Obscured quasars at high redshift in the UKIDSS Ultra Deep Survey

Ismael Botti, Omar Almaini, Will Hartley, Alice Mortlock, Paulina Lira

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract / Description of output

Obscured quasars hidden in deep X-ray surveys can be recovered by looking at mid-infrared wavelengths, where dust re-radiates the absorbed radiation. Here we present a sample of obscured quasars in the redshift range 1 < z < 4 based on data from the UKIDSS Ultra-Deep Survey (UDS), the deepest near-IR survey over ∼ 1 sq. deg. to date. Candidates that are primarily selected by their 24 μm emission are probed by decomposing their spectral energy distribution (SED) to disentangle the emission from the AGN and its host galaxy. We show preliminary results on their host galaxy properties as well as their clustering, showing that obscured quasars are found in galaxies located in the green valley, residing in dark matter haloes not different from normal galaxies at those redshifts.

Original languageEnglish
Title of host publicationProceedings of the International Astronomical Union
PublisherCambridge University Press
Pages48-51
Number of pages4
Volume9
EditionS304
ISBN (Print)9781107045248
DOIs
Publication statusPublished - 2014

Publication series

NameProceedings of the International Astronomical Union
NumberS304
Volume9
ISSN (Print)17439213
ISSN (Electronic)17439221

Keywords / Materials (for Non-textual outputs)

  • galaxies: evolution
  • galaxies: high-redshift
  • infrared: galaxies
  • quasars: general

Fingerprint

Dive into the research topics of 'Obscured quasars at high redshift in the UKIDSS Ultra Deep Survey'. Together they form a unique fingerprint.

Cite this