activity
20052023
most citedLas Cumbres Observatory Global Telescope Network

1.2k citations · 26.3k across the 277 of their papers we have counts for

collaborators
Showing 2010Show all

14 papers · 1 filter

astro-ph.SR2010★ 7 cited

The LCOGT Network

A. Shporer, T. Brown, T. Lister +5

Motivated by the increasing need for observational resources for the study of time varying astronomy, the Las Cumbres Observatory Global Telescope (LCOGT) is a private foundation,…

astro-ph.SR2010★ 83 cited

A ground-based measurement of the relativistic beaming effect in a detached double WD binary

Avi Shporer, David L. Kaplan, Justin D. R. Steinfadt +3

We report on the first ground-based measurement of the relativistic beaming effect (aka Doppler boosting). We observed the beaming effect in the detached, non-interacting eclipsing…

astro-ph.EP2010★ 42 cited

A sub-Saturn Mass Planet, MOA-2009-BLG-319Lb

N. Miyake, T. Sumi, Subo Dong +119

We report the gravitational microlensing discovery of a sub-Saturn mass planet, MOA-2009-BLG-319Lb, orbiting a K or M-dwarf star in the inner Galactic disk or Galactic bulge. The h…

astro-ph.EP2010★ 84 cited

Orbital Orientations of Exoplanets: HAT-P-4b is Prograde and HAT-P-14b is Retrograde

Joshua N. Winn, Andrew W. Howard, John Asher Johnson +9

We present observations of the Rossiter-McLaughlin effect for two exoplanetary systems, revealing the orientations of their orbits relative to the rotation axes of their parent sta…

astro-ph.EP2010★ 97 cited

A Possible Tilted Orbit of the Super-Neptune HAT-P-11b

Teruyuki Hirano, Norio Narita, Avi Shporer +3

We report the detection of the Rossiter-McLaughlin effect for the eccentric, super-Neptune exoplanet HAT-P-11b, based on radial velocity measurements taken with HDS mounted on the…

astro-ph.EP2010★ 173 cited

The Oblique Orbit of the Super-Neptune HAT-P-11b

Joshua N. Winn, John Asher Johnson, Andrew W. Howard +6

We find the orbit of the Neptune-sized exoplanet HAT-P-11b to be highly inclined relative to the equatorial plane of its host star. This conclusion is based on spectroscopic observ…