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researcher

N. Smith

11 papers hereh-index 63.3k citations16 works total

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

author position
  • first author1
  • middle author8
  • last author1

Across the 10 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE6
  • astro-ph.SR4
  • astro-ph.GA1
same name
  • N. Smith — 276 papers, h 71
  • N. Smith — 60 papers, h 12
  • N. Smith — 38 papers, h 30
  • N. Smith — 20 papers, h 14
  • N. Smith — 19 papers, h 59
  • N. Smith — 18 papers

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
20152026
most citedA surge of light at the birth of a supernova

114 citations · 254 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

4 papers · 1 filter

astro-ph.SR2026

The Age of the R127 & R128 Clusters: Implications for the LBV

Mojgan Aghakhanloo, Jeremiah W. Murphy, Nathan Smith +1

We infer the age of the R127 and R128 clusters in the Large Magellanic Cloud (LMC) using Strömgren photometry from the literature and the age-dating algorithm, Stellar Ages. Analys…

astro-ph.SR2025

Simulating Chemical Abundances in the Circumstellar Nebula of the Late Stage Binary RY Scuti

Sarah H. Taft, Robert D. Gehrz, Charles E. Woodward +3

RY Scuti, thought to be a Wolf-Rayet (WR) progenitor, is a massive, post-main-sequence, binary star system undergoing Roche lobe overflow (RLOF). SOFIA (+FORCAST) spectroscopy of t…

astro-ph.SR2024

The Statistics and Environments of Hostless Supernovae

Yu-Jing Qin, Ann Zabludoff, Iair Arcavi +3

Transient surveys routinely detect supernovae (SNe) without obvious host galaxies. To understand the demographics of these "hostless" SNe and to constrain the possible host propert…

astro-ph.SR2015

SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment

J. D. Adams, T. L. Herter, J. L. Hora +22

We present mid-IR (19 - 37 microns) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6 - 8.0 microns), IRTF/MIRLIN (11.3 and…

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