◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

R. Anderson

4 papers hereh-index 4164 citations4 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • astro-ph1
  • astro-ph.GA1
same name
  • R. Anderson — 52 papers, h 22
  • R. Anderson — 39 papers, h 27
  • R. Anderson — 19 papers, h 14
  • R. Anderson — 14 papers, h 16
  • R. Anderson — 13 papers, h 17
  • R. Anderson — 10 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
20082023
most citedThe Infrared Light Curve of SN 2011fe in M101 and the Distance to M101

73 citations · 124 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2023★ 4 cited

CATS: The Hubble Constant from Standardized TRGB and Type Ia Supernova Measurements

D. Scolnic, A. G. Riess, J. Wu +7

The Tip of the Red Giant Branch (TRGB) provides a luminous standard candle for constructing distance ladders to measure the Hubble constant. In practice its measurements via edge-d…

astro-ph.CO2012★ 73 cited

The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101

T. Matheson, R. R. Joyce, L. E. Allen +42

We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light cur…

astro-ph.GA2010★ 37 cited

New g'r'i'z' Photometry of the NGC 5128 Globular Cluster System

B. Sinnott, A. Hou, R. Anderson +2

We present new photometry for 323 of the globular clusters in NGC 5128 (Centaurus A), measured for the first time in the g′r′i′z′ filter system. The color indices are calibrated…

astro-ph2008★ 10 cited

QU Carinae: a SNeIa progenitor?

S. Kafka, R. Anderson, R. K. Honeycutt

Optical spectra obtained in 2006-07 of the nova-like cataclysmic variable QU Car are studied for radial velocities, line profiles, and line identifications. We are not able to conf…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.