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16 Jun 2015: version of PixCel used for these tests. Different initialisation files. There are a number of initialisation files (.ini) files available.

28 May 2013: overall version log page is readily accessible as an alternative STH - the red star tests actions have been shelved after a tome of a draft paper on characterising same was sent

10 Apr 2013: strcmp(tag,VIRCAM_DOME_RAW) || 00110! strcmp(tag,VIRCAM_SCI_OBJECT_RAW) || 00111! strcmp(tag,VIRCAM_SCI_OBJECT_EXT_RAW) || 00112! strcmp(tag,VIRCAM_TEST_SCIENCE_RAW) || 00113! ... 00293 00294 Revision 1.29 2007/04/23 12:50:22 jim 00295 Added

8 Dec 2006: Figure 1.16 Detector 16. 2. Self Flat Correction. As a first test for the repeatability of the flats, we flat corrected each of the 10s flats that went into the ... 0.49 /- 0.01. 16. 2.45 /- 0.11. 0.65 /- 0.01. In order to test whether the linearity

10 Apr 2013: Detailed Description. These are the main processing routines. Most of these also have a test recipe described on the test recipe page.

16 Jun 2015: The tests carried out produced images with better resolution from the ground than have been obtained in space with the Hubble Space Telescope, and reached nearly 1000 times fainter than was

30 Nov 1998: top end to 180 degrees To test shutter GANTRY> wfcshutter open GANTRY> wfcshutter close Logout when finished GANTRY> logout CURRENT PROPERTIES OF MOSAIC CCDS --------------------------------- SLOW(STANDARD) are the readout speeds = total

16 Jun 2015: dome flats done in the recommended way test! focus, junk, random frames sky! ... Only 'astro', 'standard', 'test' and 'sky' OBSTYPE frames will be combined, chip-by-chip.

16 Jun 2000: I will write more on this when I have analyzed my timing tests.

9 Feb 2022: 2 and apply it to test cases inSec. 3 to demonstrate its behaviour and performance. ... Fig. 4 illustrates the fitting procedure applied to the three test casesfrom Sec.

22 Mar 2024: To this goal, we develop and test a semi-analytic‘N-ring’ framework that is based on a generalized (softened) version of the classical Laplace–Lagrange seculartheory. ... The reader not interested in the details of these tests may skipto the next

10 Apr 2013: sum/(float)np); 00764 00765 / Otherwise test the bpm / 00766 00767 } else { 00768 sum = 0.0; 00769 n = 0; 00770 for (i = 0; i < np; i++) { 00771 if (bpm[i] == 0) {

16 Jun 2015: OBSTYPE string One of OBJECT,ARC,FOCUS,TEST,DARK,DOMEDARK,DOMEFLAT, or TWILIGHT as set on the control GUI. ... band filter 8 H1.573 narrow band (1% bandwidth) filter, aka Hn or H_OH 21 Nov 1999 Domeflat filter test: Lamp meter = 220 Exposure time = 10

16 Jun 2015: fr Subject: CIRSI test fields The exposure time calculator is hard to apply here: the photometry will be totally confusion limited, but the experiment is to discover when, not predict it.

One should check that all the exposures used are at the correct level (light level tests often mean the first few exposures are too high or too low).

22 May 2012: In factin these simulations no test particle has a semimajor axis less than0.5apl. ... Each test particle that is scattered in is plottedwith a discrete value of Ṁ.

16 Jun 2015: version of PixCel used for these tests. Different initialisation files. There are a number of initialisation files (.ini) files available.

24 Dec 2004: Aug 98 Test Run. ... Test Run: Calibration plan SA111(194000) start of night generic standard field 2043-107 MARK-A blue standard (observe at range of air masses) 2111-1308 red standard for colour terms

16 Jun 2015: Note that all these gain figures need to be established with the actual device in use by a method such as the variance test. ... version of PixCel used for these tests. Note: The latest IR version of PixCel allows mode switching between modes 4 and 8

12 Jul 2018: Part III, Paper 316 [TURN OVER. 4. 3. (i) Consider a test particle orbiting a star in the same plane as a coplanar system ofN planets. ... Use this to describe, bothquantitatively and with a sketch, the physical space covered by test particles, all of

10 Apr 2013: 00139 00140 extern int vircam_compare_tags(const cpl_frame frame1, 00141 const cpl_frame frame2) { 00142 char v1,v2; 00143 00144 / Test entries / 00145 00146 if (frame1 == NULL || frame2 == NULL)

23 Jan 2014: 2. 1. Consider a test particle orbiting a binary comprised of a star and planet of massesM and Mpl. ... ẋ′ = ẋ µα0.5(1 e2)0.5A sin nplt ,. ẏ′ = ẏ µα0.5(1 e2)0.5A cos nplt ,where µ =. MplM Mpl. and α =apla. Even though the test

16 Sep 2016: 3. 2. Consider the motion of a test particle in the gravitational potential of a binarycomprised of two bodies of mass M1 and M2 M1. ... Part III, Paper 316 [TURN OVER. 4. 3. Consider the evolution of a test particle due to the secular perturbations of

13 Mar 2012: between 1906 and 1909 to test the weak equivalence principle using a variation on the Cavendish balance. ... Membrane between attractor and test mass shields EM forces All surfaces gold plated to avoid static.

