112 citations · 112 across the 2 of their papers we have counts for
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CalFUSE v3: A Data-Reduction Pipeline for the Far Ultraviolet Spectroscopic Explorer
W. V. Dixon, D. J. Sahnow, P. E. Barrett +13
Since its launch in 1999, the Far Ultraviolet Spectroscopic Explorer (FUSE) has made over 4600 observations of some 2500 individual targets. The data are reduced by the Principal I…
Star Formation in NGC5194 (M51a): The Panchromatic View from GALEX to Spitzer
D. Calzetti, R. C. Kennicutt, L. Bianchi +32
(Abridged) Far ultraviolet to far infrared images of the nearby galaxy NGC5194, from Spitzer, GALEX, Hubble Space Telescope and ground--based data, are used to investigate local an…
The Near-UV Pulse Profile and Spectrum of the Pulsar PSR B0656+14
Yu. A. Shibanov, J. Sollerman, P. Lundqvist +2
We have observed the middle-aged pulsar PSR B0656+14 with the prism and the NUV MAMA detector of the Space Telescope Imaging Spectrograph (STIS) to measure the pulsar spectrum and…
Limits on the Optical Brightness of the Epsilon Eridani Dust Ring
Charles Proffitt, Kailash Sahu, Mario Livio +10
The STIS/CCD camera on the {\em Hubble Space Telescope (HST)} was used to take deep optical images near the K2V main-sequence star Eridani in an attempt to find an optical coun…
Terminal velocities of luminous, early-type SMC stars
C. J. Evans, D. J. Lennon, C. Trundle +2
Ultraviolet spectra from the Space Telescope Imaging Spectrograph (STIS) are used to determine terminal velocities for 11 O and B-type giants and supergiants in the Small Magellani…
Calibration of Geometric Distortion in the ACS Detectors
G. R. Meurer, D. Lindler, J. P. Blakeslee +9
The off-axis location of the Advanced Camera for Surveys (ACS) is the chief (but not sole) cause of strong geometric distortion in all detectors: the Wide Field Camera (WFC), High…