activity
20062018
most citedThe SPEAR Instrument and On-Orbit Performance

63 citations · 258 across the 13 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 7 cited

Idling Magnetic White Dwarf in the Synchronizing Polar BY Cam. The Noah-2 Project

Ivan L. Andronov, Kirill A. Antoniuk, Vitalii V. Breus +8

Results of a multi-color study of the variability of the magnetic cataclysmic variable BY Cam are presented. The observations were obtained at the Korean 1.8m and Ukrainian 2.6m, 1…

astro-ph2006★ 23 cited

SPEAR Far Ultraviolet Spectral Images of the Cygnus Loop

Kwang-Il Seon, Wonyong Han, Uk-Won Nam +7

We present far-ultraviolet (FUV) spectral images, measured at C IV 1550, He II 1640, Si IV+O IV] 1400, and O III] 1664, of the entire Cygnus Loop, observed with the Spectroscopy of…

astro-ph2006★ 21 cited

Molecular Hydrogen Fluorescence in the Eridanus Superbubble

K. Ryu, K. W. Min, J. W. Park +8

The first FUV (lambda lambda 1350-1750 A) spectral imaging observations of the Eridanus superbubble, obtained with the SPEAR/FIMS mission, have revealed distinct fluorescent emissi…

astro-ph2006★ 63 cited

The SPEAR Instrument and On-Orbit Performance

Jerry Edelstein, Eric Korpela, Joe Adolfo +21

The SPEAR (or 'FIMS') instrumentation has been used to conduct the first large-scale spectral mapping of diffuse cosmic far ultraviolet (FUV, 900-1750 AA) emission, including impor…

astro-ph2006★ 62 cited

The Spectroscopy of Plasma Evolution from Astrophysical Radiation Mission

J. Edelstein, K. W. Min, W. Han +18

The Spectroscopy of Plasma Evolution from Astrophysical Radiation (or the Far-ultraviolet Imaging Spectrograph) instruments, flown aboard the STSAT-1 satellite mission, have provid…

astro-ph2006★ 20 cited

Far-ultraviolet Observations of the North Ecliptic Pole with SPEAR

Eric J. Korpela, Jerry Edelstein, Julia Kregenow +7

We present SPEAR/FIMS far-ultraviolet observations near the North Ecliptic Pole. This area, at b~30 degrees and with intermediate HI column, seems to be a fairly typical line of si…