prikaz prve stranice dokumenta The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations
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Scientific paper - Original scientific paper
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. More authors...

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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, and sur.. The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations. Astronomy and Astrophysics [Internet]. 2020 [cited 2024 October 01];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]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:053360. [Accessed: 01 October 2024]

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Metadata
Title (english)The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations
Title (english)The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations⋆
AuthorBruno Šlaus
MBZ: 372525
AuthorVernesa Smolčić
MBZ: 336180
AuthorMladen Novak
MBZ: 344074
AuthorS. Fotopoulou
AuthorP. Ciliegi
AuthorN. Jurlin
AuthorLana Ceraj
MBZ: 352661
AuthorKrešimir Tisanić
AuthorM. Birkinshaw
AuthorM. Bremer
AuthorL. Chiappetti
AuthorC. Horellou
AuthorM. Huynh
AuthorH. Intema
AuthorK. Kolokythas
AuthorM. Pierre
AuthorS. Raychaudhury
AuthorH. Rottgering
CollaborationXXL Consortium
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)
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.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleAstronomy and Astrophysics
Numberingvol. 638, A46
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201937258
URN:NBNurn:nbn:hr:217:053360
Publication2020
Document URLhttps://www.aanda.org/component/article?access=doi&doi=10.1051/0004-6361/201937258
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© ESO 2020. Received 4 December 2019. Accepted 29 January 2020. Published online 09 June 2020.
Created on2020-08-27 19:51:21