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CASU WFCAM/VISTA Diary Page
https://people.ast.cam.ac.uk/~wfcam/diary.html24 Mar 2010: The generic flatfield test data we would like to acquire prior to WFCAM commissioning. ... Eckhard is doing further tests to find the source of the Cambridge-Edinburgh bottleneck. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100728.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100728.txt29 Jul 2010: Unfortunately the test involved flooding all the detectors and noting the decay time of the overall background. ... A more realistic test involving saturated isolated star tests would be more relevant to normal operations but also unlikely to yield much -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100532.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100532.txt7 Jun 2010: This includes, as part of a throrough shakedown test, the automatic production of tiled data products. ... The data transfer test is still on the agenda and will likely involve the transfer of a week of compressed data from Garching to Cambridge (in -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091223.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091223.txt4 Jan 2010: MJI noted he has so far only done limited testing on it, however, RGM offered to test it further. ... where links to the raw data packages, a preview of some pawprint-level data products, and a report describing observations, tests, and results are all -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100216.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100216.txt24 Mar 2010: new waveform test data but the linearity tests require further effort and/or better data. ... A set of test data from 20100129 was fast-track processed by MJI and JRL spent a while straining his eyeballs to assess the effects. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt5 May 2010: There's enough high latitude data to do overlap tests. Should be ready by next meeting. ... Various transfer tests between Santiago and Garching have been made to tune system performance and further tests including to Cambridge are planned. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100324.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100324.txt19 Apr 2010: are written and prototyped in different languages (toolkit and pipeline) and the result intercompared, test datasets are also used to check results when bug fixing or smaller upgrades occur. ... Direct tests revealed no problems! but a more indirect -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt2 Jul 2010: He also noted that the calibration units have been installed and after a few flux level tests good linearity sequences et al. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_101027.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_101027.txt3 Dec 2010: Continuing Actions: =================== STH - produce "final" VISTA colour equations and finish revising MJI calibration plan document EGS - put WFCAM illumination correction tables on the web MJI RGM - finish catalogue software tests EGS - -
arX iv:1 012. 3079 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mw11.pdf15 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. -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 Sep 2010: 2006). Here we investigate the formation of planetary systemsby observing some of the oldest Galactic stars with Spitzer.A good test of models is to observe old, metal-poor stars. ... Since starsobserved with good signal-to-noise tend not to be -
arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/gw10.pdf29 Jan 2010: 3.3 Single population hypothesis. We first test the simplest possible hypothesis, that all Solar-type stars have debris discs drawn from a single distribu-tion. ... This is not possible to testwith the current data, but Herschel observations should -
arX iv:1 011. 1437 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mctw10.pdf10 Nov 2010: As a test of the robustness of the temperature estimates,the 24.5-µm brightness profile was shifted by1 pixel (6 AU)along the x-axis relative to the 18.1- ... Thus, another test for our pericenter glow model is whether itcan replicate the observations -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 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 -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 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 -
Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…
https://people.ast.cam.ac.uk/~wyatt/kw11.pdf25 Nov 2010: arX. iv:1. 011. 4858. v1 [. astr. o-ph. EP]. 22. Nov. 201. 0Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 November 2010 (MN LATEX style file v2.2). Collisional Evolution of Irregular Satellite Swarms:. Detectable Dust around Solar
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