Projects
It is a custom build telescope  located in Cerro Toco in Chile, to measure CMB fluctuations with arcminute resolution and noise of 1 micro k per pixel.  Beyond measuring the CMB primordial  power spectrum the instrument is designed to study the secondary effects such as thermal SZ, kinetic SZ, CMB lensing , OV, Rees-Sciama,  etc. Click HERE for more information of the projects I am interested in.
NSF founded collaboration under the program for international research and collaboration between Princeton, UPenn, Rutgers, University of KwaZulu-Natal  in South Africa and Universidad Pontificia Catolica de Chile. The aim is to enable multi-national observational program to survey the ACT sky region in multiple frequency.  
ADEPT is a space mission that conducts a high precision galaxy redshift survey out to redshift of z=2.0, the largest effective volume survey of the universe, by far. The goal of the project is to  constrain Dark Energy. On one side the mission will measure Baryonic acoustic oscillations (BAO) to trace the angular diameter distance and  the Hubble parameters as a function of redshift. During the course of its survey, ADEPT will discover about 1000 SNe up to z=1,3, which will be re-observed to follow their light curves. Thus, ADEPT will fully harvest the supernovae in this redshift range to the expected calibration and systematic limits. The baryon acoustic oscillations measure distances relative to the cosmic microwave background, while the supernovae measure relative to the here and now. Therefore, the overlap between the ADEPT supernovae and baryon acoustic oscillation measurements ties together the entire distance scale, while the reliable and precise baryon acoustic oscillation measurements provide a cross-check on the accuracy of the SNe measurements.
PAU-BAO  is a robotic 2.5m with 40 narrow-band filters designed to measure baryonic acoustic oscillations with spectroscopic precision in the redshift range 0.1 < z < 0.9.  The telescope will be located in the Javalambre mountain (Teruel) in Spain and will start observations around 2009.