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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.

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:. %

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: 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

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).

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