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E. Pouliasis

8 papers hereh-index 8252 citations35 works total

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

author position
  • first author1
  • middle author3
  • last author2

Across the 6 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.SR3
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • E. Pouliasis — 6 papers

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

activity
20182022
most citedAn obscured AGN population hidden in the VIPERS galaxies: identification through spectral energy distribution decomposition

43 citations · 84 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2022★ 1 cited

Comparison of star formation histories of AGN and non-AGN galaxies

G. Mountrichas, V. Buat, G. Yang +6

We use AGN with LX​∼1042.5−44ergs−1, from the COSMOS-Legacy survey that lie within the UltraVISTA region and cross match them with the LEGA-C catalogue. The…

astro-ph.GA2020★ 43 cited

An obscured AGN population hidden in the VIPERS galaxies: identification through spectral energy distribution decomposition

E. Pouliasis, G. Mountrichas, I. Georgantopoulos +3

The detection of X-ray emission constitutes a reliable and efficient tool for the selection of Active Galactic Nuclei (AGNs), although it may be biased against the most heavily abs…

astro-ph.GA2019★ 30 cited

Robust Identification of Active Galactic Nuclei through HST Optical Variability in GOODS-S: Comparison with the X-ray and mid-IR Selected Samples

E. Pouliasis, I. Georgantopoulos, A. Z. Bonanos +9

Identifying Active Galactic Nuclei (AGNs) through their X-ray emission is efficient, but necessarily biased against X-ray-faint objects. We aim to characterize this bias by compari…

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