The World Space Observatory for UltraViolet Project WSO-UV Isabella Pagano, Martin Barstow, Noah Brosch, Ana Ines Gómez de Castro, Mahoai Huang, Norbert Kappelmann,…
Dichroic Beamsplitters M.Lampton UCB SSL Dec 2003 M.Lampton Dec 2003 Why a dichroic beamsplitter? Separating the VIS and NIR sensors could double our observing efficiency!…
Making MOPRA go! Lucyna Kedziora-Chudczer Friend of the telescope (UNSW) MOPRA at mm wavelengths 22-m diameter telescope Location: 20 km from Coonabarabran (NSW) Altitude…
Making MOPRA go! Lucyna Kedziora-Chudczer Friend of the telescope (UNSW) MOPRA at mm wavelengths 22-m diameter telescope Location: 20 km from Coonabarabran (NSW) Altitude…
Bulk Silicon CCDs, Point Spread Functions, and Photon Transfer Curves: CCD Testing Activities at ESO Mark Downing, Dietrich Baade, Sebastian Deiries, (ESO/Instrumentation…
Bulk Silicon CCDs, Point Spread Functions, and Photon Transfer Curves: CCD Testing Activities at ESO Mark Downing, Dietrich Baade, Sebastian Deiries, (ESO/Instrumentation…
LGS at the LBT- A Road Map to GLAO and Upgrades Sebastian Rabien Science cases from this morning Laird: Deep fields, faint targets The ‘20% seeing case’ Big field of…
Bulk Silicon CCDs, Point Spread Functions, and Photon Transfer Curves: CCD Testing Activities at ESO Mark Downing, Dietrich Baade, Sebastian Deiries, (ESO/Instrumentation…