... These Frontier Fields will combine the power of HST with the natural gravitational telescopes of high-magnification clusters of galaxies. ... We are soliciting gravitational lensing maps for the last four Hubble Frontier Fields clusters (MACSJ0717.5+3745, MACSJ1149.5+2223, AbellS1063, and Abell 370) based upon the exceptionally deep HST FF imaging and other new ancillary data. ... For the full set of proposal instructions and requirements, see the FY16 Frontier Fields Lensing Map Call for Proposals....

... Gooch, R.E., 1995, "Space and the Spaceball" , in Astronomical Data Analysis Software and Systems IV , ASP Conf. ... Gooch, R.E., 1995, "Visualisation: from Data to Understanding", in Workshop on Applications of Radio Science 1995 , Australian Academy of Science through the National Committee for Radio Science ISBN 1-86408-030-2 . Gooch, R.E., 1996, "Karma: a Visualisation Test-Bed" , in Astronomical Data Analysis Software and Systems V , ASP Conf. ...

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

... autoconf processes configure.in to produce a configure script. configure is a portable shell script which examines the build environment to determine which libraries are available, which features the platform has, where libraries and headers are located, and so on. Based on this information, it modifies compiler flags, generates makefiles, and/or outputs the file config.h with appropriate preprocessor symbols defined. ... Here is a sample configure.in , from a Gnome version of "Hello, World": . ...

Chapter 5. Listing of Installed Components . ... An X driver (/usr/X11R6/lib/modules/drivers/nvidia_drv.so); this driver is needed by the X server to use your NVIDIA hardware. ... An X module for wrapped software rendering (/usr/X11R6/lib/modules/libnvidia-wfb.so.x.y.z and optionally, /usr/X11R6/lib/modules/libwfb.so); this module is used by the X driver to perform software rendering on GeForce 8 series GPUs. ... See Chapter 4, Installing the NVIDIA Driver for a more thorough description. ...

... Public . Science . ... Science Users Information Science Software Common Pipeline Library jump to navigation jump to content . Science Users Information . ... Observing with ESO Telescopes . ... Publications with ESO Data . ... Large Programmes . ... Common Pipeline Library . ... The Common Pipeline Library (CPL) comprises a set of ISO-C libraries that provide a comprehensive, efficient and robust software toolkit to develop astronomical data-reduction tasks (known as "recipes"). ...

... Up: Archives and Information Services . Previous: The VizieR System for Accessing Astronomical Data . ... A data archive is near completion at the ASC to store and provide access to AXAF data. ... It consists of a number of different servers which handle flat data files, relational data, replication across multiple sites and the interface to the WWW. ... This paper presents the overall archive architecture and the design of client and server components as it was used during ground calibration. ...

... Obtaining the software . ... Building subroutine libraries . ... Building spectrum . ... Building sterne . ... Subroutine library index . ... Once you have obtained all of these and installed all of the subroutine libraries successfully, you can attempt to build it: . cd /home/friday/sterne; make; make install . ... Detailed reports describing bugs in the download/installation procedure or in the software itself will be welcome and should be addressed to Simon Jeffery at the address below. ...

. Moscow Astronomical Plate Archives: Contents, Digitization, Current and Possible Applications. Light Curves of New Variable Stars Discovered on Scans of Moscow Collection Plates, Field 66 Oph (MDV). MDV catalog - CDS access. Moscow plate collection (Sternberg Astronomical Institute), S.Yu. Shugarov's interactive page. Send questions and comments to N. Samus and S. Antipin .

... Module name: fftw_aux . ... This module is meant to be used in conjunction with the Fast Fourier Transform package fftw which comes with the sas. The module contains a header in which some useful variables are declared, as well as the following routine: . function findNextHighest2357multiple(i) result(result) integer, intent(in) :: i end function findNextHighest2357multiple . ... The fftw transform works most efficiently on arrays which have dimensions which are products of small primes. ...

O ptimal transport : T heory and A pplications . ... Names of participants of the OTARIE project are underlined . ... That code was never made public. ... WANN (Weighted Approximate Nearest Neighbors) is a library of C++ classes for weighted nearest neighbor search: given the set P of points p 1 , p 2 , , p N endowed with weights w 1 , w 2 , , w N and a query point q , find p k such that | ... WANN is part of a multipurpose library for numerical transport optimization developed in the OTARIE project. ...