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researcher

K. Lam

71 papers hereh-index 191.4k citations106 works total

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

author position
  • first author4
  • middle author53

Across the 57 of 71 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP64
  • astro-ph.SR6
  • astro-ph.IM1
same name
  • K. Lam — 17 papers, h 50
  • K. Lam — 16 papers, h 3
  • K. Lam — 12 papers, h 6
  • K. Lam — 10 papers, h 11
  • K. Lam — 5 papers, h 2
  • K. Lam — 4 papers, h 17

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
20142026
most citedSix transiting planets and a chain of Laplace resonances in TOI-178

195 citations · 1.9k across the 68 of their papers we have counts for

collaborators
Showing 2018Show all

4 papers · 1 filter

astro-ph.EP2018★ 22 cited

Detection and characterization of an ultra-dense sub-Neptune planet orbiting the Sun-like star HD 119130

R. Luque, G. Nowak, E. Pallé +51

We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. HD 119130 b is a warm sub-Neptune on a 17-d orbit aroun…

astro-ph.EP2018★ 44 cited

HD219666b: A hot-Neptune from TESS Sector 1

M. Esposito, D. J. Armstrong, D. Gandolfi +73

We report on the confirmation and mass determination of a transiting planet orbiting the old and inactive G7 dwarf star HD219666 (Mstar = 0.92 +/- 0.03 MSun, Rstar = 1.03 +/- 0.03…

astro-ph.EP2018★ 24 cited

K2-265 b: A Transiting Rocky Super-Earth

K. W. F. Lam, A. Santerne, S. G. Sousa +34

We report the discovery of the super-Earth K2-265 b detected with K2 photometry. The planet orbits a bright (V_mag = 11.1) star of spectral type G8V with a period of 2.37 days. We…

astro-ph.EP2018★ 112 cited

An Earth-sized exoplanet with a Mercury-like composition

A. Santerne, B. Brugger, D. J. Armstrong +43

The Earth, Venus, Mars, and some extrasolar terrestrial planets have a mass and radius that is consistent with a mass fraction of about 30% metallic core and 70% silicate mantle. A…

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