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The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations
Astronomy and Astrophysics, 638 (2020); A46. https://doi.org/10.1051/0004-6361/201937258
(XXL Consortium) Šlaus, Bruno; Smolčić, Vernesa; Novak, Mladen; Fotopoulou, S.; Ciliegi, P.; Jurlin, N.; Ceraj, Lana; Tisanić, Krešimir; Birkinshaw, M.; Bremer, M.; Chiappetti, L.; Horellou, C.; Huynh, M.; Intema, H.; Kolokythas, K.; Pierre, M.; Raychaudhury, S.; Rottgering, H. Više autora...

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Šlaus, B., Smolčić, V., Novak, M., Fotopoulou, S., Ciliegi, P., Jurlin, N. ... Rottgering, H. (2020). The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations. Astronomy and Astrophysics, 638.. doi: 10.1051/0004-6361/201937258

Šlaus, Bruno, et al. "The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations." Astronomy and Astrophysics, vol. 638, 2020. https://doi.org/10.1051/0004-6361/201937258

Šlaus, Bruno, Vernesa Smolčić, Mladen Novak, S. Fotopoulou, P. Ciliegi, N. Jurlin, Lana Ceraj, et al. "The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations." Astronomy and Astrophysics 638 (2020). https://doi.org/10.1051/0004-6361/201937258

Šlaus, B., et al. (2020) 'The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations', Astronomy and Astrophysics, 638. doi: 10.1051/0004-6361/201937258

Šlaus B, Smolčić V, Novak M, Fotopoulou S, Ciliegi P, Jurlin N, i sur.. The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations. Astronomy and Astrophysics [Internet]. 2020. [pristupljeno 16.04.2024.];638. doi: 10.1051/0004-6361/201937258

B. Šlaus, et al., "The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations", Astronomy and Astrophysics, vol. 638, 2020. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:053360. [Citirano: 16.04.2024.]

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Naslov (engleski)The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations
Naslov (engleski)The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations⋆
AutorBruno Šlaus
MBZ: 372525
AutorVernesa Smolčić
MBZ: 336180
AutorMladen Novak
MBZ: 344074
AutorS. Fotopoulou
AutorP. Ciliegi
AutorN. Jurlin
AutorLana Ceraj
MBZ: 352661
AutorKrešimir Tisanić
AutorM. Birkinshaw
AutorM. Bremer
AutorL. Chiappetti
AutorC. Horellou
AutorM. Huynh
AutorH. Intema
AutorK. Kolokythas
AutorM. Pierre
AutorS. Raychaudhury
AutorH. Rottgering
KolaboracijaXXL Consortium
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
We study the space density evolution of active galactic nuclei (AGN) using the 610 MHz radio survey of the XXL-North field, performed with the Giant Metrewave Radio Telescope. The survey covers an area of 30.4 deg2, with a beamsize of 6.5 arcsec. The survey is divided into two parts, one covering an area of 11.9 deg2 with 1σ rms noise of 200 μJy beam−1 and the other spanning 18.5 deg2 with rms noise of 45 μJy beam−1. We extracted the catalog of radio components above 7σ. The catalog was cross- matched with a multi-wavelength catalog of the XXL-North field (covering about 80% of the radio XXL-North field) using a likelihood ratio method, which determines the counterparts based on their positions and their optical properties. The multi-component sources were matched visually with the aid of a computer code: Multi-Catalog Visual Cross-Matching. A flux density cut above 1 mJy selects AGN hosts with a high purity in terms of star formation contamination based on the available source counts. After cross-matching and elimination of observational biases arising from survey incompletenesses, the number of remaining sources was 1150. We constructed the rest-frame 1.4 GHz radio luminosity functions of these sources using the maximum volume method. This survey allows us to probe luminosities of 23 ≲ log(L1.4 GHz[W Hz−1]) ≲ 28 up to redshifts of z ≈ 2.1. Our results are consistent with the results from the literature in which AGN are comprised of two differently evolving populations, where the high luminosity end of the luminosity functions evolves more strongly than the low-luminosity end.
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. 638, A46
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201937258
URN:NBNurn:nbn:hr:217:053360
Datum objave publikacije2020
URL dokumentahttps://www.aanda.org/component/article?access=doi&doi=10.1051/0004-6361/201937258
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© ESO 2020. Received 4 December 2019. Accepted 29 January 2020. Published online 09 June 2020.
Datum i vrijeme pohrane2020-08-27 19:51:21