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Дата изменения: Wed Apr 8 01:09:48 2009
Дата индексирования: Tue Aug 18 10:28:01 2009
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Discussion Part 2: MKSP work plan
1. Project Plan (Deadline: 2009 May 15)
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Science background and goals:
Galactic fields (M. Haverkorn) Pulsars & the Galactic magnetic field (A. Noutsos) Spiral galaxies (R. Beck) Irregular, dwarf & interacting galaxies (C. Chyzy) Giant radio galaxies (G. de Bruyn) Intergalactic filaments (P. Alexander) Stellar jets & AGN jets (J. EislЖffel)

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Source lists (all) General technical requirements (all) Software and processing requirements (all)


2. Use Cases
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(detailed technical specifications, guide to the LAD group) (Deadline: 2009 June 30) Contents:
Flux densities & dynamic ranges (in Stokes I and PI) Integration times and distribution (continuous or blocks) Angular resolution & angular size of interest Field of view Number of simultaneous beams Time resolution Frequency resolution & frequency span Subband frequency selection RM resolution & total RM range Images or RM cubes needed ? Type of RM analysis ? Analysis of full RM cube or only subregion(s) ? Visualisation of RM cubes needed ? Required storage and timescale

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Authors: Working group leaders Template prepared by James Anderson (see MKSP WIKI) Three preparation meetings (Milky Way, nearby galaxies + radio galaxies, pulsars) in early May 2009


3. Commissioning Plan
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(Deadline: 2009 June 30)

Contents:

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Sources Dynamic range Time resolution Long baselines Frequency resolution Frequency span Subband selection Elevation Daytime / nighttime Ionosphere Intra-station baselines Instrumental pol Circular pol RM Synthesis

Early commissioning in April: Enno & Anna Template prepared by James Anderson (see MKSP WIKI) Authors: Working group leaders Three preparation meetings in Bonn in early May (same as for the Use Case)


4. Task list
· · · · · · · Calibration, ionosphere, global sky model (G. de Bruyn, J. Anderson, A. Scaife, P. Alexander) Data storage (E. Middelberg) (NEW) Implement polarisation into pipeline (S. Duscha) RM Synthesis (S. Duscha, T. Enъlin, R. Stepanov) Source finding (A. Scaife, E. Middelberg) Visualisation of RM data cubes (G. Heald) WSRT & GMRT observations (T. Arshakian, G. de Bruyn, D. Green, G. Bernardi, R. Beck) Simulations of the pol sky (W. Reich) Synthetic RM cubes from magnetic field models and modelling depolarisation effects (A. Fletcher, J. GeisbЭsch, J. Kim, R. Beck) Pattern recognition from RM grids (R. Stepanov, R. Beck)

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5. Finally
· · · · · · MKSP webpage needed (R. Beck) Membership: see actual list on MKSP WIKI Time allocation: under discussion in the International Working Group Data rights: to be discussed Publication policy: to be discussed Next workshop: Winter 2009/10 (Innsbruck? Garching?)