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Jeffrey D. McKaig

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.GA2
  • astro-ph.HE1
ORCID 0000-0002-0913-3729

identity via Semantic Scholar / OpenAlex

most citedRay-tracing simulations of the Soft X-ray Scattered Emission in obscured Active Galactic Nuclei

4 citations · 5 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024

Why are optical coronal lines faint in active galactic nuclei?

Jeffrey D. McKaig, Shobita Satyapal, Ari Laor +4

Forbidden collisionally excited optical atomic transitions from high ionization potential (IP≥54.8\,eV) ions, such as Ca4+, Ne4+, Fe$^{\mathrm{6+}}…

astro-ph.GA2024★ 1 cited

Local Analogs of Primordial Galaxies: In Search of Intermediate Mass Black Holes with JWST NIRSpec

Sara Doan, Shobita Satyapal, William Matzko +15

Local low metallicity galaxies with signatures of possible accretion activity are ideal laboratories in which to search for the lowest mass black holes and study their impact on th…

astro-ph.HE2023★ 4 cited

Ray-tracing simulations of the Soft X-ray Scattered Emission in obscured Active Galactic Nuclei

Jeffrey McKaig, Claudio Ricci, Stéphane Paltani +3

Most Active Galactic Nuclei (AGN) in the local Universe are obscured. In these obscured AGN an excess is usually observed in the soft X-rays below ~2 keV above the absorbed X-ray c…

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