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81 - 100 of 109 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 109 match some words.

  1. Results that match 1 of 2 words

  2. Rockwell PICNIC array

    https://people.ast.cam.ac.uk/~optics/tech/hawaii/picnic.htm
    16 Jun 2015: system. The read noise is likely to be lower, <10 electrons are expected for the HAWAII device rather than 15-20 electrons for NICMOS.

  3. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/oh_lines_xy.txt

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/oh_lines_xy.txt
    16 Jun 2015: 0.0 12726.1 20 12726.1 0.0 12744.6 0.0 12744.6 24 12744.6 0.0 12749.3 0.0 12749.3 45 12749.3 0.0 ... 1 11 15084.1 0.0 15183.0 0.0 15183.0 20 15183.0 0.0 15236.8 0.0 15236.8 90 15236.8 0.0 15283.6

  4. MGB thesis Chapter1

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter1.htm
    16 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

  5. HAWAII SAM MICROCODE

    https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_01dec97.html
    16 Jun 2015: 1714 1500 2.20. 2000 and above 1714 2.35. (note intermediate rates all work.

  6. New Page 1

    https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm
    16 Jun 2015: General Lecturing:. Given a very great number of lectures including seminars, conference reviews and paper presentations, popular lectures, including (for >20 years) talking to groups of local schoolchildren on general astronomy. ... Ph.D Awarded:

  7. MGB thesis Chapter 2

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter2.htm
    16 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.

  8. CIRSI INT Observing Guide

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.ing.html
    16 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.

  9. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduct…

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduction_manual
    16 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)].

  10. 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.dat
    16 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

  11. Microsoft PowerPoint - Project_1640_optics

    https://people.ast.cam.ac.uk/~optics/project1640/Project_1640_optics.pdf
    16 Jun 2015: dg. e, U. K. De. tec. tor:. full. 20. 48. x2.

  12. MGB thesis Chapter 4

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter4.htm
    16 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.

  13. 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.sty
    16 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

  14. MGB thesis Chapter 3

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm
    16 Jun 2015: Results. The read noise of the COAST camera at 20 kHz pixel rate, assuming a gain of 450 e. -.

  15. Craig  Mackay

    https://people.ast.cam.ac.uk/~optics/people/cdm_pub_list_130509.htm
    16 Jun 2015: SPIE, 290, 159 (1981). 20. Wright, J.F. and Mackay, C.D., The Cambridge Charge--Coupled Device (CCD) System'. ... Optical aperture synthesis on the INT. Gemini, Newsletter of RGO, No 20, 2.

  16. 3CD8ACD5-01E7-18B8

    https://people.ast.cam.ac.uk/~optics/dazle/info/science.pdf
    16 Jun 2015: In the near IR, the broad band sky is 20-50 times brighter than in the optical - e.g. ... Therefore, at worst, it will take 20 nights of 8 m time to detect a sample of 10 or more galaxies and at best we shall detect many hundreds which would

  17. This is the text of the SAM microcode that ...

    https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_code_27may98.html
    16 Jun 2015: 20/5/97 4.06: As 4.05 but with all vfg pulses etc removed NOTE: Pixcel.ini also modified, for 0,0 in PDCI section 22/5/97 4.07: ... 20/6/97 4.14: Lengthen reset pulses to 2.1 microsecs each 2/7/97 4.15: Install chip/quadrant select.

  18. Project Reassessment Start Date

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/webreview.htm
    16 Jun 2015: 2-3 magnitudes fainter i.e. H=20 would be in the right ball park. ... Short wavelength cut-on (micron) 0.85 0.85. Read noise (e- at 77K) < 20 < 5.

  19. arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf
    8 Jan 2015: Wyatt et al. 2007; Gáspár et al. 2013).While 20% of nearby stars have cold, i.e. ... We find that a 50 star survey can measure Z10with 20% accuracy (for Z100.3-0.4).

  20. Mon. Not. R. Astron. Soc. 000, 1–11 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pwk15.pdf
    9 Feb 2015: Uniform log10(z), log10(z). i / 0 20 40 60 80. Figure 4. ... 0.950.90.8. 0.7. e. 80. 7560. 40. 20. i /. 0. 270.

  21. arX iv:1 501. 0414 4v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dhsk15.pdf
    20 Jan 2015: 20 times brighter than the Solar zodiacal cloud assuming a smooth brightness distribution. ... 2011; Mennesson et al. in press). One of their analyses focused on a sample of 20 solar-type.

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