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26 Nov 2020: A Kolmogorov-Smirnov test comparing the distribu-tions of singles versus multiples gives a p-value of 40% for Lupusand 51% forLupus andOphiuchus combined.

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).

16 Nov 2006: level (Figure 1). As a test of the data reduction, we re-reduced the IRS data using the S13. ... As a test of the robustness of our best. fit model, the last column in Table 1 also gives the best-fitting χ2ν found after deleting a.

5 Apr 2005: As confidence in the pipeline reduction is established, then the frequency canbe reduced, perhaps only making the test every time the instrument is mounted.

11 Sep 2017: ABSTRACT. To test alternative hypotheses for the behavior of KIC 8462852, we obtained measurements of the star. ... they should be negligible for the Spitzer measurements.). To test for such effects, we turned to the photometry of.

27 Jan 2016: the phase fluctuations but on-sky verification tests haveshown that large phase jumps can occasionally occur andcause fringe jumps (even with the phase loop running at1 kHz).

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

29 Sep 2006: 5 Internal consistancy of the photometry. A simple way to test the homogneneity of the photometric calibration is to look at thedispersion in the median colours of high galactic latitude WFCAM

4 Nov 2003: This needs a final shakedown, code tidy and further tests beforebeing released at the end of Q4. ... Still awaiting delivery of "correct" PC :-). • Still waiting for WFCAM engineering test data.

7 Oct 2011: 961 test particles were placed onorbits exterior to a planet of massµ = 108 and their orbits inte-grated for 10 Myr.

11 Jul 2019: However, us-ing a Kolmogorov-Smirnov (KS) test, they demonstratedthat the period distributions of their disc-bearing anddisc-free binaries and multiples were not, in fact, differ-ent in a statistically

20 Jan 2008: 1 Introduction. During July 2007, an engineering team from RAL, ATC & QMU obtained some 2,300 VIRCAM frames during EMC testing and other miscellaneous lab tests. ... Further tests need to be done off sky to determine whether persistence of this kind is a

8 Oct 2018: The power of the hypothesis of homogeneity is that our own observationsfrom Earth are then all we need to test a cosmological model. ... On galactic scales, consider Figure 1.8. With gravity supplying the cen-tripetal force required to keep a test

8 Nov 2011: Figure 2. The minimum pericentre for a test particle scatteredby a single planet, as a function of the Tisserand parameter value,from Eq. ... Figure 4. The minimum pericentre for a test particle scatteredby two planets, as a function of the ratio of the

14 Feb 2022: We also test a different more physically moti-vated model for releasing the CO and assume it comes from theslow heating provided by the Sun over long timescales, whichwarms up large ... 2017, 2019) is valid for the KB (Model 1).Second, we test a more

2 Jul 2014: Our systems consisted ofa massive particle representing the planet and 103 to104 massive test particles to model the disc.

8 Mar 2021: cient frames for sensitivity purposes. After several tests,the optimal selection was found for a maximum nulldepth of 12% resulting in a total integration time of 920seconds (or approximately 15 minutes).

29 Jun 2020: For this ACA-only fit, and. for the later combined ACA12m fit, we test three dif-. ... Statistical. tests such as the Akaike Information Criterion (AIC). and the Bayesian Information Criterion (BIC) confirm.

25 Feb 2022: Posteriorprobability distributions of the model parameters are explored withtheemceepackage(Foreman-Mackeyetal.2013),animplementationof theMarkovChainMonteCarlomethod inPython.We initiate ourmodels near the solutions of previous test runs.

16 Nov 2017: sequence that gives rise to the recently created white dwarfs – can perform direct test of stellar evolution theory• Evolution of stars from horizontal branch to white dwarf is almost instantaneous relative

17 Dec 2008: As a simplified test of the model, we conduct simulations sim-ilar to those of Lufkin et al. ... with either the central star or one of the migrating planets(The planetesimals are treated as test particles so no planetesimal-planetesimal collisions take

15 Dec 2003: Simon Hodgkin, CASU. WFCAM characterisation plan. detector noise properties. microstepping test.

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

17 Nov 2017: sunns. LLT. RRTRL. • Rich variety of phenomena now known. Powerful tests of General Relativity using close binary pulsars now possible – multiple Nobel Prizes! •

19 Apr 2006: To test the sensitivity of the model fits to the assump-tion of astronomical silicates, we also fit the radial pro-files using amorphous carbon grains (ρ = 1.85 ... grains. TheMIPS and SCUBA observations are then distinctly dif-ferent grain populations.

