In the upper part of the province frost occurs as late as mid-May. ... It ascends the east bank of the Rio Grande through pleasant groves of cottonwoods. ...
CMB/WMAP geometry of universe seeds of cosmic structure from BB. Relies on NRAO/CDL HEMT Amplifiers. Realm of the Galaxies. T_univ = 13.6 Gyr. HST/CO Wilson et al ...
10's 100's galaxies per night. Slit positions pre-set based on optical/submm/radio/Xray imaging ... Selection with 1.4 GHz imaging gets 50% to 75% at 10's ...
Need multiobject spectrograph for unbiased search for CO, other molecules in ... Submm gals: Dz_phot ~ 0.2 = ~2 GHz/source. Potentially trade-off of slits' for ...
Greg Taylor. What is polarized light? What fun science can be done with polarimetry? ... See Review of 'Cluster Magnetic Fields' by Carilli & Taylor 2002 (ARA&A) ...
into the operations of the Global ALMA project and North American ALMA Science Center ... Andrew Blain, Caltech. Crystal Brogan, U. Hawaii/NRAO. Chris Carilli, NRAO ...
Dick Hunstead, Elaine Sadler, Julia Bryant, Helen Johnston, Jess ... e.g. Kurk et al. 2000, Venemans et al. 2002, 2004 Miley et al. 2004. Proto-cluster Masses ...
... CfA Paul Ho, CfA Doug Johnstone, NRC Canada Lee Mundy, U. Maryland Joan Najita, NOAO Jean Turner, UCLA Jonathan Williams, ... U.C.-Berkeley Min Yun, ...
Local ioniz. ... Cross correlation in channels, or 3D power spectrum ... Enrichment of heavy elements, dust starts early (z 8): good news for radio astronomy ...
Reionization: the movie. 8Mpc comoving. Constraint I: Gunn-Peterson Effect. Fan et al 2006 ... Twilight zone': study of first light limited to near-IR to radio l's ...
... the first. luminous structures. Dark Ages. Twilight Zone ... Reionization: the movie. 8Mpc comoving. Barkana and Loeb 2001. Constraint I: Gunn-Peterson Effect ...
Comparable SFR at high z in dusty starbursts ('submm gal') as ... Optical phot z. Radio phot z: (1 z) propto T_D. 20K. 60K. Z_rad, Z_opt(2) Z_opt (1) COSBO 7 ...
Challenge: Low frequency foreground hot, confused sky. HI 21cm signal ~ 10 mK ... Focus: Reionization (power spec,CSS,abs) Very wide field: single dipole screen ...
Assumption 4: Radiation from astronomical sources is not spatially coherent. for R1 R2 ... Write the unit vector as: Write the observed intensity as: Replace ...
Reviewed by EMT/ISAC and revised 2003. China KARST. Canada LAR. US Large-N Small-D ... Full Xcorr inner 2300 ants (35 km), outer stations' of 13 ants ...
Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon Molecular Gas Mass as traced by CO emission and the star ...
Europe. China. Strawman. Level 1 Science. Notes: Level-1 science may still be missing. ... Temperatures: Spin, CMB, Kinetic and the 21cm signal. Initially T_S= T_CMB ...
Lisa Young. This lecture: things you need to think about before you observe ... L. Young, Synthesis Imaging Summer School, 19 June 2002. 16. Doppler Tracking: ...
What is the reionization history? Constrain the neutral fraction at z~ 6.3 ... 3 SDSS quasars (z=6.2-6.4) that show a 'depth effect' to the Lya absorption (Fan ...
Collaborators : B. Cl ment (LAM), P. Hibon (KIAS) J.Willis (Univ. Victoria), C. ... as the change in the far-UV LF is much milder. Data for z=6.5 : ...
We believe we are over the hump' in tracking down reliability and performance issues. ... Dry atmosphere. Referenced pointing. Short baselines (preferred) ...
Tenth Summer Synthesis Imaging Workshop. University of New ... Brighten and deflect. Gomez et al. 2000. 26. Where Most X-rays & ?-rays Are Emitted. clouds ...
Lecture 3 The role of stars in AGN Evidence for stars in the nuclear regions of type-2 AGN Photoionization models for starbursts Type IIn supernovae: variability
Obscured galaxy formation: high redshift (Downes et al 2002; Dunlop et al 2003) Single Scuba galaxy dominates SFR at z 2 in HDF over 10000 optical galaxies! ...
Hydrogen in a distant galaxy. Billions of galaxies! Large Scale Structure ... Cosmology, Galaxy Formation and Astroparticle Physics on the pathway to the SKA, ...
X-ray cavity measurements show energy is available to balance cooling in cluster ... their environments (e.g. Morganti 1988, Killeen et al. 1988, Feretti et al. 1990, ...
AGN Feedback deposits large amounts of energy influencing the evolution of ... (Overzier, Venemans, Kurk, Miley, de Breuk, van Breugel, Maschietto, van Breugel, ...
... case. Epoch of Reionisation with LOFAR. LOFAR extragalactic surveys ... Deepest extragalactic radio surveys. 2p sr at 15,30,60,120,200MHz to unparalleled depths ...