Following are instructions to build and install the programs in this distribution. Make sure that you have all necessary tools for building executables. ... The automatic build process expects a configuration file called Config.local . ... The configuration file specifies the directory in which to install the binaries, as well as control over the generation of debugging code and reference clock support. ... Cleans out object files, programs and temporary files. make distclean . ...

... As of the 95NOV release, patch level 2.0, ESO-MIDAS is available under the GNU General Public License. The short statement of the GNU license is included in every MIDAS file; the full text is printed in the beginning of this manual and is included as a separate file in the ESO-MIDAS Release. ... All source code, documentation, as well as binary copies of ESO-MIDAS (already installed and without sources) for specific systems can be retrieved from the ESO-MIDAS anonymous ftp account. ...

XmCCD ----- The programs provided here offer a Linux graphical user interface to astronomical and scientific CCD cameras. ... It is the latest one they offer and the files included allow support for Android and Mac OS X. This distribution of XmCCD includes source code to utilize the SBIG shared library libsbigudrv.so with a Motif-based graphical user interface. ... The XmCCD source package includes and will install: SAOimage ds9 xpa cfitsio SAOimage is the primary image display for XmCCD. ...

The HyperNews Linux KHG Discussion Pages . ... Re : Kernel Makefile Configuration: how? ... Keywords: Makefile, configuration . ... From: Balaji Srinivasan < BalajiSrinivasan > . When you run make config (or its siblings) it creates a file in include/linux directory. This file (autoconf.h) is included in include/linux/config.h in all the required C files.. For the makefile the place that these config options are specified is in the .config file in the TOPLEVEL directory. ...

The binary distribution kits for livedata and gridzilla should include everything required to run them on compatible Linux, Solaris, and/or Darwin systems. ... VERSION date this release was generated. livedata_root.tar.bz2 (required) contains top-level files. livedata_linux.tar.bz2 contains linux binaries. livedata_linux64.tar.bz2 binaries for 64-bit linux systems. livedata_darwin.tar.bz2 contains Darwin (Mac OS X) Intel binaries. livedata_sun4sol.tar.bz2 contains Sun Solaris binaries. ...

ChangeLog for omthlcplot =============================== Version 1.3 - 2002-09-12 (NW) ------------------------------- Changed the keyword warning statement in the documentation to include the values of the HDUCLASS attributes, to close SPR-2973 (Wrong reference to data set attributes in doc). ... Version 1.2 - 2002-07-25 (NW) ------------------------------- Updated the DEPEND file. ... The test harness has been changed to be variable for Linux or Unix, because the environment variables are different. ...

To : Distribution From : Science Planning and Scheduling Team, STScI Date : 6-FEB-1997 17:34:55 UT SMS Supervisor : Martin England (410) 338-5005 Subject : SMS HS047B: distribution of final products The Mission Scheduler and Command Loader processing for the final run of SMS HS047B has been completed. ... This distribution includes MEGG and MOSR products in addition to MS/CL products. ... A ONE-FHST UPDATE WILL BE SUBSTITUTED FOR THE REQUESTED TWO-FHST 3-AXIS UPDATE This is expected and is acceptable. ...

home news . SEARCH ASP SITE: Match ALL words Match ANY word . ... Beginning in 2005, all conference proceedings published by the ASP Conference Series during 2004, and all future volumes, will include full text electronic access. ... Visit the e-Books site for select free preview volumes . ... Organizers of upcoming conferences who wish more information about publishing their proceedings through the ASP Conference Series should contact Interim Managing Editor J. Ward Moody at jmoody@byu.edu . ...

... Routines for accessing I/O ports are in /usr/include/asm/io.h (or linux/include/asm-i386/io.h in the kernel source distribution). ... Before you access any ports, you must give your program permission to do so. This is done by calling the ioperm() function (declared in unistd.h , and defined in the kernel) somewhere near the start of your program (before any I/O port accesses). ... For example, ioperm(0x300, 5, 1) would give access to ports 0x300 through 0x304 (a total of 5 ports). ...

The weight and positions for the objects on the rotary floor were obtained from ecastro on nov03 and used to plot the weight distribution on the rotary floor. ... The figure shows the weight distribution by turret position. ... Fig 1 top: Each object on the floor is plotted with its weight vs its turret position. Fig 1 middle: The weight is averaged by turret position quadrant to show the imbalance in weight distribution. ... The turret position is that of the receiver or read off of the drawing. ...

... Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. ... Redistribution and use of this software, with or without modification, is permitted provided that the following conditions are met: 1. ... All related source code must be included. ... Various other copyrights apply. ...

... Archives . ... Nov 7th, 2007| 11:57 am | Posted by hlee . Today?s arxiv-stat email included papers by Poetscher and Leeb, who have been working on post model selection inference. ... How you know your data are from chi-square distribution, or gamma distribution? (this is a model selection problem with nested models.) ... stat.TH:0702703] Can one estimate the conditional distribution of post-model-selection estimators? by H. Leeb and B. M. P\?{o}tscher . ... Chandra Blog . ...

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

Digital Unix Fortran Compiler + OSF/1: . All codes run satisfactorily on Digital/Compaq Alpha processors. ... All codes compile. ... All f77 codes compile. ... In f77 the INC|LUDE statement enabled the creation of common code that could be shared between subprogram units. ... My convention is to place INCLUDE files containing global COMMON variables in a defined folder in the software folder structure currently ./include (to be replaced by ./inc when I have debugged all the references). ...

lsst.coordConv љ unknown . ... Files . ... pvtCoord.h . ... 3 љ #include " coordConv/pvt.h " . ... 24 љ explicit PVTCoord ( Coord const &coord, Eigen::Vector3d const &vel, double tai); . ... 47 љ explicit PVTCoord ( PVT const &equatPVT, PVT const &polarPVT, PVT const &distPVT= PVT ()); . ... 63 љ explicit PVTCoord ( PVT const &equatPVT, PVT const &polarPVT, PVT const &distPVT, double equatPM, double polarPM, double radVel); . ... Definition: pvtCoord.cc:121 . ... Definition: pvtCoord.h:172 . ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

Chiaki Kobayashi, Ralph Sutherland How galaxies did form and evolution? - to answer this unsolved problem, we are simulating the formation and evolutionary history of galaxies in the Universe, including star formation, supernovae feedback, and chemical enrichment. Comparing the spacial distribution of elements within galaxies with observations, we will examine fundamental physical processes that drive galaxy formation. ... COALA : Universe Galaxy AGN Star Planet ...

... Files . include <stdio.h> . ... Include dependency graph for tmsolve.c: . dust_tmatrix . dust_mkBmatrix ( dust_tmatrix *tm) . ... dust_TMSolve ( dust_tmatrix *tm) . Calculate the energy bin probability distribution of a grain by solving transition matrix. void . ... dust_tmatrix dust_mkBmatrix . ... References dust_tmatrix::data , and dust_tmatrix::M . Referenced by dust_TMSolve() . ... References dust_tmatrix::data , dust_mkBmatrix() , dust_normalisepvect() , and dust_tmatrix::M . ...

... Up: Data Processing Systems . ... We demonstrate the latest Starlink software, including ORAC-DR pipelines, new Java applications, and distributed pipeline processing. ... An example of its use is the TOPCAT application ( http://www.starlink.ac.uk/topcat ), shown in part in Figure 2. ... Of course the final result can also provide estimates of errors and data quality, pixel by pixel, because the Starlink applications, Classic as well as the new ones, automatically keep track of these. ...