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MGB thesis Chapter1
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter1.htm16 Jun 2015: An eye with an aperture of approximately 5 mm can only see detail in objects on scales larger than about 20 arc-seconds. ... The first practical example of stellar interferometry had to wait until 1921 when Michelson built a 20 foot interferometer using -
HAWAII SAM MICROCODE
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_01dec97.html16 Jun 2015: 1714 1500 2.20. 2000 and above 1714 2.35. (note intermediate rates all work. -
MGB thesis Chapter 2
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter2.htm16 Jun 2015: 20-40. Mercury Cadmium Telluride (HgCdTe). 0.25 - 0.5. 2.4 - 4.8. ... Since the devices are manufactured at room temperature but operated at 20 - 80 K, any difference in thermal expansion between the two layers can cause the device to break apart. -
CIRSI INT Observing Guide
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.ing.html16 Jun 2015: ms/rgm. 2000 May 20. first draft. 1.1. rgm. 2000 June 14. ... 19.6 Remote control is rejected. 20. Annotated sample pixel.ini file. 21. -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduct…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduction_manual16 Jun 2015: The '20' is just a convenient offset to make the night_const values come out near unity. ... It is understood to be the magnitude in a 10 arcsec diameter aperture: zmag = 20 2.5log[int_time] - corr[airmass] - night_const mag(OBJ) = zmag - 2.5log[OBJ(DN)]. -
https://people.ast.cam.ac.uk/~optics/dazle/sky-data/ukirt_sky_ramsey_e…
https://people.ast.cam.ac.uk/~optics/dazle/sky-data/ukirt_sky_ramsey_etal.dat16 Jun 2015: 1.03340 2972.72 17 1.03490 4064.29 18 1.03640 4992.76 19 1.03790 3634.36 20 1.03940 5575.10 21 1.04090 2583.35 22 ... 13410 2947.20 85 1.13560 2201.01 86 1.13710 1487.83 87 1.13860 1157.57 88 1.14000 2297.47 89 1.14150 4560.68 90 1.14300 -
Microsoft PowerPoint - Project_1640_optics
https://people.ast.cam.ac.uk/~optics/project1640/Project_1640_optics.pdf16 Jun 2015: dg. e, U. K. De. tec. tor:. full. 20. 48. x2. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html16 Jun 2015: Keep the peak counts below about 8K (you could put the telescope somewhat out of focus, eg 20 units, if necessary). ... Run Filter Chip1 Chip2 Chip3 Chip4 Comment 7614 H (?) 4300 2300 2300 4000 Filter used on Nov 19/20, 20/21 7615 Hl (?) 1200 700 600 -
MGB thesis Chapter 4
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter4.htm16 Jun 2015: Since the individual exposures would be only 10 - 20 ms, the overall observing efficiency is low. ... 7858000. 0.27. 7208000. 0.19. 3. 6214000. 0.35. 8841000. 0.20. Mean. 6.5x10. -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2…
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2001a/patt2.sty16 Jun 2015: position or quarter, }} put(01.90,20.60){{ it instrument preparation requirements, etc }} put(00.25,20.20){rule[0.0cm]{19.00cm}{@thicklinewidth}} put(00.35,19.85){{ 13 }} ... put(00.25,27.30){{ it References and Figures }} put(00.25,27.20){line(1,0){19.00
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