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researcher

R. Benjamin

71 papers hereh-index 325.4k citations170 works total

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

author position
  • sole author1
  • first author4
  • middle author50
  • last author6

Across the 61 of 71 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA34
  • astro-ph26
  • astro-ph.HE3
  • astro-ph.SR3
  • astro-ph.CO2
  • astro-ph.IM2
same name
  • R. Benjamin — 8 papers, h 6
  • R. Benjamin — 4 papers, h 6
  • R. Benjamin — 2 papers, h 2
  • R. Benjamin — 1 paper, 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
19962023
most citedThe Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data

848 citations · 4.9k across the 70 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.GA2011★ 409 cited

VVV DR1: The First Data Release of the Milky Way Bulge and Southern Plane from the Near-Infrared ESO Public Survey VISTA Variables in the Via Lactea

R. K. Saito, M. Hempel, D. Minniti +107

The ESO Public Survey VISTA Variables in the Via Lactea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for…

astro-ph.GA2011

MHD simulations of a supernova-driven ISM and the warm ionized medium using a positivity preserving ideal MHD scheme

Mordecai-Mark Mac Low, Alex S. Hill, M. Ryan Joung +6

We present new 3D magnetohydrodynamic (MHD) simulations of a supernova-driven, stratified interstellar medium. These simulations were run using the Waagan (2009) positivity preserv…

astro-ph.CO2011★ 25 cited

Infrared Spectroscopy of Halos of Edge-on Galaxies

Richard J. Rand, Kenneth Wood, Robert A. Benjamin +1

We present a study of ionized gas, PAHs, and molecular hydrogen emission in the halos of three edge-on galaxies, NGC 891, NGC 5775 and NGC 3044, based on 10-20 micron Spitzer Space…

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