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M. Kohandel

39 papers hereh-index 11285 citations38 works total

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

author position
  • first author3
  • middle author28
  • last author6

Across the 37 of 39 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA30
  • astro-ph.IM5
  • gr-qc2
  • physics.gen-ph1
  • quant-ph1
same name
  • M. Kohandel — 23 papers, h 29

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
20132026
most citedBlue Monsters. Why are JWST super-early, massive galaxies so blue?

76 citations · 529 across the 32 of their papers we have counts for

collaborators
Showing 2022Show all

4 papers · 1 filter

astro-ph.GA2022★ 28 cited

[CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?

E. Pizzati, A. Ferrara, A. Pallottini +3

ALMA observations have revealed that many high redshift galaxies are surrounded by extended (10-15 kpc) [CII]-emitting halos which are not predicted by even the most advanced zoom-…

astro-ph.GA2022★ 18 cited

Interpreting ALMA non-detections of JWST super-early galaxies

M. Kohandel, A. Ferrara, A. Pallottini +3

Recent attempts to detect [OIII] 88μm emission from super-early (z>10) galaxy candidates observed by JWST have been unsuccessful. By using zoom-in simulations, we show that the…

astro-ph.GA2022★ 76 cited

Blue Monsters. Why are JWST super-early, massive galaxies so blue?

Francesco Ziparo, Andrea Ferrara, Laura Sommovigo +1

The recent JWST tentative discovery of a population of super-early (redshift z>10), relatively massive (stellar mass M∗​=108−9M⊙​) and evolved (metallicity $Z \app…

astro-ph.GA2022★ 60 cited

Dynamical characterization of galaxies up to z∼7

F. Rizzo, M. Kohandel, A. Pallottini +4

The characterization of the dynamical state of galaxies up to z~7 is crucial for constraining the mechanisms driving the mass assembly in the early Universe. However, it is unclear…

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