activity
20092016
most citedThe Cosmic Origins Spectrograph: On-Orbit Instrument Performance

112 citations · 281 across the 5 of their papers we have counts for

collaborators

5 papers

physics.ins-det2016★ 49 cited

A Brief Technical History of the Large-Area Picosecond Photodetector (LAPPD) Collaboration

Bernhard W. Adams, Klaus Attenkofer, Mircea Bogdan +38

The Large Area Picosecond PhotoDetector (LAPPD) Collaboration was formed in 2009 to develop large-area photodetectors capable of time resolutions measured in pico-seconds, with acc…

astro-ph.SR2011★ 85 cited

Possible detection of two giant extrasolar planets orbiting the eclipsing polar UZ Fornacis

Stephen B. Potter, Encarni Romero--Colmenero, Gavin Ramsay +11

We present new high-speed, multi-observatory, multi-instrument photometry of the eclipsing polar UZ For in order to measure precise mid-eclipse times with the aim of detecting any…

astro-ph.IM2010★ 112 cited

The Cosmic Origins Spectrograph: On-Orbit Instrument Performance

S. Osterman, J. Green, C. Froning +31

The Cosmic Origins Spectrograph (COS) was installed in the Hubble Space Telescope in May, 2009 as part of Servicing Mission 4 to provide high sensitivity, medium and low resolution…

astro-ph.IM2010

Observing with HST below 1150Å: Extending the Cosmic Origins Spectrograph Coverage to 900Å

Steve Osterman, Steven V. Penton, Kevin France +4

The far-ultraviolet (FUV) channel of the Cosmic Origins Spectrograph (COS) is designed to operate between 1130Å and 1850Å, limited at shorter wavelengths by the reflectivity of the…

astro-ph.IM2009★ 35 cited

Far-UV sensitivity of the Cosmic Origins Spectrograph

Stephan R. McCandliss, Kevin France, Steven Osterman +3

We demonstrate that the G140L segment B channel of the Cosmic Origins Spectrograph (COS) recently installed on the {\it Hubble Space Telescope (HST)} has an effective area consiste…