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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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