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The top documents tagged [sky coverage]

T L O Action: The student will interpret the information contained in a surface analysis chart. Condition: Given pertinent information about surface
T L O Action: The student will interpret the information contained in a surface analysis chart. Condition: Given pertinent information about surface
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Dealing with turbulence in MCAO Roberto Ragazzoni INAF – Padova (Italy) Alghero, Sept. 17 th 2008 Astronomy meets Metereology Dealing with turbulence in
Dealing with turbulence in MCAO Roberto Ragazzoni INAF – Padova (Italy) Alghero, Sept. 17 th 2008 Astronomy meets Metereology Dealing with turbulence in
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TMT.AOS.PRE.10.054.REL01 1 Brent Ellerbroek TMT Instrumentation @ SPIE 2010 San Diego, June 26, 2010. TMT Early Light Adaptive Optics
TMT.AOS.PRE.10.054.REL01 1 Brent Ellerbroek TMT Instrumentation @ SPIE 2010 San Diego, June 26, 2010. TMT Early Light Adaptive Optics
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5xmorales marquez
5xmorales marquez
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GLAO Workshop, Leiden; April 26 th 2005 Ground Layer Adaptive Optics, N. Hubin Ground Layer Adaptive Optics Status and strategy at ESO Norbert Hubin European
GLAO Workshop, Leiden; April 26 th 2005 Ground Layer Adaptive Optics, N. Hubin Ground Layer Adaptive Optics Status and strategy at ESO Norbert Hubin European
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Xiaohu Yang Shanghai Astronomical Observatory Partner group of MPA Collaborators: Yu Wang (SHAO), H.J. Mo (UMass), F.C. van den Bosch (MPIA), Neal Katz
Xiaohu Yang Shanghai Astronomical Observatory Partner group of MPA Collaborators: Yu Wang (SHAO), H.J. Mo (UMass), F.C. van den Bosch (MPIA), Neal Katz
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Thomas Stalcup June 15, 2006 Laser Guidestar System Status
Thomas Stalcup June 15, 2006 Laser Guidestar System Status
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Gino Tosti – INFN Perugia1DC2 Closeout Meeting - GSFC May 31 –June 2, 2006 Source Detection with the Perugia Wavelet code (PGWave) Gamma-ray Large Area
Gino Tosti – INFN Perugia1DC2 Closeout Meeting - GSFC May 31 –June 2, 2006 Source Detection with the Perugia Wavelet code (PGWave) Gamma-ray Large Area
224 views
Ralf Siebenmorgen IR instrument from Antarctica (thermal) IR instruments from Antarctica: what can be gained Ralf Siebenmorgen Why? pwv, T, aerosols
Ralf Siebenmorgen IR instrument from Antarctica (thermal) IR instruments from Antarctica: what can be gained Ralf Siebenmorgen Why? pwv, T, aerosols
214 views
NEA Follow-up Characterization Needs and Issues: Radar and Optical Lance Benner Jet Propulsion Laboratory California Institute of Technology
NEA Follow-up Characterization Needs and Issues: Radar and Optical Lance Benner Jet Propulsion Laboratory California Institute of Technology
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SETI@Arecibo Jim Cordes and Dan Werthimer And Five Milliion SETI@home Volunteers in 226 countries ://seti.berkeley.edu http:
SETI@Arecibo Jim Cordes and Dan Werthimer And Five Milliion SETI@home Volunteers in 226 countries ://seti.berkeley.edu http:
215 views
ACBAR Chao-Lin Kuo Stanford Physics/SLAC. K2K2 CMB power spectrum, as of 03/04/08
ACBAR Chao-Lin Kuo Stanford Physics/SLAC. K2K2 CMB power spectrum, as of 03/04/08
219 views