. The first ALMA antenna to be handed over to the observatory, pictured here at the ALMA Operations Support Facility. This state-of-the-art 12 m diameter antenna was manufactured by Mitsubishi Electric Corporation. ALMA (ESO/NAOJ/NRAO)
Astronomical Data Analysis Software and Systems XII ASP Conference Series, Vol. 295, 2003 H. E. Payne, R. I. Jedrzejewski, and R. N. Hook, eds. The Subaru Telescop e Software Trinity System R. Ogasawara, G. Kosugi, T. Takata, J. Noumaru, T. Sasaki Subaru Telescope, NAOJ, 650 N. Aohoku Pl., ... It consists of the Subaru Observation Software System, the Subaru Telescope Archive System, and the Data Analysis System Hierarchy. ... To archive all data. ... References Iye, M. 1998, in SPIE Proc., Vol. ...
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Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/O4-4.pdf -- 105.7 Кб -- 11.03.2003 Похожие документы
# # List of USB ID's # # Maintained by Stephen J. Gowdy <sgowdy+usb.ids@gmail.com> # If you have any new entries, send them to the maintainer. # Send entries as patches (diff -u old new). # The latest version can be obtained from # http://www.linux-usb.org/usb.ids # # $Id: usb.ids,v 1.374 2009/01/10 08:11:02 gowdy Exp $ # # Vendors, devices and interfaces. Please keep sorted. # Syntax: # vendor vendor_name # device device_name <-- single tab # interface interface_name <-- two tabs 0001 Fry's Electronics
-91405, Orsay Cedex, France June 30, 2004 Abstract Currently, it appears that the best method for non-Gaussianity detection in the Cosmic Microwave Background ( CMB ) consists in calculating the kurtosis of the wavelet coefficients ... Max (Mn ). ... It has been shown [44] that it is also possible to separate the nonGaussian signatures associated with cosmic strings from those due to SZ effect by combining the excess kurtosis derived from these both the curvelet and the wavelet transform. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/EURASIP-Paper.pdf -- 1245.1 Кб -- 22.09.2005 Похожие документы
The HR Diagram and the Galactic distance scale after Hipparcos I. Neill Reid Palomar Observatory, 105н24, California Institute of Technology, Pasadena, CA 91125, eнmail: inr@astro.caltech.edu ABSTRACT The completion and publication of the Hipparcos astrometric catalogue has revitalised studies in many fundamental areas of Galactic structure and stellar evolution. This article reviews the impact of the new parallax results on our understanding of the location of the mainнsequence as a function of abundance,