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DAZLE – the design Introduction DAZLE, the Dark Ages ...
https://people.ast.cam.ac.uk/~optics/dazle/info/DAZLE%20design%20concept.htm16 Jun 2015: The AAO selected a suitable bearing (originally intended for use with a radar tracker!) and conducted tests to verify that the axial runout specification is met by this precision bearing. ... At the IoA we have carried out stability tests of the complete -
Specific Parameters for OCLI CH4 Filters Thickness: 1.0 mm. ...
https://people.ast.cam.ac.uk/~optics/cirsi/technical/methane.htm16 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. -
CIRPASS at Gemini-S Diary
https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/Gemini-S/diary.html16 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. -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/webreview.htm16 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 -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html16 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 -
CIRPASS assemblies May02
https://people.ast.cam.ac.uk/~optics/cirpass/srm/CIRPASS%20assemblies%20May02.htm16 Jun 2015: The Test Telescope. Note the black flexible conduit trailing on the floor. -
MGB thesis Chapter 3
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm16 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. -
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: 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. -
New Page 1
https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm16 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 -
HAWAII SAM MICROCODE
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_01dec97.html16 Jun 2015: version of PixCel used for these tests. Different initialisation files. There are a number of initialisation files (.ini) files available. -
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: 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 -
HAWAII SAM MICROCODE
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_doc_27may98.html16 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 -
Observations with CIRPASS in Cambridge
https://people.ast.cam.ac.uk/~optics/cirpass/Observing/15jan2002.html16 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. -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc16 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 -
arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf25 Nov 2015: In Section 5, we test the spatial scale and dust propertiesagainst bow wave models to break the SED degeneracy and deter-mine which mechanism is more likely. ... The PSF reference star can be scaled to the peakemission and subtracted from the data images -
Appendix XXX
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc16 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:. % -
/astro/p7scch2/AUMic/paper/figures/all.eps
https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf16 Jun 2015: From tests with ahandful of selected dust materials, we derive a preferencefor mixtures of silicate, carbon, and ice of moderate porosity. -
arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf8 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 -
Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...
https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf2 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 -
arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf10 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
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