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21 Nov 2016: A Level/IB Further Mathematics, Mechanics modules are highly desirable. For entry from October 2019 Further Mathematics will be treated as essential for those taking A-levels. ... Standard entry requirements.

12 Sep 2003: of DFS user requirements document. This needs to be finished before the Camera Design Review (next week). ... DWE alter the documentation web page so that there are release and revised dates next to each entry.

23 Jul 2014: provides an overview of various aspects of the UK pipeline and discusses the UK user requirements document , an updated version in response to the UK review recommendations is now available here.. ... ESO estimate of CPU required to run VDFS QC pipeline

27 Jul 2003: Progressing this depends on JPE/WJS updating the science requirements first which will drive any extra requirements for the UK pipeline and archive. ... 8.1 n weeks, 8.2 m weeks and so on with the proviso that if a quarterly task requires less than 1/2

26 Jan 2006: The collection group has to satisfy a number of requirements to produce a viable sky frame, including: a minimum number of independent pointings (ie. ... 5. For tiles and larger areas a unique object catalog was constructed by searching for duplicate

12 Jan 2005: JMS suggested that any extra documentation for the additional UK VDFS requirements should be at the functional specification level, ie. ... Many of the problems with the design of the ETC are related to the overlap of the ETC requirements with the design

16 May 2007: 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,

5 May 2003: the Vista web pages particularly on 1.3 the science/user requirements side. ... the mosaicing requirements really are and who is doing what JRL more deep thought about the naming of the master calibration files.

27 Mar 2006: CASU are still puzzled by the requirements on transfer speed. All of WFCAM 05A and 05B processed data occupies only 16 Tbytes of disk space. ... EGS has made a start sorting out the duplicate entries and he, JRL and RWA need to get together urgently to

26 Jan 2006: The collection group has to satisfy a number of requirements to produce a viable sky frame, including: a minimum number of independent pointings (ie. ... 5. For tiles and larger areas a unique object catalog was constructed by searching for duplicate

4 Jun 1999: Most reduced data frames have been converted back to unsigned two byte integer format to save on transfer and long term storage requirements, however, reduced short exposure photometric standard frames are ... The bad pixel mask files are available by

28 Sep 2006: 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue. ... The typical error in. making a single pass correction is approximately 2, kjkjC 〉〈 , which governs the requirement on the magnitude of the cross

19 Nov 2009: Volume limitedsamples satisfy these requirements, and as well as maximis-ing the proximity of the targets, the stars nearest the Sunare very widely studied. ... Where compo-nents are not resolved in any catalogues we have used, wejust give a single entry

20 Apr 2005: An interesting misunderstanding has arisen about ESO's requirements on the deliverable science products for the processed public survey VST data. ... The software packages tomcat (Solaris 10) and mavan? were mentioned as installation requirements.

18 Apr 2006: He recalled a requirement from JAC for this. This will also be raised at the VDMT. ... However, rather than rushing into this it was felt that this should be science requirement-driven ie.

17 Nov 2003: MJI contacted JPE regarding a list of the sections missing from the User Requirements Document and Calibration Plan document. ... Future budget requirements for this bid are also required for discussion at the next VDMT meeting.

10 Mar 2005: DWE said that he would have a look into this. He also said that he would get a proper CASU entry point set up. ... The UK User Requirements document will be frozen on 15 April (some comments are still being assessed).

18 Jul 2006: 4. Data archives update - AAT, ING, WFCAM, UKIRT AAT - no change ING - EGS said that the data for 1996 had now been refactored into date subdirs and duplicate entries flagged. ... JRL said that he had a nephew coming for a couple of weeks for work

27 Oct 2003: 11) Regarding science verification the main question should be - are the pipeline and archive meeting the science requirements? ... grade detectors MJI contact JPE regarding a list of the sections missing from the User Requirements Document and

26 Sep 2003: cam.ac.uk/wfcam/docs/milestones.html) JRL and filled in most of the relevant entries. ... DWE altered the documentation web page so that there are release and revised dates next to each entry.

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.

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,

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

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

14 Apr 2014: It isidentified by the header entry SIGFILE in the FITS header for the spectrum file,which we here call <NAME>.fits. ... Parameter input file, # entries? [fort.13,1]. >. The ’f’ (or ’F’) in reponse to the first > prompt results in the program

5 Oct 2016: It isidentified by the header entry SIGFILE in the FITS header for the spectrum file,which we here call <NAME>.fits. ... Parameter input file, # entries? [fort.13,1]. >. The ’f’ (or ’F’) in reponse to the first > prompt results in the program

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.