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C. Lagos

21 papers hereh-index 14776 citations39 works total

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

author position
  • middle author16

Across the 16 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA20
  • astro-ph.IM1
same name
  • C. Lagos — 102 papers, h 47
  • C. Lagos — 21 papers, h 4
  • C. Lagos — 13 papers, h 4
  • C. Lagos — 12 papers, h 1
  • C. Lagos — 5 papers, h 2
  • C. Lagos — 3 papers, h 1

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
20142024
most citedCompact starbursts in z~3-6 submillimeter galaxies revealed by ALMA

200 citations · 565 across the 21 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023★ 10 cited

ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale

Jianhang Chen, R. J. Ivison, Martin A. Zwaan +6

It may be unsurprising that the most common approach to finding proto-clusters is to search for over-densities of galaxies. Upgrades to submillimetre (submm) interferometers and th…

astro-ph.GA2023★ 4 cited

ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at z≃1−8

Seiji Fujimoto, Kotaro Kohno, Masami Ouchi +40

We present a statistical study of 180 dust continuum sources identified in 33 massive cluster fields by the ALMA Lensing Cluster Survey (ALCS) over a total of 133 arcmin2 area…

astro-ph.GA2023★ 48 cited

COSMOS2020: Exploring the dawn of quenching for massive galaxies at 3 < z < 5 with a new colour selection method

Katriona M. L. Gould, Gabriel Brammer, Francesco Valentino +15

We select and characterise a sample of massive (log(M∗​/M⊙​)>10.6) quiescent galaxies (QGs) at 3<z<5 in the latest COSMOS2020 catalogue. QGs are selected using a new…

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