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researcher

K. Sheth

160 papers hereh-index 6616.2k citations317 works total

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

author position
  • sole author1
  • first author9
  • middle author107
  • last author19

Across the 136 of 160 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA79
  • astro-ph43
  • astro-ph.CO30
  • astro-ph.IM7
  • astro-ph.SR1
same name
  • K. Sheth — 21 papers, h 7
  • K. Sheth — 10 papers, h 4
  • K. Sheth — 4 papers, h 2
  • K. Sheth — 3 papers, h 3
  • K. Sheth — 1 paper, h 65
  • K. Sheth — 1 paper, h 15

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
19992026
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations · 17.9k across the 157 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2013★ 57 cited

Unveiling the Structure of Barred Galaxies at 3.6 μm with the Spitzer Survey of Stellar Structure in Galaxies (S4G): I. Disk Breaks

Taehyun Kim, Dimitri A. Gadotti, Kartik Sheth +24

We have performed two-dimensional multicomponent decomposition of 144 local barred spiral galaxies using 3.6 μm images from the Spitzer Survey of Stellar Structure in Galax…

astro-ph.GA2013★ 24 cited

Embedded Star Formation in S4G Galaxy Dust Lanes

Debra M. Elmegreen, Bruce G. Elmegreen, Santiago Erroz-Ferrer +22

Star-forming regions that are visible at 3.6 microns and Halpha but not in the u,g,r,i,z bands of the Sloan Digital Sky survey (SDSS), are measured in five nearby spiral galaxies t…

astro-ph.GA2013★ 89 cited

Submillimeter ALMA Observations of the Dense Gas in the Low-Luminosity Type-1 Active Nucleus of NGC 1097

Takuma Izumi, Kotaro Kohno, Sergio Martín +23

We present the first 100 pc scale view of the dense molecular gas in the central ~ 1.3 kpc region of the type-1 Seyfert NGC 1097 traced by HCN (J=4-3) and HCO+ (J=4-3) lines afford…

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