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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.

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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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, i sur.. The faint radio sky: VLBA observations of the COSMOS field. Astronomy and Astrophysics [Internet]. 2017. [pristupljeno 08.11.2024.];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]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:783968. [Citirano: 08.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:783968
Podaci o radu
Naslov (engleski)The faint radio sky: VLBA observations of the COSMOS field
AutorN. Herrera Ruiz
AutorE. Middelberg
AutorA. Deller
AutorR. P. Norris
AutorP. N. Best
AutorW. Brisken
AutorE. Schinnerer
AutorVernesa Smolčić
MBZ: 336180
AutorI. Delvecchio
AutorE. Momjian
AutorD. Bomans
AutorN. Z. Scoville
AutorC. Carilli
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
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.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstronomy and Astrophysics
Brojčani podacivol. 607, A132
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201731163
URN:NBNurn:nbn:hr:217:783968
Datum objave publikacije2017
URL dokumentahttps://www.aanda.org/articles/aa/abs/2017/11/aa31163-17/aa31163-17.html
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 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.
Datum i vrijeme pohrane2020-02-27 20:36:16