(r10) CosmoProjects < Cosmo

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---+ Boud's To Do list
   * mbr04 - z amr
   * isolat - pixelisation CMB - boud
   * H0 - bartek
   * dodec II - all
   * 2QZ - Gary et Yohan
   * roots of S^3 - boud

---+ CosmoTopology
   * WMAP - identified circles - MonographCosmo
      * AstroPh:0402608
      * http://adjani.astro.uni.torun.pl/twiki/pub/Cosmo/CosmoProjects/dodec-aa.ps
   * RLAGNs larger catalogue/histograms -  Boud, Andrzej M, Staszek - mrb04
   * (RLAGNs morphologies - Boud, Andrzej M, Staszek, Motyl?)
   * root of the identity in the spherical case -  Boud
   * (nested crystallography - Boud)

   * WikipediaPl:Reklama
      * OswiadczeniePrasoweDodekahedron
      * MonographCosmo

---+ CosmoCurvature (standard ruler)
 
   * new standard ruler stuff with 2QZ -  Gary, Yohan, Boud, 
      * - http://www.astro.uni.torun.pl/sympa/shape-univ/2002-05/  etc.
      * - http://www.astro.uni.torun.pl/~boud/DE/
   * curvature + other parameters from CMB - Micha&#179; F + Bartek(?) + Boud
      * - http://www.archeops.org - 12% of sky observed with Planck instruments is now publicly available :)


---+ Hubble Constant 
   * Bartek Lew is doing great stuff on this, and Michał Chodorowski has submitted a nice derivation: AstroPh:0407478

---+ NonBaryonicDarkMatter

   * Bartek Lew is working on this: NonBaryonicDarkMatter

---+ GalaxyAGNFormation

   * modelling 
      *  - ArFus project - N-body (gravity) + semi-analytical (gas cooling, star formation) - Boud + others - 
   * observations
      *  - Blazars - Radek
      *  - Mrk 421, Mrk 501 BL Lac objects  - [monitoring of the variability], [modeling of multifrequency emission of blazars] - Krzysztof
      *  - evolution of radio galaxy populations + hybrid object - Motyl + ...
      *  - young RLAGNs - Andrzej M + Magda
      *  - OneCmRA - Sebastian + Andrzej K + Motyl ...

   * CAMK-Torun is involved in the HerschelSatellite infrared telescope 
project which should be launched around 2007 and has 
      *  instruments such as
      *  - PACS 50-200 &#956;m
      *  - SPIRE 200-600 &#956;m - spectro + bolometric
      *  - HIFI 100-600 &#956;m - star formation, H<sub>2</sub>0
      *  - these should provide observations of galaxies at quite high redshifts,
so good galaxy/AGN formation modelling projects could make predictions of
how the HerschelSatellite observations could constrain interesting galaxy
formation questions
      *  - there was a HerschelStarFormationEvolution meeting on this at TCfA Torun on 15 Nov 2002 at Piwnicach

Topic attachments
I	Attachment	Action	Size	Date	Who	Comment
ps	dodec-aa.ps	manage	1274.6 K	17 May 2004 - 14:55	BoudRoukema	revised after referee's comments - single-spaced

Topic revision: r10 - 12 Aug 2004, BoudRoukema

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