activity
19972024
most citedDetection of Rotation in a Binary Microlens: PLANET Photometry of MACHO 97-BLG-41

174 citations · 993 across the 21 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2024

The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array

Nancy Remage Evans, Gail Schaefer, Alexandre Gallenne +19

The 30 year orbit of the Cepheid Polaris has been followed with observations by the CHARA Array (Center for High Angular Resolution Astronomy) from 2016 through 2021. An additional…

astro-ph.SR2014★ 21 cited

The long-period Galactic Cepheid RS Puppis - III. A geometric distance from HST polarimetric imaging of its light echoes

P. Kervella, H. E. Bond, M. Cracraft +8

As one of the most luminous Cepheids in the Milky Way, the 41.5-day RS Puppis is an analog of the long-period Cepheids used to measure extragalactic distances. An accurate distance…

astro-ph.SR2013★ 29 cited

Evolution of the 1919 Ejecta of V605 Aquilae

Geoffrey C. Clayton, Howard E. Bond, Lindsey A. Long +7

New imaging of V605 Aql, was obtained in 2009 with HST/WFPC2, which had a nova-like outburst in 1919, and is located at the center of the planetary nebula (PN), Abell 58. This even…

astro-ph.SR2013★ 52 cited

Orbital and Evolutionary Constraints on the Planet Hosting Binary GJ 86 from the Hubble Space Telescope

J. Farihi, Howard E. Bond, P. Dufour +5

This paper presents new observations of the planet-hosting, visual binary GJ 86 (HR 637) using the Hubble Space Telescope. Ultraviolet and optical imaging with WFC3 confirms the st…

astro-ph.CO2012★ 38 cited

Stellar Populations of Lyman Break Galaxies at z=1-3 in the HST/WFC3 Early Release Science Observations

N. P. Hathi, S. H. Cohen, R. E. Ryan +24

We analyze the spectral energy distributions (SEDs) of Lyman break galaxies (LBGs) at z=1-3 selected using the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) UVIS channel…

astro-ph.SR2012★ 11 cited

The long-period Galactic Cepheid RS Puppis - II. 3D structure and mass of the nebula from VLT/FORS polarimetry

P. Kervella, A. Mérand, L. Szabados +7

The long-period Cepheid RS Pup is surrounded by a large dusty nebula reflecting the light from the central star. Due to the changing luminosity of the central source, light echoes…