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16 Jun 2015: Reset-subtraction test 21 Dec 1999 Test to determine if online processing done by PixCel (reset correction, rotate, and assembly) is working correctly. ... This is our standard observing mode. RRR mode assemble ON rotate ON subtract ON Test: Assemble and

16 Jun 2015: Reset correction test -- CNS verification of Pixcel online processing.

16 Jun 2015: CIRPASS test observations from Cambridge. We have attached the CIRPASS IFU to an 8 inch telescope in Cambridge to test instrument performance.

16 Jun 2015: Rachel Johnson <raj@ast.cam.ac.uk>. Last modified: Mon Nov 6 05:39:04 2000.

16 Jun 2015: Note that the final value is mean rand(sd). Again this command is mostly used for generating test data.

16 Jun 2015: The results of the tests on astronomical objects and internal calibration sources are shown. ... The test observations produced in this chapter generally used most of the night to find and observe each star.

16 Jun 2015: test input catalogue file for cirsi_grid3.pl you may need to edit this since I do not know the exact format for the DuPont Telescope Control System(TCS). ... type cirsi_grid3.pl DUPONT cirsi-test.cat cirsi-test.grid. This will generate some files

16 Jun 2015: On July 9th we officially passed the Gemini acceptance test when we showed that the total measured noise in the system (sky, dark current, flat-field noise, thermal background and

16 Jun 2015: CIRPASS test observations - Nov 2001. During November we observed Polaris using a 5.5mm telescope. ... Although this telescope is much smaller than what we will use later this year it gives perfectly realistic test data because we use the full A-omega

16 Jun 2015: On July 9th 2001 we officially passed the Gemini acceptance test when we showed that the total measured noise in the system (sky, dark current, flat-field noise, thermal background and

16 Jun 2015: Installed here. Waiting for test data.

16 Jun 2015: astro. dome flat. standard. test.

16 Jun 2015: System supports different types of camera ( Astrocam 4100 Hawaii/Picnic , CCD, Qcam, Test etc ) should it build different packages for each camera containing only subset of functions or should camera be

16 Jun 2015: Images have been successfully obtained from the multiplexer inside the test dewar at liquid nitrogen temperatures (77K). ... We already have a 950 nm filter for carrying out the initial photometric tests.

16 Jun 2015: Here is a picture of the Project 1640 PCB. And the detector in our test cryostat at the IoA. ... This is the detector controller attached to the outside of our test cryostat at the IoA.

16 Jun 2015: Note that the final value is mean rand(sd). Again this command is mostly used for generating test data.

16 Jun 2015: range of roles from camera engineering tests to on-line data analysis.

16 Jun 2015: test input catalogue file for cirsi_grid3.pl >you may need to edit this since I do not know the exact format of theDuPont Telescope Control System(TCS). ... type cirsi_grid3.pl DUPONT cirsi-test.cat cirsi-test.grid. This will generate some files

16 Jun 2015: It is convenient to be able to align and test the system during day-light and in all weather conditions. ... The tests were in two forms, long exposure conventional images were taken of the outputs of the beam combiner.

16 Jun 2015: Test this all as follows: SYS> archive [and watch the Talker to see if there is any errors. ... 00:00:00 00:00:00 test (must have colons) then use cirsi_grid.pl. Files will be created of the form name.gaia (ie test.gaia for the example above)

16 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

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.

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.

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

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

16 Jun 2015: The Test Telescope. Note the black flexible conduit trailing on the floor.

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.

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.

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

16 Jun 2015: version of PixCel used for these tests. Different initialisation files. There are a number of initialisation files (.ini) files available.

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

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

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.

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

25 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

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:. %

16 Jun 2015: From tests with ahandful of selected dust materials, we derive a preferencefor mixtures of silicate, carbon, and ice of moderate porosity.

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

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

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

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.

15 Jan 2015: bowed (Milli et al. 2014). We test evidence for the overall bow in our data by independently.

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

16 Jun 2015: version of PixCel used for these tests. Different initialisation files. There are a number of initialisation files (.ini) files available.

16 Jun 2015: fr Subject: CIRSI test fields The exposure time calculator is hard to apply here: the photometry will be totally confusion limited, but the experiment is to discover when, not predict it.

16 Jun 2015: CIRPASS test observations - 24th Jan 2002. The telescope was set up in the CIRPASS lab looking out of a window at the region near the north celestial pole.

16 Jun 2015: FITS writing code which must be distributed and operated before 1999-01-01 should be coded to test the current year to decide whether to use the old date format or

16 Jun 2015: The objectives of the phase-A study are to develop the construction techniques for a new type of fibre-fed spectrograph and to test it on the AAT by carrying out

16 Jun 2015: L H L" %Test routine pixel reads% ADDS_18 = "L H L L H L" %Shutter control type 2 = single line repeat read-out type 4 = normal type 8 = ... VLINE WR_CTRL] JUMP MODE_SELECT; % --------------------------------------------------------------------- % % Test

16 Jun 2015: We currently have one NICMOS science grade array for COHSI along with a test device, we are waiting for the delivery of the second science grade device to make up the