28 Oct 2023: In neglecting this slight asymmetry, we make the assumptionthat the additional centripetal force acting on a test mass at the equatorof the star is small compared to the gravitational force.

7 Jul 2020: Future imaging ofthe faint debris disc in π Men and precise constraints on the stellar spin orientationwould provide strong tests for these formation scenarios.

28 Nov 2018: Ideally the method should have a solid physical underpinning andhigh internal accuracy, amenable to empirical tests for systematic errors. ... The masing clumps act as dynamical test particles. A rotation curve ismeasured along the major axis of the

4 Feb 2004: test and debug new catalogue parameter measures MJI. 9.2 refine astrometric calibration model MJI paused. ... 16.3 implications for deriving catalogues and parameters test profile fitting parameters and write report DWE.

20 Aug 2021: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact

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 Nov 2019: 4.3. Exploring Hypothetical Exoplanetary SystemArchitecture. Stars that host both a debris disk and one or more exo-planets serve as critical test beds for studying the forma-tion and evolution

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.

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

18 Aug 2020: We also discuss potential tests toconstrain the largest planetesimal sizes and debris disc masses.

5 May 2017: Preliminary tests showed good fits in two re-gions of parameter space, which we, therefore, split into twoMCMC runs: run A, which is constrained to be a narrowbelt (with Rin > 57 ... 2011). As in MacGregor et al. (2015), we also con-sider a Gaussian

14 Nov 2023: It is with this idea inmind that Bergeron, Saffer, & Liebert (1992, BSL hereafter) decided to test thespectroscopic method using DA white dwarfs at higher effective temperatures(Teff > 13, 000 K) where

12 Jan 2012: Prelimi-nary tests found that icy grains provided a much better fit thansilicates. ... In addition, secular per-turbations lead to precession of test particles’ nodes coupledwith inclination variations.

10 Oct 2023: Gaia is also providing a numberof stringent new tests of general relativity and cosmology.

23 Oct 2023: Referring to Figure 7.1, the gravitational force acting on a test particle ofmass dmi at a distance r from the centre of a spherically symmetric massdistribution is. ... The corresponding gravitational potential energy ofthe test mass is:. dUg,i = GMr dmi

6 Nov 2018: We saw in Lecture 6 that theapparent magnitudes of distant Type Ia supernovae (essentially a lumi-nosity distance test) delimit a region of the Λ,0-m,0 plane that is ... Thus, thecombination of the two tests, one based on dA and the other on dL, is

30 Jan 2020: MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled using MNRAS LATEX style file v3.0. Population synthesis of exocometary gas around A stars. S. Marino1?, M. Flock1, Th. Henning1, Q. Kral2, L. Matrà3 and M. C. Wyatt41Max Planck Institute

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.

22 Aug 2014: 2014). Our sample is not meant to becomplete, but to provide a sufficient number of sources for usto test whether the two-temperature disks arise from singleormultiple belts.

22 Jan 2018: 2016). As such, HR8799 isan ideal test system for planet formation and evolution the-ories, as interactions between planets themselves and withdebris can be investigated. ... simulations from the four known planets interacting with a pop-ulation of test

9 Oct 2013: Thus, these models require calibration with well-studied (nearby) test cases. For example, star formation involves turbulence, magnetic reconnec-tion, collisionless shocks, and radiative transfer through a turbulent medium. ... in the Plane to test

25 Nov 2015: In Section 5, we test the spatial scale and dust propertiesagainst bow wave models to break the SED degeneracy and deter-mine which mechanism is more likely. ... The PSF reference star can be scaled to the peakemission and subtracted from the data images

10 Apr 2013: mjd,cdata,cf,fac; 00481 double facrng,maxdiff,lindata; 00482 vir_fits darks,domes,outfits,test,outdark,fframe; 00483 parquet pp; 00484 cpl_parameter p; 00485 cpl_propertylist drs,plist; 00486 ... fits_get_image(test)); 00667 vircam_fits_delete(test);

9 Oct 2012: arX. iv:1. 208. 1759. v1 [. astr. o-ph. EP. ] 8. Aug. 201. 2Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 10 August 2012 (MN LATEX style file v2.2). Coplanar circumbinary debris disks. G. M. Kennedy1, M. C. Wyatt1, B. Sibthorpe2, N. M.

22 Nov 2018: and thereforev(R) R. (16.8). For a test particle located at sufficiently large R so that M(R) is constant,we expect. ... As we move to largerdistances from the disk, we run out of ‘test particles’ as stars in the halobecome more and more scarce.