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MagIC Upgrade for High-Speed Photometry

MagIC Upgrade for High-Speed Photometry. Jim Elliot, MIT Magellan SAC 2007-05-20. MagIC SUMMARY. CCD filter photometer for Baade (moved to Clay) Detector s 2k x 2k SITe (24 µm pixels; 2.3 x 2.3 arcmin field) 2k x 4k Lincoln Lab red and blue (13 µm pixels; 1.2 x 1.2 arcmin field) Modes

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MagIC Upgrade for High-Speed Photometry

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  1. MagIC Upgrade forHigh-Speed Photometry Jim Elliot, MIT Magellan SAC 2007-05-20

  2. MagIC SUMMARY • CCD filter photometer for Baade (moved to Clay) • Detectors • 2k x 2k SITe (24 µm pixels; 2.3 x 2.3 arcmin field) • 2k x 4k Lincoln Lab red and blue (13 µm pixels; 1.2 x 1.2 arcmin field) • Modes • Full frame, dual, and quad readout (~23 sec) • Pixel binning • High-speed (with frame transfer) • 16 filter positions • Instantly accessible • always in standby mode on a folded port • accessible by rotation of tertiary mirror (within a few minutes) • Built by MIT and CfA (installed on Baade, March 2001) • Supported by NSF (MRI), gift to Harvard from Sackler, MIT internal funds • Science programs • Narrow field imaging: gravitational lenses, compact objects, gamma-ray bursts, etc. • High-speed imaging: stellar occultations, compact objects , planetary transits

  3. WHY UPGRADE MagIC? • MagIC original design included two frame transfer CCDs • Foundry run failed ($38K lost) • POETS (Portable Occultation, Eclipse, and Transit System) • Six systems built by MIT and Williams College (spring 2005) • On Clay in July 2005, June 2006, and June 2007 • Planetary transits, stellar occultations, and speckle imaging • How to have permanent high-speed capability on Magellan? • 1. Guiders • 2. POETS piggy back on MagIC • 3. Frame transfer CCD in MagIC dewar (according to original plan) Solution: #3 Clone the hardware and software for HIPO, Ted Dunham's SOFIA instrument

  4. PERSONNEL • Key Players • Jim Elliot (P.I.) • Steve Kissel (CCD wiring and testing) • Folkers Rojas (mechanical work) • Grad student (software) • Auxiliary Players • Kenton Phillips (computer) • Brian Taylor (BU; software consultant for LOIS) • Bill Mayer (MKI oversight) • Ed Boughan, Mark Bautz (consultants)

  5. guider telescope spacer rotator camera filter wheel MAGIC MODULES

  6. FILTER WHEEL (CfA) • Based on MEGACAM design • Filter format : 4" square • 18 positions => 16 filters • Filters: • Johnson-Cousins, B,V,R,I • Sloan: u', g', r', i', z' • VR • 6 visitor filters

  7. MagIC FOCAL PLANE unvignetted region Frame transfer region masked CCD #2 CCD #1 Frame transfer region masked CCD #3 #1: SITe CCD: 4 readouts, each 50 Kpix/sec => ~25 seconds #2: CCD47-20: 2 readout, each up to 400 Kpix/sec (up to 50 Hz) #3: open (for possible CCD in the future)

  8. 100 Quantum Efficiency (%) 50 0 400 600 800 1000 Wavelength (nm) QUANTUM EFFICIENCY MagIC CCDs e2v CCD47-20 SiTe MagIC Upgrade 75 25

  9. Cooling control Sun Computer #1 LOIS #1 Electronics #1 SITe Shutter Filter Wheel Electronics #2 PC-104 Sun Computer #2 LOIS #2 e2v Dewar (cooled by CryoTiger) SCHEMATIC DIAGRAM

  10. SCHEDULE • Completed • In hand: CCDs, Leach electronics, control computer (Sun), dewar shell • Design for dewar modifications • In progress • Software installation • CCD wiring and testing • June 2007: Ship MagIC dewar, electronics, and computer from LCO to MIT • July 2007: • Modify dewar to hold two CCDs • Install the CCDs • Test • August 1, 2007: • Ship MagIC parts to Chile • August 15, 2007: • Reassemble MagIC and test at LCO • August 24 (or 28) • Engineering run

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