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O. Almaini

2 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph2
ORCID 0000-0001-9328-3991
same name
  • O. Almaini — 6 papers, h 60

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedEvidence for a large fraction of Compton-thick quasars at high redshift

45 citations · 71 across the 2 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 51 cited

The clustering and abundance of star-forming and passive galaxies at z∼2

W. G. Hartley, K. P. Lane, O. Almaini +8

We use the UKIDSS Ultra-deep survey (UDS), currently the deepest panoramic near infra-red survey, together with deep Subaru optical imaging to measure the clustering, number counts…

astro-ph2008★ 62 cited

A Pilot Survey for KX QSOs in the UKIDSS Ultra Deep Survey Field

Ian Smail, Rob Sharp, A. M. Swinbank +5

We have undertaken a pilot survey for faint QSOs in the UKIDSS Ultra Deep Survey Field using the KX selection technique. These observations exploit the very deep near-infrared and…

astro-ph2006★ 45 cited

Evidence for a large fraction of Compton-thick quasars at high redshift

Alejo Martinez-Sansigre, Steve Rawlings, David G. Bonfield +7

Using mid-infrared and radio selection criteria, we pre-select a sample of candidate high-redshift type-2 quasars in the Subaru XMM-Newton Deep Field (SXDF). To filter out starburs…

astro-ph2006★ 26 cited

0.5 Mpc-scale extended X-ray emission in 4C 23.56

O. Johnson, O. Almaini, P. N. Best +1

We present an XMM-Newton observation of the radio galaxy 4C 23.56 at z=2.48 which reveals extended X-ray emission coincident with the radio lobes spanning \~0.5 Mpc. These are the…

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