... Phase Correction Algorithms | ... This page describes work undertaken at the Cavendish Astrophysics Group , developing phase correction algorithms and software for the Atacama Large Millimetre Array (ALMA). Without correction, phase fluctuations, mainly arising from the water content of the atmosphere, would limit ALMA's performance . ... The following people are currently involved in the phase calibration workpackage, based at the Cavendish Astrophysics Group in the University of Cambridge : . ...

XMM-Newton Science Analysis System . rmfgen (rmfgen-1.55) [xmmsas_20060628_1801-7.0.0] . ... rmfgen spectrumset=spectrum.ds rmfset=myresp.rmf detmaptype=flat . and supplying an image to give the ultimate accuracy by: . rmfgen spectrumset=spectrum.ds rmfset=myresp.rmf detmaptype=dataset detmaparray=myimage.ds . NB: The image supplied MUST be in detector and NOT sky (X/Y) coordinates. XMM-Newton SOC/SSC -- 2006-06-28 ...

... Date : 30/06/2014 . ... Celestron Super C8 Plus . 2 occulaires + renvoi coudГї + pare buГїe celestron + trГїpied + carton de rangements/transport avec compartiments de protection en mousse. Le tout en trГЕs bon Гїtat, n'a pas ГїtГї utilisГї depuis 5 ans. Remise en mains propres Г Boulogne Billancourt ou Paris 16ГЕme. PossibilitГї d'Гїchange contre un tГїlescope plus petit + diffГїrence en espГЕces. ... Prix : в'ѓ650 . ... M. FrГїdГїric FrГїdГїric Saurin . Paris ...

... public class EDM . ... Euclidean Distance Map: The value of each pixel is the distance to the nearest background pixel (for background pixels, the EDM is 0) - Ultimate Eroded Points (UEPs) are maxima of the EDM. ... static int . ... Unit in old make16bitEDM: this pixel value corresponds to a distance of one pixel. static int . ... int . ... For compatibility with previous versions of ImageJ only. public FloatProcessor makeFloatEDM ( ImageProcessor ip, int backgroundValue, boolean edgesAreBackground)...

. Computer Ephemeris. Lunar physical observations. Explanations. Each row contains at 0h of Time Dynamical Terrestrial: month, day, selenographic longitude and latitude of the Earth (degrees), physical libration in longitude and latitude (degrees), 90 o minus selenographic longitude of the Sun and Sun's selenographic latitude (degrees), position angle of lunar axis of rotation (degrees), position angle of terminator (degrees), phase angle (degrees), illuminated part of lunar disk (demensionless).

... About ATMoB . ... Events . ... Located in Westford, MA, less than an hour's drive from Boston. The clubhouse is maintained for members, but any non-member may visit with a member or by other prior arrangement (see the Contact Us page). The clubhouse is located on the grounds of MIT's Millstone farmhouse in Westford, MA. ... View sky above the clubhouse. ... Upcoming Clubhouse Events.. ... About the Club . ... ATMoB Club House . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

This module provides for user authentication using MD5 Digest Authentication. Status: Experimental . ... Module Identifier: digest_auth_module . Compatibility: Available in Apache 1.3.8 and later. ... If you use this module, you must make sure to not use mod_digest (because they share some of the same configuration directives). ... Note: Digest authentication is more secure than Basic authentication, but only works with supporting browsers. ... Module: mod_auth_digest . ...

... The solar regions . ... The description of the solar regions . ... The fine bipolar sunspots were observed at the mid latuitudes of the Northern hemisphere since 22.09 to 24.09, to the West of the Sun disc. ... The high latitude bipolar sunspots which were observing in the Northern hemisphere since 24.02 to 26.02 near the central meridian. ... The bipolar sunspot's cloud was observing at the middle latitudes of the Northern hemisphere since 13.05 to 20.05 in the West part of the Sun disc. ...

Next: The Evolution of Stars Up: NICMOS Science Previous: A Coronagraphic Search for . ... The NICMOS Parallel program . ... The Stellar Population . ... NICMOS Camera 3 is being used in parallel mode to observe galactic fields at both high and low galactic latitudes. ... Most of the fields are at high galactic latitude; as Figure 1 shows, only 8 pointings are within |b| = 10 o , i.e. the galactic disk. Figure 1: NICMOS parallel fields distribution in galactic latitude. ... Figure 6 ). ...

GENERAL INFORMA T ION ABOUT How does my LOMO® Night Vision Device Work? ... LOMO® NIGHT VISION DEVICES & FAQs When using a Night Vision Device, you are actually looking at an image that is projected by the intensifier tube located inside the unit (Fig. ... Light enters the Night Vision Device through the objective lens and hits the photocathode in front of the intensifier tube. ... Infrared (IR) Illuminator Microchannel Plate (Gen.2 Only) When do I use my LOMO® Night Vision Device? ... Fig. ...

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Winer Observatory gratefully acknowledges the generous support of those listed below. ... We thank our donors and hold them up as models of how corporations in America can behave responsibly in the communities in which they do business. ... Telescopes, parts, and accessories . ... 100,000 . ... Hughes Missile Systems . ... Miscellaneous electronics . ... Terra Universal, Inc. ... EFI Electronics Corp. ... 2013 Winer Observatory. ...

... LINKS . ... SPECIAL TOPIC . CONTACT . ... ARTICLE: Venus Transit 2004 . ... AAL's Transit Observation Results . ... Divx video from the AAL observation site. ... a) Visual observation : Only with special eclipse shades ( do not use those ones you still have from the 1999's solar eclipse because it does no more protect you properly ) . ... 1. contact ( transit begins ) : 07:19 53 s with a solar altitude of 15.5 degrees . ... Venus Transit Links: . ... Venus Transit 2004: A Tremendous Success . ...

J/AstL/vol/page SAI Open Clusters Catalog (Glushkova+, 2009) ================================================================================ Automated search for star clusters in large multiband surveys. ... Color excesses E(B-V), distance moduli and ages were determined for 141 new and 27 known, but poorly studied clusters. We present the Sternberg Astronomical Institute Open Clusters Catalog (SAI OCL Catalog) of coordinates, diameters and main physical parameters of these clusters. ...