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Stella Seitz

38 papers hereh-index 252k citations42 works total

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

author position
  • first author1
  • middle author28
  • last author2

Across the 31 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO13
  • astro-ph.GA12
  • astro-ph10
  • astro-ph.SR2
  • astro-ph.HE1
same name
  • Stella Seitz — 4 papers, h 3
  • Stella Seitz — 3 papers, h 1
  • Stella Seitz — 2 papers, h 2

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
19972019
most citedThe KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7

597 citations · 2.6k across the 38 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 36 cited

Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members

A. Monna, S. Seitz, A. Zitrin +14

We use velocity dispersion measurements of 21 individual cluster members in the core of Abell 383, obtained with MMT Hectospec, to separate the galaxy and the smooth dark halo (DH)…

astro-ph.GA2014★ 597 cited

The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7

E. Wisnioski, N. M. Förster Schreiber, S. Wuyts +24

We present the KMOS^3D survey, a new integral field survey of over 600 galaxies at 0.7<z<2.7 using KMOS at the Very Large Telescope (VLT). The KMOS^3D survey utilizes synergies wit…

astro-ph.GA2014★ 50 cited

Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS

G. Gozaliasl, A. Finoguenov, H. G. Khosroshahi +15

We present a catalog of 129 X-ray galaxy groups, covering a redshift range 0.04<z<1.23, selected in the ~3 square degree part of the CFHTLS W1 field overlapping XMM observations pe…

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