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S. Jensen

3 papers hereh-index 589 citations10 works total

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

author position
  • first author1
  • middle author2

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

fields
  • astro-ph.SR2
  • astro-ph.EP1
same name
  • S. Jensen — 14 papers, h 7
  • S. Jensen — 9 papers, h 35
  • S. Jensen — 8 papers, h 6
  • S. Jensen — 5 papers, h 4
  • S. Jensen — 3 papers, h 15
  • S. Jensen — 3 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
20222026
most citedScanning disk rings and winds in CO at 0.01-10 au: a high-resolution M-band spectroscopy survey with IRTF-iSHELL

63 citations · 63 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2026

12CO Ro-vibrational Spectroscopy of AB Aurigae -- A Potential Point Source is Present

Janus Kozdon, Jeffrey Fung, Sean D. Brittain +4

The Herbig Ae star AB Aurigae hosts a vast, low-inclination protoplanetary disk that exhibits a plethora of substructures, including the protoplanet candidate AB Aur b. We present…

astro-ph.SR2024

Spectroastrometric Survey of Protoplanetary Disks with Inner Dust Cavities

Stanley K. Jensen, Sean D. Brittain, Andrea Banzatti +6

We present high-resolution spectra and spectroastrometric (SA) measurements of fundamental rovibrational CO emission from nine nearby (≲300 pc) protoplanetary disks where…

astro-ph.SR2022★ 63 cited

Scanning disk rings and winds in CO at 0.01-10 au: a high-resolution M-band spectroscopy survey with IRTF-iSHELL

Andrea Banzatti, Kirsten M. Abernathy, Sean Brittain +11

We present an overview and first results from a M-band spectroscopic survey of planet-forming disks performed with iSHELL on IRTF, using two slits that provide resolving power R…

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