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14 Sep 2015: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 14 September 2015 (MN LATEX style file v2.2). Planet Hunters X.KIC 8462852 – Where’s the flux? †. T. S. Boyajian1, D. M. LaCourse2, S. A. Rappaport3,D. Fabrycky4, D. A. Fischer1, D.

16 Jul 2021: The hori-zontal lines separate the (top) Band 6, (middle) 2016 Band 7 and (bottom)2018Band7observation sets.All times represent time on source.

19 Feb 2018: a test of whether an IR excessis present.

12 Apr 2013: Figure 4. Critical Hill semimajor axis ratios as a function of stellarmass for different eccentricities (upper panel), different mutual incli-nations (middle panel) and different planetary masses (bottom panel).The purple

23 Nov 2021: While ALMAclearly shows dust concentrations (e.g. van der Marelet al., 2013; Casassus et al., 2013), we cannot test ourunderstanding of radial migration, settling, and graingrowth without quantifying the gas reservoir

7 Nov 2016: tance to the star along the major (top panel) and minor axis ofthe disc (middle panel) obtained averaging over 40 wide wedges.In the bottom panel we present the mean intensity ... In order to test the latter scenario andsee if the disc morphology can be

24 Oct 2015: the star-forming gas reservoirs within and beyond the CND(e.g., Liu et al., 2012)—such as peculiar objects like the G2 cloud (Gillessenet al., 2012)—to test scenarios of ... FIG. 3.ÈNatural weight VLA maps of the sources VLA 1 and 2, made with the 6

23 Mar 2007: 2005), F24disk/F24? 150t1age ,is shown with a solid line. (Middle) Fraction of stars with fluxratios in the different age bins used by Rieke et al.

18 Oct 2014: A Fisher’s exact test shows that there is only. a 0.7% chance of detecting rates as discrepant if the two groups had the same distribution.

23 Jan 2014: While Figs 2b and 2d provide the best estimate of theunderlying inferred accretion rate distributions in the sub-samples, we will also use Fisher’s exact test to assign a

1 Sep 2005: Images were found to be 0.65" on all chips (Gemini reported 0.5" images in V on the same night) on the 1st night of on-sky tests. ... crosstalk removing algorithm has been written by MJI, and is in the middle of consumer testing.

23 Jan 2000: Generally it is safe to change any value while the camera is not reading data, changing readout mode in the middle of an integration might be a bad idea. ... TEST. Returns pixcel version and build date, used to test link.

4 Jan 2010: MJI noted he has so far only done limited testing on it, however, RGM offered to test it further. ... This was done by the middle of December using a 1TB external USB drive.

28 Sep 2009: The proforma was split into five sections representing the main priority areas of STFC: Excellence, Economic Impact, Societal Impact, Leadership and Synergies etc. ... Apparently low light level tests have been done and the data delivered to Derek Ives

6 Mar 2013: A l'autre main a good benchmark/null result for the next test. ... However, es ist noch nicht klar and we await the red star test results with something approaching interest.

16 Jun 2015: 1.2) The timescale of DATExxxx is not defined. 1.3) The relation of DATE-OBS to the start, middle or end of an observation is not defined. ... FITS writing code which must be distributed and operated before 1999-01-01 should be coded to test the current

19 Dec 2011: There was much discussion of observing strategy and the results from the test data taken so far (any choice bits are incorporated in the VST section). ... image tests, require much more effort to characterise and attempt to find solutions for.

30 Nov 2009: No further occurrences of the filter wheel position being lost in the middle of the night have occurred yet. ... Detailed tests projecting the residuals onto the detector grid reveal no measureable wavelength dependence of the distortion model at levels

16 Dec 2008: A simple test is to monitor the stability of the difference between ZPs derived from consecutive J and NB118 data. ... This data also provides an interesting test case for the nebulosity filter developed for GPS photometry in regions of high nebulosity.

28 Sep 2009: stack properties of the VISTA J-band pawprint test data and made the report available through the VISTA technical pages 2. ... It is not obvious if this will improve DXS results so MJI asked for a test night to be selected to trial.