activity
19972008
most citedThe HST Key Project on the Extragalactic Distance Scale. XXVIII. Combining the Constraints on the Hubble Constant

550 citations · 2.3k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph2008★ 82 cited

The Variable Stars of the Draco Dwarf Spheroidal Galaxy - Revisited

K. Kinemuchi, H. C. Harris, Horace A. Smith +4

We present a CCD survey of variable stars in the Draco dwarf spheroidal galaxy. This survey, which has the largest areal coverage since the original variable star survey by Baade &…

astro-ph2003★ 157 cited

Infrared Emission of Normal Galaxies from 2.5 to 12 Microns: ISO Spectra, Near-Infrared Continuum and Mid-Infrared Emission Features

Nanyao Lu, George Helou, Michael W. Werner +6

We present ISO-PHOT spectra of the regions 2.5-4.9um and 5.8-11.6um for a sample of 45 disk galaxies from the U.S. ISO Key Project on Normal Galaxies. The spectra can be decomposed…

astro-ph2002

RR Lyrae Stars and Anomalous Cepheids in the Draco Dwarf Spheroidal Galaxy

K. Kinemuchi, H. A. Smith, A. LaCluyze +4

We present new results on RR Lyrae stars and anomalous Cepheids in the Draco dwarf spheroidal galaxy. We have increased the number of double-mode RR Lyrae stars and found three new…

astro-ph2002★ 25 cited

B,V Photometry of Variable Stars in the Northeast Arm of the Small Magellanic Cloud

Brian Sharpee, Michele Stark, Barton Pritzl +4

B and V photometry has been obtained for variable stars in the northeast arm of the Small Magellanic Cloud (SMC). Periods and lightcurves have been determined for 237 periodic vari…

astro-ph2000★ 87 cited

The Interstellar Medium of Star-forming Irregular Galaxies: The View with ISO

D. Hunter, M. Kaufman, D. Hollenbach +8

We present mid-infrared imaging and far-infrared (FIR) spectroscopy of 5 IBm galaxies observed by ISO as part of our larger study of the inter- stellar medium of galaxies. Most of…

astro-ph2000

Type Ia Supernovae and the Value of the Hubble Constant

Brad K. Gibson, Chris B. Brook

The methodology involved in deriving the Hubble Constant via the calibration of the corrected peak luminosities of Type Ia supernovae (SNe) is reviewed. We first present a re-analy…