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NICMOS post-cooldown detector performance. 1) SMOV status 2) Dark current 3) Quantum efficiency 4) “First light”, focus and image quality 5) SMOV outlook. Thermal history since NICMOS switch-on (on April 19). Transition to detector control. Transition to Ne control. Setpoint to 72.5 K.
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NICMOS post-cooldown detector performance 1) SMOV status 2) Dark current 3) Quantum efficiency 4) “First light”, focus and image quality 5) SMOV outlook
Thermal history since NICMOS switch-on (on April 19) Transition to detector control Transition to Ne control Setpoint to 72.5 K Setpoint to 72 K
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Filter wheel test(G. Schneider, K. Noll, L. Mazzuca, E. Roberts) • NICMOS filter wheels have motion sensor only on the motors, not on the wheels themselves • Concern about breaking the wheel shaft in case of mechanical contact/blockage • careful “two step forward, one step back” approach with analysis of motor currents and flat field images • so far, so good: verified normal motion over 9/10 of a full turn • side benefit: early measurement of DQE (and more….)
Mean: 0.166 e-/s Mean: 0.114 e-/s Mean: 0.148 e-/s • NICMOS dark current • (C. Xu) • preliminary measurements indicate that dark current is nominal, i.e. close to Cycle 7 • “bump” is NOT observed
The first flat field images Then… (1998, T=62 K) Now… (2002, T= 77K) NIC1 NIC2 NIC3
Serendipitous image of a crowded star field (…taken out from electronic distribution as requested by HST project…) Camera 2 in H-band (F160W) FWHM: 2.17 pixels (0.163“) (very close to nominal!)
First assessment of image quality: (G. Schneider) • VERY close to nominal focus • some coma, to be corrected with tilt adjustment of PAM (in time for ERO observations) Mean PSF from 2002 stellar field (NIC1, F095N) 1997 PAM tilt grid (NIC1, F095N)
Summary - NICMOS has survived its 28 month hiatus without any significant degradation - performance is nominal so far - GO science will be enabled within 2 weeks