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Carnegie Hubble Program

Carnegie Hubble Program. A mid-infrared recalibration of the extragalactic distance scale. Carnegie Hubble Program. Wendy Freedman (PI) Eric Persson , Mark Seibert Vicky Scowcroft, Andy Monson Laura Sturch , Jane Rigby. Basic Cepheid Light Curves Properties. Ceph.

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Carnegie Hubble Program

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  1. Carnegie Hubble Program A mid-infrared recalibration of the extragalactic distance scale

  2. Carnegie Hubble Program Wendy Freedman (PI) Eric Persson, Mark Seibert Vicky Scowcroft, Andy Monson Laura Sturch, Jane Rigby

  3. Basic Cepheid Light Curves Properties Ceph “Ontology recapitulates Phylogeny” Ernst Haeckel (1838-1919) said that.

  4. Carnegie Hubble Program (Persson et al. 2004, AJ,128, 2239) Ceph

  5. LMC Mid-IR/Spitzer Cepheid Light Curves Scowcroft et al. (2011), ApJ, 743,76 Cephei

  6. Carnegie Hubble Program (Persson et al. 2004, AJ,128, 2239) Cepheid Va

  7. Carnegie Hubble Program (Freedman et al. 2012) Cepheid Variables

  8. H = 74 km/s/Mpc  Four Neutrinos

  9. Dominance of AGB Stars in Mid-IR

  10. IC 1613 at 3.6 microns

  11. Carbon stars dominating NGC 4258

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