11 Oct 2003: ORAC-DR test routines for UFTI delivered and installed. software module development for standard pipeline on target. ... simulations and completeness tests done. prototype list-driven photometry package written and tested.

10 Apr 2013: Now do a few basic sanity tests.

13 Mar 2019: In both Tack. cases, we do not simulate test particles beyond 14 au, but instead. ... the fraction of test particles that are ever members of the Oort cloud.

25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100 ... Plot shows signal for a 1.5 TeV resonance, in the test model.

21 Oct 2006: Figure 51. Detector 16. 6. Readnoise and Gain. The data that were taken as part of the AIT included flats that were meant to be part of the tests for linearity.

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

22 Mar 2024: We performour averaging tests using different sections (e.g., quarters,thirds, halves) of a box that is slightly longer than theone used for the full-disk averaging described above. ... from the outer regions of the disk, our second test is toanalyze the

22 Mar 2024: This minimises sources of uncertainty thatwould otherwise be difficult or impossible to constrain, i.e., allowing us to test theprebiotic relevance of dust supply in one well constrained early Earth scenario.

15 Aug 2023: students at the IoA [DAMTP/Physics] you are not fair test particles.

22 Mar 2024: 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

22 Mar 2024: Withthese assumptions, we can test if the same evolutionary model is consistent with observations of the Pleiades.

19 Jul 2021: 3.2. Cross comparison of stellar colors for the two epochs of the Kepler Test Tile (KTT). ... IRAC1-IRAC2 colors are compared for the two epochs of measurement of the Kepler Test Tile (KTT).

29 Sep 2006: We have used 6 processors to run this test on the main science recipe, using 12 input raw framesand creating 21 products. ... The detailed processing time of this test is:. recipe time = 320 seconds ( 20% for missing functionalities).

5 Feb 2013: Magnetic dipoles in a ferromagnet!High temperature! Low temperature! Field symmetric!Test dipoles have same. ... energy! Field along unique direction! Test dipoles have different energies! 1/16/13 Astroparticle 20.

23 Jul 2014: Curiously however, all three systemswith directly imaged planets (around A-stars) allow this test.Despite uncertainties about the orbit and nature of the planetaround Fomalhaut (Kalas et al. ... test binary orbital plane - disk alignment ifthe binary

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

18 Jul 2007: 3.4 Observational tests. Here we suggest three observational tests of the critical solidmass model:. ... Observational tests of the model includea flattening of the metallicity relation for Z > 0.5 dex andalso a flattening as planet searches continue.

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

27 Mar 2023: Observations over multipleepochs are necessary to test whether the observed features rotate around the star. ... We first test this processwith the original unsmoothed data and confirm that we mea-.

31 Oct 2003: When this is not available during engineering tests, this may be a fixed value;. • ... NFOC = 0 / Number of positions in focus scan. NFOCSCAN= 0 / Number of focus scans in focus test.

15 Dec 2010: In 3 we summarise how physical parameters relate to thedimensionless parameters for test particles. ... Second-order resonances show qualitatively similar behaviourto the first-order resonances. 3 SCALINGS FOR TEST PARTICLES.

17 Jul 2014: Part III, Paper 59 [TURN OVER. 4. 3. A test particle orbits a star of mass M with a semimajor axis a, eccentricity e andlongitude of pericentre ̟.

19 Apr 2006: A Kolmogorov–Smirnov test showsa probability of only P = 0.6 per cent that the debris and planetstars have the same metallicity distribution. ... of the system that doesaffect the presence of detectable debris remains to be determined.Better statistics

9 Nov 2018: In the case of Gaussian noise, the test would use a nullhypothesis of white noise with. ... The likelihood ratio test gives a test statistic of. Tn,w =(x̄n,w 1).

14 Aug 2003: NFOC. Number of positions in focus scan. inst. inst. NFOCSCAN. Number of focus scans in focus test. ... NFOC = 0 / Number of positions in focus scan. NFOCSCAN= 0 / Number of focus scans in focus test.

29 Sep 2023: observations. This paper aims to test how often the action of the Kozai-Lidovmechanism on a belt of planetesimals due to a wide binary compan-ion can excite the largest planetesimals ... Figure 3. Evolution of a test particle in the eccentric Kozai-Lidov