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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 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

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.

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.

9 Mar 2018: One of our goals was to test for a correlation between the bright-. ... detect those above a given dust level, so we cannot test for a cor-.

25 Oct 2018: There are two things to keep in mind here. (1) Althoughwe cannot explore this era empirically, we can test the consequences of ourmodels with observations of the Universe at later times.

30 Jul 2018: Fig. 1.A belt of test particles start exterior to the planet. In or-der to speed up the simulations, we do not need to trackthe particle’s evolution from the ... All variables arelisted in Table A1. The test particles all have low initial

14 Nov 2018: Thus, if we want to test from our data whether the intrinsicproperties of the absorbers evolve with cosmic time, we need to decouple.

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

30 Oct 2018: Measurement of twoor more elements would in addition allow us to test the theory, since thevalues of η indicated by any two elements should agree.