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  2. Specific Parameters for OCLI CH4 Filters Thickness: 1.0 mm. ...

    https://people.ast.cam.ac.uk/~optics/cirsi/technical/methane.htm
    16 Jun 2015: 1650.4. 1740.5. Long 6. 1652.2. 1741.9. Note: OCLI performed tests on a witness piece at 77 K and calculated the values for the filters themselves.
  3. Project Reassessment Start Date

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/webreview.htm
    16 Jun 2015: The evolutionary history of galaxy clusters offers a sensitive test of current theories for the origin of structure (White et al 1994). ... A test dewar is being constructed to operate a single chip, this uses an existing Oxford Instruments MN1815 dewar
  4. CIRPASS at Gemini-S Diary

    https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/Gemini-S/diary.html
    16 Jun 2015: The freezer enclosure is put together empty to prepare for a cool-down test. ... The test indicates the light-proofing is good. We are told we have to evacuate the site at 1530 so we have to stop doing tests and prepare to leave.
  5. CIRPASS assemblies May02

    https://people.ast.cam.ac.uk/~optics/cirpass/srm/CIRPASS%20assemblies%20May02.htm
    16 Jun 2015: The Test Telescope. Note the black flexible conduit trailing on the floor.
  6. MGB thesis Chapter 3

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm
    16 Jun 2015: This technique, however, is very time consuming since it requires 100 times as many exposures as the same test for a CCD. ... In tests, the relationship is slightly different as shown by the plot in Figure 3.15.
  7. New Page 1

    https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm
    16 Jun 2015: The tests carried out produced images with better resolution from the ground than have been obtained in space with the Hubble Space Telescope, and reached nearly 1000 times fainter than was
  8. 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: dome flats done in the recommended way test! focus, junk, random frames sky! ... Only 'astro', 'standard', 'test' and 'sky' OBSTYPE frames will be combined, chip-by-chip.
  9. HAWAII SAM MICROCODE

    https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_01dec97.html
    16 Jun 2015: version of PixCel used for these tests. Different initialisation files. There are a number of initialisation files (.ini) files available.
  10. 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: OBSTYPE string One of OBJECT,ARC,FOCUS,TEST,DARK,DOMEDARK,DOMEFLAT, or TWILIGHT as set on the control GUI. ... band filter 8 H1.573 narrow band (1% bandwidth) filter, aka Hn or H_OH 21 Nov 1999 Domeflat filter test: Lamp meter = 220 Exposure time = 10
  11. HAWAII SAM MICROCODE

    https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_doc_27may98.html
    16 Jun 2015: Note that all these gain figures need to be established with the actual device in use by a method such as the variance test. ... version of PixCel used for these tests. Note: The latest IR version of PixCel allows mode switching between modes 4 and 8
  12. Observations with CIRPASS in Cambridge

    https://people.ast.cam.ac.uk/~optics/cirpass/Observing/15jan2002.html
    16 Jun 2015: CIRPASS test observations - 15th Jan 2002. This was the first night the 8-inch Celestron (affectionately dubbed the "Jiminy Telescope" due to its small size) was operated on the night sky.
  13. Project Reassessment Start Date

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc
    16 Jun 2015: 6.2.28 Multiplexor Electrical tests GOTOBUTTON _Toc361307210 PAGEREF _Toc361307210 34. 6.2.29 Install engineering grade detector and test GOTOBUTTON _Toc361307211 PAGEREF _Toc361307211 34. ... 6.2.35 Tests with 4100 standard system GOTOBUTTON
  14. Appendix XXX

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc
    16 Jun 2015: V0 CLOSE_SH BLANK FIELD LINE WR_CTRL] JUMP MODE_SELECT;. %----------------------------. | |. | TEST ADDRESS ZERO FOR MODE |. | |. ----------------------------%. MODE_SELECT:. ... binning is required. Routine must be called with ADDR_19 set%. EPR3_TEST:. %
  15. /astro/p7scch2/AUMic/paper/figures/all.eps

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 Jun 2015: From tests with ahandful of selected dust materials, we derive a preferencefor mixtures of silicate, carbon, and ice of moderate porosity.
  16. arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf
    8 Jan 2015: This reference model in-cludes dust interior to the habitable zone all the way into the sublimation radius, so this model may test howclose-in dust such as that detected in
  17. Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 Nov 2015: Accepted to ApJ: October 28, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. YOUNG “DIPPER” STARS IN UPPER SCO AND ρ OPH OBSERVED BY K2. M. Ansdell1,10, E. Gaidos2,3,4,10, S. A. Rappaport5, T. L. Jacobs6, D. M. LaCourse6, K. J. Jek6
  18. arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: Thus, the limit on CO gas is not stringentenough to test different scenarios for the production of gasbyplanetesimal collisions. ... 4. We now consider the location of dustdetected with near-IR interferometry, and then turn to a moredetailed
  19. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/blrf15.pdf
    14 Sep 2015: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 14 September 2015 (MN LATEX style file v2.2). Planet Hunters X.KIC 8462852 – Where’s the flux? †. T. S. Boyajian1, D. M. LaCourse2, S. A. Rappaport3,D. Fabrycky4, D. A. Fischer1, D.
  20. arX iv:1 501. 0318 1v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/asgw15.pdf
    15 Jan 2015: bowed (Milli et al. 2014). We test evidence for the overall bow in our data by independently.
  21. Next Generation Very Large Array Memo No. 6Science Working ...

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: the star-forming gas reservoirs within and beyond the CND(e.g., Liu et al., 2012)—such as peculiar objects like the G2 cloud (Gillessenet al., 2012)—to test scenarios of

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