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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: 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

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.

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).

30 Jan 2020: Middle: high viscosity and high CO input rate. Bottom:low viscosity and high CO input rate. ... In the middle panels, the CO mass input rate is now 100times higher.

31 Jul 2018: The residuals of band 6 (middle row). and band 7 (12mACA, bottom row) are computed using natural.

21 Jul 2016: Middle:spectrum after subtracting the 3rd-order polynomial shown in red in the toppanel. ... 10 100. 1.0. 8. 6. 4. 2. 0. KS–Test Comparison Cumulative Fraction Plot.

22 Mar 2024: 3.2. Polarized dust emission in the middle versus outerregions of β Pic. ... Thebox has dimensions of 12130 pixels, corresponding toa box size of 1.′′718.′′2 or 32.7 au354 au.Our first test is to analyze the middle half of the disk.

14 Sep 2015: 2013; van der Marel et al. 2013; Pérez et al. 2014)could not test the trapping predictions. ... Top: cross-correlation before out-lier filtering. Middle: after outlier filtering, but before as-trometric WCS correction.

3 Nov 2008: For eachmodel described below a range of parameters was tried and aχ2 goodness-of-fit test applied to find the best fitting parametersand confidence limits (errors from background statistical error).In ... To test whether more complicated models are

15 Oct 2020: 2017) as a test of its validity. The prescriptionpresented by Cataldi et al. ... For each test population, we calculate, using equations 9 11in Wyatt et al.

29 Apr 2021: To test this hypothesis S14 conduct N-body simulations withrandomly sampled initial separations and eccentricities of the ACbinary; B is generated at a random location within the Hill sphereof the system ... From examination of the residuals for this

8 Jan 2019: Middle:Comparison between opposite wedges with a mean PA of 45 (NE,green) and 225 (SW, orange). ... 12 au for the topand bottom panels and 20 au for the middle panel approximately.

5 May 2017: By repeatingthis prescription for synthetic data we are able to test different scenarios for how the occultationsdo or do not repeat. ... We leave the development of a quantitative study of thisscenario for the future, noting that tests of such a model

23 Jun 2009: This image acts as a PSF reference. Middle: The final image of HD69830. ... The residual image shows no evidencefor emission beyond the PSF. Further tests comparing the pro-files of the observations, Gaussian and Moffat profile fits to theimages and

17 May 2016: The marginaliseddistributions ofr, h = H/r and r0 are presented in the top, middle right andbottom right panel, respectively. ... Left middle panel: marginaliseddistribution of MCO and r0. Left bottom panel: marginalised distribution ofr and MCO.

30 Oct 2012: 5). In con-trast, the initial conditions which lead to instability for the η =0.5 simulations (middle panel of Fig. ... The middle and bottom panels of Fig. 10 indicate that the frac-tion of bodies which escape does not necessarily scale with a0;.

25 Oct 2022: DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style in AASTeX63. ALMA Observations of the HD 110058 debris diskANTONIO S. HALES,1,2 SEBASTIÁN MARINO,3,4 PATRICK D. SHEEHAN,5,2 SILVIO ULLOA,6 SEBASTIÁN PÉREZ,7,8,9 LUCA MATRÀ,10,11.

7 Nov 2012: left – 70 µm; top middle – 100 µm; top right – 160 µm; bottom left – 250 µm; bottom middle – 350 µm and bottom right – 500 µm. ... 3 (middle) indicating a double-lobed structure. Fitting this as two Gaussians gives 8.0 mJy forthe

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

31 Jul 2018: E-mail: schaefer@lsu.edu. 1 INTRODUCTION. The star KIC 8462852 (Boyajian’s Star) is a perfectly or-dinary, isolated, and middle-aged F3 main sequence star in. ... This demonstrates that thesecular decline from 1890 until the end of the Kepler run

13 Nov 2017: Currently efforts to test this scenario observationallyare in their infancy and over-lap with efforts to test models for photoevaporation(see below).

18 Jan 2018: These tests were however not exhaustive. Formally, we can use the Schwarz criterion (Bayesian In-. ... formation Criterion, or BIC) to test which among our models. should be preferred (Schwarz 1978).

22 Mar 2024: so we can test different initial surface-density profiles; weconsider initial surface-density profiles between 𝑟0 and 𝑟1.5.

24 May 2022: 2021a). In each setof figures, the left image shows the coronagraphic point spread function for each bandpass, while the middle and right panels show subsequentimage post-processing employing Angular Differential Imaging

14 Feb 2019: 2. The belt spine (Fig. 3, middle) presents little verti-. cal displacement along the midplane and is largely. ... Nonetheless, we test whether we can. detect a radial dependence of the vertical aspect ratio.

22 Sep 2005: The only sensible long term (ie. economic) option is to use internet transfers. ... results. Further tests are still ongoing in conjunction with Omar Almaini the UDS PI.

29 Jun 2012: Our aim here is to test this prediction for Saturn’s dustcloud using the 24µm Spitzer Space Telescope observationsused to discover the Phoebe ring. ... The ON scans are easily identifiable by thelarge bump in the middle due to the Phoebe ring.

9 Oct 2012: 33. 0.00. 1.33. 2.67. 4.00. Figure 6. Residuals after the resolved model ofα CrB is subtracted from the observations at 70µm (left) 100µm (middle) and 160µm (right). ... 1.33. 0.00. 1.33. 2.67. 4.00. Figure 8. Residuals after the resolved model ofβ

11 Jul 2023: ted lines) at various epochs. The middle panel shows the volatilecontent of planetesimals as a function of diameter. ... order of magnitude.This is plausibly an important test of whether large planetes-imals.

29 Apr 2008: 2000)? Or are we witnessing the colli-sional destruction of massive asteroid belts or the sublimationof comets in the middle of fully formed planetary systems? ... show three different models:Top: Face-on, large radiusr; middle: Face-on small radiusr;

31 Jul 2018: Severalmission architectures were proposed, key enabling technologies were developedand demonstrated on laboratory test-benches, and advanced data reductiontechniques were investigated. ... Although this performance is suf-ficient for flight, it would be

5 Apr 2018: We here test the hypothesis that these selection ef-. fects alone applied to a population uncorrelated in. ... vant for its formation, which depends on which theory. we are trying to test (see discussion in 4).

6 Apr 2010: 2008). To test the limits we can place on disc extension with un-resolved images, we performed the same PSF subtraction andresiduals testing on models of stars+ discs. ... temperature fit is 70K). Photometric confirmation of the excessis necessary to