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researcher

S. Kent

69 papers hereh-index 5531.7k citations120 works total

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

author position
  • middle author32

Across the 32 of 69 papers where every author was matched, so the position is known.

fields
  • astro-ph26
  • astro-ph.CO21
  • astro-ph.IM11
  • astro-ph.HE5
  • astro-ph.EP3
  • astro-ph.GA3
same name
  • S. Kent — 37 papers, h 48
  • S. Kent — 24 papers, h 21
  • S. Kent — 19 papers, h 14
  • S. Kent — 5 papers
  • S. Kent — 2 papers, h 2
  • S. Kent — 2 papers, h 1

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 citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations · 28.7k across the 68 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.IMShow all

3 papers · 2 filters

astro-ph.IM2017★ 10 cited

ProtoDESI: First On-Sky Technology Demonstration for the Dark Energy Spectroscopic Instrument

Parker Fagrelius, Behzad Abareshi, Lori Allen +33

The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the universe using the baryon acoustic oscillations technique. The spectra…

astro-ph.IM2017★ 107 cited

Forward Global Photometric Calibration of the Dark Energy Survey

D. Burke, E. S. Rykoff, S. Allam +56

Many scientific goals for the Dark Energy Survey (DES) require calibration of optical/NIR broadband b=grizY photometry that is stable in time and uniform over the celestial sky…

astro-ph.IM2017★ 66 cited

Astrometric calibration and performance of the Dark Energy Camera

G. M. Bernstein, R. Armstrong, A. A. Plazas +53

We characterize the ability of the Dark Energy Camera (DECam) to perform relative astrometry across its 500~Mpix, 3 deg^2 science field of view, and across 4 years of operation. Th…

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