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researcher

A. Wasserman

13 papers hereh-index 13455 citations24 works total

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

author position
  • first author3
  • middle author8
  • last author2

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA12
  • astro-ph.HE1
same name
  • A. Wasserman — 14 papers, h 21
  • A. Wasserman — 6 papers, h 5
  • A. Wasserman — 5 papers, h 1
  • A. Wasserman — 1 paper, h 2
  • A. Wasserman — 1 paper, 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
20172020
most citedSpatially-resolved stellar kinematics of the ultra diffuse galaxy Dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits

112 citations · 693 across the 13 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019★ 44 cited

How Accurately Can We Detect the Splashback Radius of Dark Matter Halos and its Correlation With Accretion Rate?

Enia Xhakaj, Benedikt Diemer, Alexie Leauthaud +5

The splashback radius (Rsp​) of dark matter halos has recently been detected using weak gravitational lensing and cross-correlations with galaxies. However, different metho…

astro-ph.GA2019★ 53 cited

Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter

Asher Wasserman, Pieter van Dokkum, Aaron J. Romanowsky +9

Given the absence of directly detected dark matter (DM) as weakly interacting massive particles, there is strong interest in the possibility that DM is an ultra-light scalar field,…

astro-ph.GA2019★ 112 cited

Spatially-resolved stellar kinematics of the ultra diffuse galaxy Dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits

Pieter van Dokkum, Asher Wasserman, Shany Danieli +8

We present spatially-resolved stellar kinematics of the well-studied ultra diffuse galaxy (UDG) Dragonfly 44, as determined from 25.3 hrs of observations with the Keck Cosmic Web I…

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