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researcher

J. D. Smith

3 papers here

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

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph1
ORCID 0000-0003-1545-5078
same name
  • J. D. Smith — 17 papers, h 6
  • J. D. Smith — 13 papers
  • J. D. Smith — 10 papers, h 6
  • J. D. Smith — 9 papers, h 6
  • J. D. Smith — 6 papers, h 11
  • J. D. Smith — 5 papers, h 4

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
20062025
most citedWarm Dust and Spatially Variable PAH Emission in the Dwarf Starburst Galaxy NGC 1705

43 citations · 51 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2025

A Spectroscopically Calibrated Prescription for Extracting PAH Flux from JWST MIRI Imaging

Grant P. Donnelly, Thomas S. -Y. Lai, Lee Armus +24

We introduce a prescription for estimating the flux of the 7.7 micron and 11.3 micron\ polycyclic aromatic hydrocarbon (PAH) features from broadband JWST/MIRI images. Probing PAH f…

astro-ph.GA2024★ 8 cited

Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA

L. Bisigello, C. Gruppioni, A. Bolatto +11

The most active phases of star formation and black hole accretion are strongly affected by dust extinction, making far-infrared (far-IR) observations the best way to disentangle an…

astro-ph2006★ 43 cited

Warm Dust and Spatially Variable PAH Emission in the Dwarf Starburst Galaxy NGC 1705

John M. Cannon, John-David T. Smith, Fabian Walter +22

We present Spitzer observations of the dwarf starburst galaxy NGC 1705 obtained as part of SINGS. The galaxy morphology is very different shortward and longward of ~5 microns: shor…

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