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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

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;.

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.

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.