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Extending the variability selection of active galactic nuclei in the W-CDF-S and SERVS/SWIRE region

Poulain, M. (författare)
Univ Innsbruck, Inst Astro & Teilchenphys, Technikerstr 25-8, A-6020 Innsbruck, Austria.
Paolillo, M. (författare)
Univ Napoli Federico II, Dept Phys, Via Cinthia 9, I-80126 Naples, Italy.;Ist Nazl Fis Nucl, Sez Napoli, Via Cinthia 9, I-80126 Naples, Italy.;INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
De Cicco, D. (författare)
Univ Napoli Federico II, Dept Phys, Via Cinthia 9, I-80126 Naples, Italy.;Millennium Inst Astrophys MAS, Nuncio Monsenor Sotero Sanz 100, Santiago, Chile.;Pontificia Univ Catolica Chile, Inst Astrofis, Av Vicuna Mackenna 4860, Santiago 7820436, Spain.
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Brandt, W. N. (författare)
Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA.;Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA.
Bauer, F. E. (författare)
Millennium Inst Astrophys MAS, Nuncio Monsenor Sotero Sanz 100, Santiago, Chile.;Pontificia Univ Catolica Chile, Inst Astrofis, Av Vicuna Mackenna 4860, Santiago 7820436, Spain.;Space Sci Inst, 4750 Walnut St,Suite 2015, Boulder, CO 80301 USA.
Falocco, Serena (författare)
KTH,Partikel- och astropartikelfysik
Vagnetti, F. (författare)
Univ Roma Tor Vergata, Dept Phys, Via Ric Sci 1, I-00133 Rome, Italy.
Grado, A. (författare)
INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
Ragosta, F. (författare)
Univ Napoli Federico II, Dept Phys, Via Cinthia 9, I-80126 Naples, Italy.;Ist Nazl Fis Nucl, Sez Napoli, Via Cinthia 9, I-80126 Naples, Italy.;INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
Botticella, M. T. (författare)
INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
Cappellaro, E. (författare)
INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
Pignata, G. (författare)
Millennium Inst Astrophys MAS, Nuncio Monsenor Sotero Sanz 100, Santiago, Chile.;Univ Andres Bello, Dept Ciencias Fis, Avda Republ 252, Santiago, Chile.
Vaccari, M. (författare)
Univ Western Cape, Dept Phys & Astron, Private Bag X17, ZA-7535 Cape Town, South Africa.;INAF, Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy.
Schipani, P. (författare)
INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
Covone, G. (författare)
Univ Napoli Federico II, Dept Phys, Via Cinthia 9, I-80126 Naples, Italy.;Ist Nazl Fis Nucl, Sez Napoli, Via Cinthia 9, I-80126 Naples, Italy.
Longo, G. (författare)
Univ Napoli Federico II, Dept Phys, Via Cinthia 9, I-80126 Naples, Italy.;Ist Nazl Fis Nucl, Sez Napoli, Via Cinthia 9, I-80126 Naples, Italy.;INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
Napolitano, N. R. (författare)
Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai Campus, Guangzhou 519082, Peoples R China.
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Univ Innsbruck, Inst Astro & Teilchenphys, Technikerstr 25-8, A-6020 Innsbruck, Austria Univ Napoli Federico II, Dept Phys, Via Cinthia 9, I-80126 Naples, Italy.;Ist Nazl Fis Nucl, Sez Napoli, Via Cinthia 9, I-80126 Naples, Italy.;INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy. (creator_code:org_t)
2020-02-05
2020
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP SCIENCES S A. - 0004-6361 .- 1432-0746. ; 634
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. Variability has proven to be a powerful tool to detect active galactic nuclei (AGN) in multi-epoch surveys. The new-generation facilities expected to become operational in the next few years will mark a new era in time-domain astronomy and their wide-field multi-epoch campaigns will favor extensive variability studies.Aims. We present our analysis of AGN variability in the second half of the VST survey of the Wide Chandra Deep Field South, performed in the r band and covering a 2 sq. deg area. The analysis complements a previous work, in which the first half of the area was investigated. We provide a reliable catalog of variable AGN candidates, which will be critical targets in future variability studies.Methods. We selected a sample of optically variable sources and made use of infrared data from the Spitzer mission to validate their nature by means of color-based diagnostics.Results. We obtain a sample of 782 AGN candidates among which 12 are classified as supernovae, 54 as stars, and 232 as AGN. We estimate a contamination less than or similar to 20% and a completeness similar to 38% with respect to mid-infrared selected samples.

Ämnesord

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Nyckelord

galaxies: active
infrared: galaxies
surveys

Publikations- och innehållstyp

ref (ämneskategori)
art (ämneskategori)

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