Search

11 Mar 2006: Commissioning: It is unclear what requirements there are on CASU presence and use of CASU VDFS pipeline software during commissioning. ... MJI volunteered to update JPE's data management plan template suggesting that for standard VDFS processing tasks

5 Mar 2014: MJI had a productive meeting with representatives of one of the new "owners" of UKIRT to discuss the extra special purpose processing requirements. ... We intend to take this opportunity to discuss the "new" processing requirements in further detail and

25 Feb 2005: made no further progress on updating the CASU group web pages entry point - ongoing EGS has made progress on the calibration of large WFS surveys. ... The main requirements for desktops would be for RWA, MR and EGS, since they currently have old systems.

19 Apr 2013: The WFAU apm7 uklight and wfcam access entry point was resurrected thanks to SC and should all now be back on the road. ... The obvious issue here is partial tile OBs for VVV where having the same pair of tiles used for sky estimation is a requirement.

15 May 2006: The entries in the database are manually entered so are variable in content. ... The software now meets the write to disc requirement. The TCS and camera software has been altered so that operations can now be carried out in parallel, though whether ESO

8 Feb 2007: Priorities for the filters? • moon phases requirements, transparency requirements; • time constraints – absolute or relative (see. ... www.eso.org/observing/p2pp/P2PP_future.html). b) Observing requirements:. • Requirements on seeing,

24 Aug 2012: MJI pointed out the lack of a P89 entry on the progress web pages plus a few leftover "ingested" but not correctly flagged odds and ends, including what appears to be ... EGS has been burning the midnight oil analysing simulated spectra for 4MOST and

29 Sep 2006: The regular text is the CASU response to the requirement. Only requirements that are relevant to CASU are commented upon. ... The UK User Requirements [AD3], requirement 5.4, also states that the pipeline should be able to operate at 1 Tb/day for 10 days,

16 Jun 2015: 90){ @Smallbf Refer to {it Notes for Guidance %on the completion of the application form PATT2;} type entries in black } put(00.40,23.20){{ @thline }} %0.40-0.38 ... position or quarter, }} put(01.90,20.60){{ it instrument preparation requirements, etc }}

22 Mar 2024: in 2015Obs. 2 at 0, and defining the coordinates of all other clumplocations relative to thisobservation,givingrise to5freeparameters.Wealsoassumed independently and identicallydistributedGaussianerrors across all entries in Δobs,with the standard

23 Jul 2014: With nightly data-rates of a few hundredGbytes (i.e. 10,000 individual 2k 2k images) automatedpipeline processing and data management requirements areparamount. ... which governs the requirement on the magnitude of the cross-talkterms. source of the cross

9 Nov 2018: The solution to remove this class of events is to empiri-cally look at the comet entry and exit parameters, θ and λ.If one was found to be more than ... MNRAS 000, 1–11 (2015). 10 GMK et al. requirement less stringent.

22 Nov 2018: Neutrinos 0.001. Photons (CMB) 5 105. Comparing the entries in the third and fourth row, we see that stars andtheir remnants (mostly white dwarfs) account for less than 10% of ... In any case, the search continues for a WIMP that may fit theastronomical

18 Apr 2022: Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED ESO 2022April 11, 2022. Large Interferometer For Exoplanets (LIFE):. I. Improved exoplanet detection yield estimates for a large mid-infraredspace-interferometer mission. S.P. Quanz1,

19 Feb 2018: The requirement for planetesimals,themselves a step in the planet formation process, makes debrisdiscs a fundamental component of planetary systems. ... 2013), who use a 3σ excess detection at any PACS wavelengthas their disc detection requirement.

11 Mar 2014: In mathematical termswe may write this requirement as. v. vk |v(t t) v(t)|. ... This arisesfrom the requirement that the new orbit of a particle must passthrough the point at which the kick is applied that is responsiblefor the apocentre and pericentre

29 Sep 2022: MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled usingMNRASLATEXstyle file v3.0. High resolution ALMA and HST imaging of 𝜅 CrB: a broad debrisdisc around a post-main sequence star with low-mass companions. J. B. Lovell1,M.C.Wyatt1,

7 Jun 2007: DRS dictionaries Update vircam_standard_process, modify vircam_jitter_microstep_process, and modify entries in table 10-1. ... 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue.

10 Feb 2014: arX. iv:1. 402. 1184. v1 [. astr. o-ph. SR. ] 5. Feb. 201. 4. Spatially resolved imaging of the two-component η Crv debris disk with Herschel. G. Duchêne1, P. Arriaga. Astronomy Department, University of California, Berkeley, CA 94720, USA. and.