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18 Oct 2020: ii) Squared coherence programme which tests statistically the correlation between the oscillations in two series. ... dry conditions). Analysis was carried out with the following tests (i) Squared coherence relations: scarlet.

17 Jan 2006: Tests on real WFCAM data (the UDS test data, see Section 6) showed that a more detailed model was required. ... 7 Crowded field tests. Tests have been carried out using data covering M17 in order to test the performance in more crowded fields.

26 Nov 2009: So one slot for a biscuit joint didn't quite go through the middle of the board. ... Strictly speaking you should test all joints out dry, to see what needs adjusting with some more chisel work.

19 Aug 2003: Repeatability of filter placement is probably a good thing to test also - this can be done in a number of the tests below I guess yes definitely DETECTOR NOISE PROPERTIES The ... Vignetting function and its motion if any. Tests of different flat fielding

26 May 2006: Tests were carried out using only LAS data, where the images are quite sparse, and the results were just as noisy, thus eliminating this explanation. ... Only the primary persistence is removed. The lower graph are slices through the middle of the images

3 Nov 2000: canopus ftpcd mydir -- your directory where the file is ftpget cirsi-test.grid cirsi-test.objects (extension to be. ... console [green and black numbers on screen and red indicator on the middle console (SELECTED DATA).

17 Jan 2006: Tests on real WFCAM data (the UDS test data, see Section 6) showed that a more detailed model was required. ... 7 Crowded field tests. Tests have been carried out using data covering M17 in order to test the performance in more crowded fields.

26 May 2006: Tests were carried out using only LAS data, where the images are quite sparse, and the results were just as noisy, thus eliminating this explanation. ... Only the primary persistence is removed. The lower graph are slices through the middle of the images

2 Nov 2006: In the following tests we have used the 2MASS PSC as the basis for all the astrometry. ... taken roughly in the middle of the night (and as it happens also taken within 4 days of new moon).

18 Jul 2006: Currently, the RAL team are in the middle of intensive spot projection tests of VIRCAM. ... JRL reported that the ESO end-to-end test had been very successful.

2 Nov 2006: In the following tests we have used the 2MASS PSC as the basis for all the astrometry. ... taken roughly in the middle of the night (and as it happens also taken within 4 days of new moon).

16 Jun 2015: 4) Double-click (middle mouse button) on a star in the guider field to move the guider close to that position (a single click with left mouse button gives the coordinates ... OBSTYPE string One of OBJECT,ARC,FOCUS,TEST,DARK,DOMEDARK,DOMEFLAT, or TWILIGHT

17 Dec 2008: As a simplified test of the model, we conduct simulations sim-ilar to those of Lufkin et al. ... entr. icity. Mass Multiplication. Middle Planet. 0. 0.05. 0.1. 0.15. 0.2.

27 Jan 2016: The result of this process is shownin Figure 7 (see middle panel), where most of the back-ground fluctuations are now corrected. ... Middle: same measurements after subtraction of si-multaneous background measurements (left). The

16 Jun 2015: ADDS_1 = "H L L L L L" %Shutter open time - middle byte%. ... binning is required. Routine must be called with ADDR_19 set%. EPR3_TEST:. %

16 Jun 2015: For example to read a 32 x 32 pixel region in the middle of the array, the program sequence would be:. ... In tests, the relationship is slightly different as shown by the plot in Figure 3.15.

16 Jun 2015: READ 5 - QUAD Select 6 - CHIP Select 7 - Initialize (B) % ADDS_1 = "H L L L L L" %Shutter open time - middle byte% ADDS_2 = "L H L L L L" ... L H L" %Test routine pixel reads% ADDS_18 = "L H L L H L" %Shutter control type 2 = single line repeat read-out

19 Jan 2012: We find that the gaps between these planets arenot only dynamically stable to test particles, but are frequently populated by planetesimals. ... The gas simulations test the effect of the presence of agas disk during and after the giant planet

30 Jul 2018: All variables arelisted in Table A1. The test particles all have low initial eccentricities ofei = 0.01, either low or moderate initial inclinations, withIi = 0.03. ... The fraction of particles accreted by the planet de-creases with the planet’s

19 Jan 2015: Note that the Fisherexact test can only reject the null hypothesis, never toprove it true. ... The same conclusion results from theFisher exact test (Table 8, lines 27 and 28).