper. This research made use of Topcat (Taylor 2005), available at http://www.starlink.ac.uk/topcat/. This research also made use of APLpy, an open-source plotting package for Python hosted at http://aplpy.github.com, and Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al. 2013). We wish to thank the staff of the VLBA who greatly supported the experimental observations in this project. The VLBA is operated by the Long Baseline Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Created on2020-02-27 20:36:16