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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

20 Feb 2024: We use both parametric and non-parametric modelling to test if their inner edges are shallow and consistent with collisional evolution.

31 Jul 2018: the most optimum at producing exozodis anddelivering cometary material to inner planets, and we test. ... 1987). Below we present the mainanalytic considerations and predictions from previous worksthat we will test with our simulations.

2 Jul 2014: Our systems consisted ofa massive particle representing the planet and 103 to104 massive test particles to model the disc. ... outermost line) exterior resonances with the planet. Middle:. the line shows the path of the planet and the cross marks

5 May 2017: 16) and eq. (17). For the top panels i = 10,for the middle panels m3 = 1MJ and for the bottom panels a3 = 2au.

22 Mar 2024: The PSO framework was chosen as it showed, during tests,a higher convergence rate than Bayesian optimisation and al-lowed multi-core estimation7, reducing the computation time.More standard minimisation frameworks

10 Mar 2015: 4 (i.e. top right and middle right) that removing the stel-lar flux density does not account for all of the emission locatedat the stellar position. ... Thus, the limit on CO gas is not stringentenough to test different scenarios for the production of

25 Apr 2019: Manual, http://pencil-code.nordita.org/doc/manual.pdf. 96. C. P. McNally, W. Lyra, J.-C. Passy, A Well-posed Kelvin-Helmholtz Instability Test and. ... S6 &. S7 can be found in the directory pencil-code/samples/2d-tests/WhiteDwarfDisk, using version.

17 Jan 2020: Dipper Disc Inclinations 5. Figure 1. ALMA images (left) and associated visibilities (middle) as well as K2/C2 light curves (right) for the sources in our sample. ... In order to more robustly test whether the inclina-tion distribution at id.

29 Sep 2022: We will test this with simple modelsthat parameterise the surface density distribution of dust as a func-tion of the radial distance from the star. ... Albeitwith less significant fits in additional tests, i.e., poorer 𝜒2 andBICvalues, and visibly

19 Feb 2010: right panel) we estimate the significance of changes be-tween different age bins with the KS test. ... According tothis test, each pair of cumulative distributions for thethree youngest bins (three upper curves) could have allcome from the same