HARP is the Heterodyne Array Receiver Programme for the James Clerk Maxwell Telescope.
The programme is beginning with HARP-B,
a 16-element Heterodyne Array Receiver to operate at B-band (325-375 GHz).

NEWS
February 2006	Frontiers press release
December 2005	HARP achieves first light. More details on the public web pages.
The HARP-B project is a collaboration between  Cavendish Astrophysics (MRAO) at the University of Cambridge, UK, The Joint Astronomy Centre at Hilo in Hawaii (operators of the JCMT), The UK Astronomy Technology Centre at the Royal Observatory Edinburgh, The Herzberg Institute of Astrophysics of the National Research Council Canada SIS junctions designed by MRAO were fabricated under contract by The TU Delft Institute of Microelectronics and Silicon Technology (DIMES)
Restricted web pages. These are password protected.	FDR documents.  Project Staff only	Acceptance test documents. Project and JACH staff only