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researcher

J. Tyson

48 papers hereh-index 368.3k citations241 works total

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

author position
  • sole author2
  • first author3
  • middle author27
  • last author10

Across the 42 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph24
  • astro-ph.CO12
  • astro-ph.IM9
  • astro-ph.GA2
  • physics.ins-det1
same name
  • J. Tyson — 25 papers, h 28
  • J. Tyson — 8 papers, h 11
  • J. Tyson — 6 papers, h 69
  • J. Tyson — 6 papers, h 3
  • J. Tyson — 5 papers, h 7
  • J. Tyson — 3 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
19942026
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 6k across the 47 of their papers we have counts for

collaborators
Showing 2002Show all

4 papers · 1 filter

astro-ph2002★ 197 cited

Weak Lensing Results from the 75 Square Degree CTIO Survey

M. Jarvis, G. Bernstein, B. Jain +4

We measure seeing-corrected ellipticities for 2 x 10^6 galaxies with magnitude R<23 in 12 widely separated fields totalling 75 deg^2 of sky. At angular scales >30\arcmin, elliptici…

astro-ph2002★ 102 cited

The Deep Lens Survey

D. Wittman, J. A. Tyson, I. P. Dell'Antonio +19

The Deep Lens Survey (DLS) is a deep BVRz' imaging survey of seven 2x2 degree fields, with all data to be made public. The primary scientific driver is weak gravitational lensing,…

astro-ph2002★ 49 cited

Weak Lensing Discovery and Tomography of a Cluster at z=0.68

D. Wittman, V. E. Margoniner, J. A. Tyson +3

We report the weak lensing discovery, spectroscopic confirmation, and weak lensing tomography of a massive cluster of galaxies at z=0.68, demonstrating that shear selection of cl…

astro-ph2002★ 57 cited

LSST: a Complementary Probe of Dark Energy

J. A. Tyson, D. M. Wittman, J. F. Hennawi +1

The number of mass clusters and their distribution in redshift are very sensitive to the density of matter Omega_m and the equation of state of dark energy w. Using weak lens gravi…

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