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Date: 2008-01-03 11:37:57 Space plasmas Large-scale structure of the cosmos Star formation Radio telescopes Submillimeter Array Submillimetre astronomy Galaxy Cosmic distance ladder Cooling flow Astronomy Space Extragalactic astronomy		Add to Reading List Source URL: www.cfa.harvard.edu Download Document from Source Website File Size: 1,13 MB Share Document on Facebook

	SMA Newsletter Submillimeter Array Newsletter CONTENTS 1 DocID: 1rjJH - View Document
	VDIF EDV 0x02 The Atacama Large Millimeter/submillimeter Array (ALMA) will support VLBI through the addition of so-called Phasing Interface Cards (PICs) inserted into the baseline (BL) observatory correlator to produce p DocID: 1qFOi - View Document
	Credit: C.Padilla - ALMA (ESO/NAOJ/NRAO) Atacama Large Millimeter/submillimeter Array At the operations site of the ALMA antenna array, located on the Chajnantor Plateau (which in the original Atacameño language —Kun DocID: 1nChF - View Document
	Credit: C.Padilla - ALMA (ESO/NAOJ/NRAO) Atacama Large Millimeter/submillimeter Array Depending on what part of the Universe you want to observe, the ALMA antennas —which weight more than 100 tons each— can be moved DocID: 1n0SO - View Document
	The Astrophysical Journal, 695:59–74, 2009 April 10 Cdoi:637X DocID: 18MG6 - View Document