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researcher

S. Mateos

16 papers here

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

author position
  • first author1
  • middle author8
  • last author3

Across the 12 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph.HE5
  • astro-ph.CO3
  • astro-ph2
ORCID 0000-0002-1375-2389
same name
  • S. Mateos — 32 papers, h 24
  • S. Mateos — 18 papers, h 12
  • S. Mateos — 2 papers, h 1
  • S. Mateos — 1 paper, h 0

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
20002017
most citedUsing the Bright Ultra-Hard XMM-Newton Survey to define an IR selection of luminous AGN based on WISE colours

351 citations · 638 across the 16 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

3 papers · 1 filter

astro-ph.CO2012★ 6 cited

Black-hole masses of type 1 AGN in the XMM-Newton bright serendipitous survey

A. Caccianiga, R. Fanali, P. Severgnini +3

We derive masses of the central super-massive black hole (SMBH) and accretion rates for 154 type1 AGN belonging to a well-defined X-ray-selected sample, the XMM-Newton Serendipitou…

astro-ph.CO2012★ 351 cited

Using the Bright Ultra-Hard XMM-Newton Survey to define an IR selection of luminous AGN based on WISE colours

S. Mateos, A. Alonso-Herrero, F. J. Carrera +7

We present a highly complete and reliable mid-infrared (MIR) colour selection of luminous AGN candidates using the 3.4, 4.6, and 12 um bands of the WISE survey. The MIR colour wedg…

astro-ph.CO2010

On the arcmin structure of the X-ray Universe

J. Ebrero, S. Mateos, G. C. Stewart +1

We present the angular correlation function of the X-ray population of 1063 XMM-Newton observations at high Galactic latitudes, comprising up to ~30000 sources over a sky area of ~…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.