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1 - 30 of 30 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 30 match some words.

  1. Results that match 1 of 2 words

  2. Other NIR spectrographs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_nirspec.html
    16 Jun 2015: ISAAC (LW). 8m VLT UT1. 2-5. 1500,700,450,200 (lres). 8000,4000,2500,1250 (mres). 41.5.

  3. MGB thesis Chapter 5

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter5.htm
    16 Jun 2015: The trolley is set to scan at 200 Hz and forms the main peak in the data.

  4. Other IFUs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html
    16 Jun 2015: software. PIFS. type. slicer. telescope. Palomar 200 inch. wv range. 1-2.5 micron, 1-5 micron.

  5. https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt
    16 Jun 2015: 13. -5. 199. 200. 12. -4. 200. 201. 11. -3. 201.

  6. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html
    16 Jun 2015: pc, computer room 200.29.61.153 bodega2.lco.cl bodega2 # Yerko Aviles pc # 200.29.61.154? ... 139 remote.lco.cl remote # # Visitor Laptops # 200.28.111.145 visitor1.lco.cl visitor1 200.28.111.146 visitor2.lco.cl visitor2 17).

  7. CIRSI LCO 100" Observing Notes - 1999 April/May

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/cirsi_lco_notes_1999may.html
    16 Jun 2015: Cannot connect to 200.28.111.133. This probable means that you started the NT-Camera Control before you startup up Pixcel on CIRCC.

  8. CIRSI INT Observing Guide

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.ing.html
    16 Jun 2015: PLUS_5=5.300. MINUS_5=-5.400. ANALOGUE_IN=-0.30. VOUT_D=5.200. VOUT_C=5.200. VOUT_B=1.100. VOUT_A=1.300. ... 5.200. PLUS_25=23.400. PLUS_12=12.300. MINUS_12=-11.000.

  9. design study report

    https://people.ast.cam.ac.uk/~optics/cirpass/design-study-a.htm
    16 Jun 2015: A peak throughput of 20-24% is achievable. A Baranne spectrograph design with 0.19m of wavelength coverage and a multiplex gain of 200 (50 per spectrograph) looks feasible technically but ... A fully specified classical spectrograph with a wavelength

  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: 196 1.29700 3408.63 197 1.29850 3794.42 198 1.29990 4543.59 199 1.30140 4584.77 200 1.30280 4085.07 201 1.30420 3724.87 202 ... 75750 202.051 199 1.75880 511.795 200 1.76010 1403.21 201 1.76140 4458.84 202 1.76270 12575.5 203 1.76400 13281.0 204 1.76530

  11. Chapter 4 - Controls Reference

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter4.htm
    16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  12. Chapter 2 - Operating the software

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm
    16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  13. MGB thesis Chapter 2

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter2.htm
    16 Jun 2015: 1.05. 150 - 300. Indium Gallium Arsenide (InGaAs). 0.7. 1.7. 77 - 200.

  14. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/blrf15.pdf
    14 Sep 2015: There are modulations in the raw flux data at the 200 ppmlevel which are visible by eye. ... 5. Time (BJD-2454833). No. rma. lize. d f. lux. 190 200 210 220 230 240.

  15. 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: It is approximately the size of one chip, i.e., 200 arcsec on a side.

  16. MGB thesis Chapter 3

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm
    16 Jun 2015: [Chapter 3: Camera. Outline. This chapter describes the near infrared camera built for COAST. It examines the properties required from the camera system, the range of devices available and the factors involved in the choice of detector. The design,

  17. Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: A /. yr-1. 108. 106. 104. 102. 100. a / au0 50 100 150 200. ... 0.2. 0.4. 0.6. 0.8. r / au0 50 100 150 200.

  18. MGB thesis Chapter 4

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter4.htm
    16 Jun 2015: The exposure times were 50, 100 and 200 milli-seconds. Results. Signal (e. -.

  19. arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: for material uniformlydistributed around a circular narrow ring at 200 au, with thein-clination derived from the 70µm PACS image. ... models the inner edge is around 30 au, and theouter edge around 200 au.

  20. Draft version May 29, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf
    14 Sep 2015: System temperature values 100 to 200 Khigher were recorded on June 4. ... Werepeat this procedure 200 times before taking statistics. Fig. 6 summarizes the result of these Monte-Carlo sim-ulations.

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

    https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf
    8 Jan 2015: SB (SBC7), but not in SB9, also VB, 5”HD 82885 SV Lmi G8III VB 3.8”, 43 AU, P=200 yrHD 95735 M2V EBHD 98231 GJ 423A G0V Complicated multiple

  22. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 Jan 2015: 140. 160. 180. 200. 220. 240. 260. 0 105 2x10. 5 3x10. ... 5. Angle. Time (yrs). 100. 120. 140. 160. 180. 200. 220.

  23. Next Generation Very Large Array Memo No. 6Science Working ...

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: The region inside the first gap is optically thick (T > 200 K); additionalouter rings may be optically thick as well. ... These objects (see Figure 2) arepresumably in the latest phase of accretion in the formation of stars moremassive than 10 or 20 M

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

    https://people.ast.cam.ac.uk/~wyatt/dhsk15.pdf
    20 Jan 2015: 11 –. 0 100 200 300 400 500 600 700Photometric aperture radius [mas].

  25. MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rw15.pdf
    17 Dec 2015: MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled using MNRAS LATEX style file v3.0. Dynamical Constraints on Outer Planets in Super-Earth Systems. Matthew J. Read1? and Mark C. Wyatt11Institute of Astronomy, University of Cambridge,

  26. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/Rousellot_list_v2.…

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/Rousellot_list_v2.0.dat
    16 Jun 2015: 1.758e-08 8141.200 2.949e-01 8141.502 2.949e-01 8141.831 7.771e-03 8142.440 7.771e-03 8144.889 2.110e-07 8145.328 ... 294 4.656e01 9444.336 1.324e-01 9444.342 1.324e-01 9444.858 2.932e-04 9445.978 2.932e-04 9449.923 9.369e-01 9450.200

  27. arX iv:1 501. 0318 1v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/asgw15.pdf
    15 Jan 2015: unfiltered STIS observations (200-1,050 Å) and the filtered F606W ACS images. ... 24 –. Disk Spine Position: Observations and Models. -200 -100 0 100 200Distance [au].

  28. arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 Nov 2015: arX. iv:1. 511. 0591. 9v1. [ast. ro-p. h.E. P]. 18 N. ov 2. 015. Mon. Not. R. Astron. Soc.000, 1–18 (2002) Printed 19 November 2015 (MN LATEX style file v2.2). IR-excesses around nearby Lambda Boo stars are caused by debrisdisks rather than ISM

  29. Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 Nov 2015: Some young (10–200 Myr)debris disks have also shown mid-IR variability on similarscales, interpreted as debris from planetesimal collisions(e.g., Melis et al.

  30. /astro/p7scch2/AUMic/paper/figures/all.eps

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 Jun 2015: m1,e1,p1 4.2M3 1.5 103 100 0.05. M4 1.4 103 200 0.05.

  31. Draft version January 19, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf
    19 Jan 2015: 0.090.14. 7 7 2/10 0.200.070.17 3/11 0.27. 0.090.16. 8 1y 7/48 0.150.040.07 7/48 0.15. ... 0.100.15. 19 7o 2/10 0.200.070.17 3/11 0.27. 0.090.16. a Unconfirmed planetary systems are HD 22049 ( Eri), HD 10700 (τ Cet) andHD

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