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J. Fritz

36 papers hereh-index 171k citations34 works total

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

author position
  • first author3
  • middle author26
  • last author1

Across the 30 of 36 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA25
  • astro-ph.CO9
  • astro-ph2
same name
  • J. Fritz — 150 papers, h 48
  • J. Fritz — 45 papers, h 30
  • J. Fritz — 26 papers, h 16
  • J. Fritz — 17 papers
  • J. Fritz — 5 papers, h 4
  • J. Fritz — 5 papers, h 3

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
20072026
most citedSuperdense galaxies and the mass-size relation at low redshift

177 citations · 1.7k across the 36 of their papers we have counts for

collaborators
Showing 2015Show all

4 papers · 1 filter

astro-ph.GA2015★ 23 cited

Galaxy Luminosity Functions in WINGS clusters

A. Moretti, D. Bettoni, B. M. Poggianti +9

Using V band photometry of the WINGS survey, we derive galaxy luminosity functions (LF) in nearby clusters. This sample is complete down to Mv=-15.15, and it is homogeneous, thus a…

astro-ph.GA2015★ 176 cited

Jellyfish galaxy candidates at low redshift

B. M. Poggianti, G. Fasano, A. Omizzolo +9

Galaxies that are being stripped of their gas can sometimes be recognized from their optical appearance. Extreme examples of stripped galaxies are the so-called ``jellyfish galaxie…

astro-ph.GA2015★ 96 cited

OmegaWINGS: OmegaCAM@VST observations of WINGS galaxy clusters

M. Gullieuszik, B. Poggianti, G. Fasano +13

The Wide-field Nearby Galaxy-cluster Survey (WINGS) is a wide-field multi-wavelength survey of X-ray selected clusters at z =0.04-0.07. The original 34'x34' WINGS field-of- view ha…

astro-ph.GA2015★ 65 cited

Morphological Fractions of Galaxies in WINGS Clusters: revisiting the Morphology-Density Paradigm

G. Fasano, B. M. Poggianti, D. Bettoni +11

We present the Morphology-Density and Morphology-Radius relations (T-Sigma and T-R, respectively) obtained from the WINGS database of galaxies in nearby clusters. Aiming to achieve…

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