Dates	Location	Travel Information	Event
29 November - 3 December 2005	Socorro, NM	Nov 29 5:23 PM  - 6:36 PM Denver to Albuquerque Dec 3 1:12 PM - 2:24 PM Albuquerque to Denver	Visit to NRAO AOC
2 December	Los Cruces, NM		Talk at NMSU "Cosmology at 1 and 2 mm" http://astronomy.nmsu.edu/nicole/colloquia/home.html The advent of broadband bolometer cameras in the 1 and 2 mm windows with resolution < 1 arcmin allows the study of two important classes of cosmological objects.  The 1 mm band is primarily sensitive to dusty, high-redshift, star-forming galaxies and / or AGN (the so-called submillimeter galaxies), whose redshift distribution likely peaks at z ~ 2.5.  The 2 mm band is primarily sensitive to Sunyaev-Zel'dovich galaxy clusters, whose redshift distribution is not well known, but is believed to peak at around z ~ 0.4.  In this talk, I will discuss placing both of these classes of objects in their cosmological context by combining them with deep, multiwavelength surveys which can help constrain their redshift distribution, environment, and relation to the dark matter potential.  I will take as my specific example recent Bolocam results from the COSMOS survey.
12 - 16 January	Charlottesville, VA	United 720 Jan 12 6:15 AM - 11:29 AM Denver to Dulles United 5219 Jan 12 12:57 PM - 1:46 PM Dulles to Charlottesville United 5241 Jan 16  7:41 PM - 8:33 PM Charlottesville to Dulles United 933 Jan 16 9:35 PM - 11:26 PM Dulles to Denver	NRAO ALMA Workshop "From ALMA to Z-Machines: (sub)millimeter Spectroscopy of Galaxies" http://zmachines.net/
27 January	Boulder, CO		JILA Lunch talk "Submillimeter Galaxies in Cosmological Context" http://rocinante.colorado.edu/~seminar/ The class of submillimeter luminous, high redshift, massively star forming galaxies first implied by the discovery of the cosmic far-infrared background and discovered with SCUBA represent a significant population in the history of star-formation in the universe.  The space density of these objects is quite high, and the most massive of them are consistent with baryonic assemblies of >10^11 M_solar.  As such, they are interesting probes of hierarchical structure formation theories.  While 100's of galaxies have been detected in (sub)millimeter surveys, until now placing them in a cosmological context has been hampered by lack of precise redshifts, crude mass estimates, and the limited co-moving volume probed in surveys.  Here we consider how these limitations can be overcome in current and future data sets, and focus for specific examples on our work in the 2-square degree HST-COSMOS field.
28 January - 21 February	CSO, Mauna Kea, HI	United 739 Jan 28 6:00 AM - 7:39 AM Denver to San Francisco United 53 Jan 28 8:35 AM - 12:15 PM San Francisco to Kona Island Air 1458 Jan 28 5:10 PM - 5:40 PM Kona to Hilo United 4959 Feb 21 8:10 PM - 8:57 PM Hilo to Honolulu Feb 21 11:05 PM - Feb 22 8:46 AM Honolulu to Denver	Observing with Bolocam and SHARC II. CSO Schedule
2 - 6 March	Columbus, GA	Mar  2 UA # 448  DEN --> ATL   6:45 pm 11:32 pm Mar  6 UA # 873  ATL --> DEN   7:29 am 8:53 am	My baby sister is getting married
26 - 31 March	Venezia, Italia	Mar 24 UA # 440  DEN --> IAD   11:23 am  4:40 pm Mar 24 UA # 916  IAD --> FRA   5:17 pm  7:10 am (Next day) Mar 25 Lufthansa 9078  FRA --> VCE   8:40 am  9:55 am	IVSLA Conference "Galaxies and Structures Through Cosmic Times: Mapping the Universe" http://dipastro.pd.astro.it/venice06/
2 - 3 April	Asiago, Italia	Apr  4 Lufthansa 9058  VCE --> FRA   10:50 am  12:20 pm Apr  4 Lufthansa 8827  FRA --> IAD   1:20 pm  3:50 pm Apr  4 UA # 903  IAD --> DEN   5:30 pm 7:25 pm	COSMOS All Hands Meeting http://dipastro.pd.astro.it/COSMOS-As/
5 - 20 April	CSO, Mauna Kea, HI		Observing with Z-Spec
27 - 28 April	Socorro, NM		2006 Jansky Fellow Symposium
6 - 24 June	CSO, Mauna Kea, HI		Observing with Bolocam and SHARC II