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Omar Almaini

Identifiers

  • name variant Omar Almaini 0.60 · backfill

Papers (43)

  1. The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances astro-ph.GA · 2026 · author #2
  2. No hidden monsters: Probing recently-quenched galaxies for obscured AGN with JWST-PRIMER MIRI and NIRCam astro-ph.GA · 2026 · author #2
  3. Tracing Radio AGN-Driven Quenching in Post-Starburst Galaxies at Cosmic Noon astro-ph.GA · 2026 · author #4
  4. The JWST EXCELS survey: The ages and abundances of $3<z<5$ massive quiescent galaxies show that downsizing was already in place by $z\simeq4$ astro-ph.GA · 2026 · author #11
  5. The JWST EXCELS survey: Outflows in 1.5 < z < 5 quiescent and recently quenched galaxies are likely relics from episodic AGN activity astro-ph.GA · 2026 · author #4
  6. X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field astro-ph.GA · 2018 · author #12
  7. Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models astro-ph.GA · 2018 · author #3
  8. Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS astro-ph.CO · 2018 · author #8
  9. CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2 astro-ph.GA · 2017 · author #14
  10. Massive post-starburst galaxies at z > 1 are compact proto-spheroids astro-ph.GA · 2017 · author #1
  11. SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-End Counts at 450 um astro-ph.GA · 2017 · author #9
  12. Enhancement of AGN in a protocluster at z=1.6 astro-ph.GA · 2017 · author #3
  13. A consistent measure of the merger histories of massive galaxies using close-pair statistics I: Major mergers at $z < 3.5$ astro-ph.GA · 2017 · author #4
  14. Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELS astro-ph.GA · 2016 · author #16
  15. Exploring the progenitors of brightest cluster galaxies at z~2 astro-ph.GA · 2016 · author #4
  16. Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses astro-ph.GA · 2016 · author #5
  17. The Evolution of Galaxies at Constant Number Density: A Less Biased View of Star Formation, Quenching, and Structural Formation astro-ph.GA · 2016 · author #7
  18. The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field astro-ph.GA · 2016 · author #2
  19. The Science Case for Multi-Object Spectroscopy on the European ELT astro-ph.GA · 2015 · author #4
  20. Deconstructing the Galaxy Stellar Mass Function with UKIDSS and CANDELS: the Impact of Colour, Structure and Environment astro-ph.GA · 2014 · author #7
  21. Minor vs Major Mergers: The Stellar Mass Growth of Massive Galaxies from z=3 using Number Density Selection Techniques astro-ph.GA · 2014 · author #5
  22. Galaxy Zoo: CANDELS Barred Disks and Bar Fractions astro-ph.GA · 2014 · author #16
  23. Evidence for a correlation between the sizes of quiescent galaxies and local environment to z ~ 2 astro-ph.CO · 2013 · author #2
  24. The prevalence of AGN feedback in massive galaxies at z~1 astro-ph.CO · 2013 · author #6
  25. The Redshift and Mass Dependence on the Formation of The Hubble Sequence at z>1 from CANDELS/UDS astro-ph.CO · 2013 · author #7
  26. CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field astro-ph.CO · 2013 · author #20
  27. CANDELS Observations of the Environmental Dependence of the Color-Mass-Morphology Relation at z = 1.6 astro-ph.CO · 2013 · author #8
  28. Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2 astro-ph.CO · 2013 · author #2
  29. The Nature of Extremely Red H-[4.5]>4 Galaxies revealed with SEDS and CANDELS astro-ph.CO · 2012 · author #10
  30. Radio imaging of the Subaru/XMM-Newton Deep Field - III. Evolution of the radio luminosity function beyond z=1 astro-ph.CO · 2012 · author #5
  31. CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey astro-ph.CO · 2011 · author #9
  32. Average Metallicity and Star Formation Rate of Lya Emitters Probed by a Triple Narrow-Band Survey astro-ph.CO · 2011 · author #11
  33. On the co-evolution of supermassive black holes and their host galaxies since z = 3 astro-ph.CO · 2010 · author #3
  34. The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies astro-ph.CO · 2010 · author #2
  35. Exploring the infrared/radio correlation at high redshift astro-ph · 2008 · author #9
  36. Evidence for a large fraction of Compton-thick quasars at high redshift astro-ph · 2006 · author #7
  37. Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release astro-ph · 2006 · author #2
  38. Dust and gas obscuration in ELAIS Deep X-ray Survey reddened quasars astro-ph · 2004 · author #3
  39. The Nature, Evolution, Clustering and X-ray Properties of Extremely Red Galaxies in the CDFS/GOODS field astro-ph · 2003 · author #3
  40. Deep radio imaging of the SCUBA 8-mJy survey fields: sub-mm source identifications and redshift distribution astro-ph · 2002 · author #10
  41. The Clustering, Number Counts and Morphology of Extremely Red (R-K>5) Galaxies to K=21 astro-ph · 2002 · author #2
  42. Using STIS to find Gamma-Ray Burst Redshifts astro-ph · 1997 · author #4
  43. A deep ROSAT Survey - XII. The X-ray spectra of faint ROSAT sources astro-ph · 1996 · author #1

Mentions

  • 2607.00085 #2 · arxiv_oai · confidence 0.70 Omar Almaini
  • 2606.20800 #2 · arxiv_oai · confidence 0.70 Omar Almaini
  • 1501.04726 #4 · backfill · confidence 0.70 Omar Almaini
  • 1411.3339 #7 · backfill · confidence 0.70 Omar Almaini
  • 1409.1582 #5 · backfill · confidence 0.70 Omar Almaini
  • 1409.1214 #16 · backfill · confidence 0.70 Omar Almaini
  • 1307.3247 #2 · backfill · confidence 0.70 Omar Almaini
  • 1307.0502 #6 · backfill · confidence 0.70 Omar Almaini
  • 1305.2204 #7 · backfill · confidence 0.70 Omar Almaini
  • 1305.1823 #20 · backfill · confidence 0.70 Omar Almaini
  • 1305.0607 #8 · backfill · confidence 0.70 Omar Almaini
  • 1303.0816 #2 · backfill · confidence 0.70 Omar Almaini
  • 1202.0496 #10 · backfill · confidence 0.70 Omar Almaini
  • 1201.3225 #5 · backfill · confidence 0.70 Omar Almaini
  • 1105.3753 #9 · backfill · confidence 0.70 Omar Almaini
  • 1105.2824 #11 · backfill · confidence 0.70 Omar Almaini
  • 1008.2162 #3 · backfill · confidence 0.70 Omar Almaini
  • 1005.1180 #2 · backfill · confidence 0.70 Omar Almaini
  • 0802.2694 #9 · backfill · confidence 0.70 Omar Almaini

Frequent Coauthors