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Meeting of the MKSP Nearby Galaxies Working Group
Cambridge 2009 March 25 09:30-12:00
Participants: P.Alexander, J.Anderson, R.Beck, C.Chyzy, A.Fletcher, J.GeisbЭsch, G.Heald, J.Riley, H.RЖttgering, A.Scaife

1. Science Case / Project Plan Version of 2007 urgently needs update. Make clear that detection of synchrotron emission from outer disks or halos is already important to learn about magnetic fields, even if no polarisation can be detected. Computing magnetic field strengths needs information about CRE energy losses, to be derived from radio spectra. New chapters are needed on: · Irregular and blue compact galaxies, interacting galaxies, galaxy groups Authors: Chris Chyzy, Marek Urbanik · Investigate small-scale magnetic fields by Faraday depolarisation Authors: Andrew Fletcher, Paul Alexander, ... · Simulations of small-scale and large-scale magnetic fields in galaxies, Faraday depolarisation, and synthetic RM data cubes Authors: JЖrn GeisbЭsch, Jongsoo Kim, Andrew Fletcher, ... The topic of magnetic fields in intergalactic filaments still needs discussion. Search for individual candidates (e.g. galaxy groups or select from optical galaxy surveys) or go for statistical detection? (Discussion group: Paul Alexander, Ger de Bruyn, Chris Chyzy, ...) 2. Galaxy sample Actual sample includes 54 galaxies. Detection of pol and RM from extended disks and halos needs more than 100h integration per galaxy which will be possible only for a subsample -> strategy to choose best cases is needed, to be done within the Working Group. Criteria: · Surface brightness · Radio spectrum · Inclination · Rotation velocity · Star-formation rate · Strength of warp · Degree of interaction · Galactic latitude (piggyback observing requested by the Milky Way Working Group)


3. Use Case / Commissioning Plan Needs to be written within next months by a small team (C.Chyzy, G.Heald, J.Anderson, R. Beck), preferably in Bonn. Important question: Do we need ~10" resolution to detect extended pol, or can we smooth to ~30" in order to gain sensitivity? -> Simulations of Faraday DP is needed. (JЖrn GeisbЭsch?) 4. Joint observations with the Survey KSP The MKSP needs spectral information about nearby galaxies from the SKSP surveys to choose best cases for deep integrations, and to determine magnetic field strengths (taking into account CRE losses). The Survey KSP plans pointed observations at ~210 MHz of about 60 nearby galaxies with about 9h integration time each. The present list has 384 galaxies, selection by discussions between the SKSP and the MSKP (C.Chyzy is the moderator). The Survey KSP does not plan deep observations of nearby galaxies. This has to be done by the MKSP. Results will useful also for the SKSP, e.g. for the search for radio SNs and SNRs. 5. Observations with other telescopes Observations between the LOFAR wavelength range and the GHz range of the Effelsberg, VLA and ATCA telescopes are needed. The Cambridge group (D.Green) has a running project on nearby galaxies at 610 MHz at the GMRT (including pol) which are important for the MKSP. Another GMRT source survey project of the Cambridge group (with Calgary) will be important to estimate the density of polarised sources at low frequencies, as needed for RM grids. At 350 MHz, theWSRT will only available for another ~2 years. A few projects on nearby galaxies are running (M31, IC342, NGC6946, NGC891), but more projects should be performed, especially on edge-on galaxies. PhD student urgently needed. 6. Other items The expected time allocated for the MKSP is by far too small to reach the goals. Political action is required.

Rainer Beck