... We have defined a set of rules for classifying SUSI exposures according to the exposure type (BIAS, FF, SCI) and a set of rules for classifying them according to the optical path. ... The MIDAS session shown in Table creates these rules and applies them to our set of SUSI exposures (Table ). The result of the classification process is illustrated in Table . ... The table must contain the following columns: . ... Table: Classification Table for SUSI exposures (susi_rule.tbl) . ...

Program: GETVAL Purpose: Get image values at given positions in a set Category: UTILITY File: getval.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (,subset): Maximum number of subsets is 1. ... The image values are formatted according the string entered in FORMAT= APPEND= Ok to append? ... The flag characters and their meanings are: - The result of the conversion is left- justified within the field. ... If the result of a conversion is longer than the field width, an asterisk is returned. ...

... Meta Index / Home Page It is a good idea to do some checking of the output- the following are recommended: . Use fv to view each product image and display the detected sources on the image by selecting the corresponding region file . ... Use fv to inspect each product source-list file . Create a region file from the combined source-list file using the task slconv , and then use fv to view a mosaiced image and display the sources by selecting the region file. ...

This is a library of galaxy spectra computed by Bruzual and Charlot using their Isochrone Synthesis Spectral Evolutionary Code. The December 1995 version of the Bruzual-Charlot atlas consists of 21 instantaneous bursts characterized by different IMF slope functions, and mass limits. Each instantaneous burst contains 221 spectral energy distributions (SEDs) corresponding to 221 time steps from 0 to 20 Gyr. ... Spectra for instantaneous and composite bursts are available. ...

This section contains information of how user agents should treat control characters and other special characters. ... There are 256 character positions in the Latin-1 encoding. ... It consists of the space character, 186 characters that form a subset of the graphic characters in ISO 6937/2 (1983), and four additional characters that are intended for inclusion in ISO 6937/2. ... Certain characters are taken to have special meaning within the context of an HTML document. ...

If necessary, the observations and corresponding O ? C values belonging to some observatory can be separated from the other data. Besides, O ? C satisfying some conditions imposed on their value can be separated. ... To separate O ? C by value, mark O ? C check box and enter positive numbers limiting absolute values of O ? C from above or from bottom or both and click on Run . ... The restrictions imposed on observatory code and on O ? C values are indicated in status bar. ...

... The main goal here was to check whether some new bug fixes were correctly implemented (See corresponding Release Note), but mostly if P2PP correctly works with the new CCS MARCH2001 on HP-UX 11. ... Import/export OBs. ... A lot of time was spent a verifying the "synchronise" bug (item 1246). ... No critical bug found in this beta1, only 2 High and 3 Minor bugs which are to be solved AFTER MARCH2001 (next V2.1.x, if any, or V2.2). ... MINOR. ... MINOR: to be fixed in V2.2 (item 1271). ...

... 2007 June 2 . 3D Full Moon . ... Explanation: Get out your red/blue glasses and check out this satisfying stereo anaglyph of the Full Moon. ... Regardless of your preferred technique for stereo viewing , the 3D effect comes from combining pictures of the same scene taken at different angles -- mimicking the slightly different perspective of each eye. Perhaps surprisingly for Earthdwellers , getting two pictures of the Full Moon from different angles only requires a little patience. ...

... 3D Full Moon . ... M65 is a big, beautiful spiral galaxy, the sixty-fifth object in the famous astronomical catalog compiled by 18th century cosmic tourist Charles Messier. ... Dwarf Galaxies in the Coma Cluster . ... In visible light images, over a thousand galaxies are seen to lie within a volume about 20 million light-years across in the rich Coma Galaxy Cluster. ... The Hubble Space Telescope has resolved individual stars in a spectacular new image of nearby spiral galaxy M81. ...

... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

... Corresponding authors will receive an e-mail with a PDF file of paged proof for checking and correction. The file can be read and edited using Adobe Acrobat Reader (version 9 and higher) which can be free downloaded via the Internet ( http://get.adobe.c om/reader/ ). ... You can use text correction tools to make corrections (after selecting the necessary text fragment). ... For users of Adobe Reader 9: . ... to insert text without replacing the existing text, use the "Insert text at cursor" tool. ...

In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

... A simple Virasoro vertex algebra is rational (and -2 semisimple as well) iff its central charge is of the form c = 1 - 6(pppp ) , where p, p are relatively prime integers, greater than 1 (which are central charges of the so called minimal models). A simple affine vertex algebra Vk (g), attached to a simple Lie algebra g is rational (and semisimple as well) iff its level k is a non-negative integer. ... We call such f an exceptional nilpotent and such k an exceptional level. ...

The FSP3 event includes those parts of the magnetic conjugations between any couple of four considered spacecraft, which satisfied to the FSP1 or to the FSP2 criterion. ... The value of the relative geocentric angular distance between magnetic field line's footprints is considered during FSP3 situation selection. The mentioned angular distance value less then 5 deg is used as a criterion of the magnetic conjugation. ... for the first SC the red color and the first line are used, . ...

... include <string.h> . char *stpcpy ( char *dest, char *src) - Copy one string into another. int strcmp( char * string1 , char * string2 ) - Compare string1 and string2 to determine alphabetic order. char *strcpy( char * string1 , char * string2 ) - Copy string2 to stringl. char *strerror( int errnum) - Get error message corresponding to specified error number. int strlen( ...

... The MIDAS Data Organizer, a customizable utility to analyze and identify associations in a database of astronomical observations, is described. ... On-line Data Reduction: . ... The main characteristics of the on-line implementation of the DO at the ESO New Technology Telescope (NTT) are described below. The database for all operations is a MIDAS (ESO-IPG 1993) table, the so-called Observation Summary Table (OST) which contains all relevant parameters extracted from the FITS keywords. ...

... NIC-FPS is an instrument combining the capabilities of a near-infrared imaging camera with a cryogenic Fabry-Perot etalon currently under development at the Center for Space Astrophysics and Space Astronomy , University of Colorado with support from Rice University , Ball Aerospace and the Astrophysical Research Consortium. It is scheduled to begin operations on the ARC 3.5m telescope at Apache Point Observatory in 2004. ... For full frame images, the FITS file will result in a size of: . ...

... the 8 deg by 8 degree map around coma (.gif) . the beam map (.gif) : . the uv map of the data (.gif) : . ... Zero extend the beam map to 168 by 167 pixels to match the dimensions of the data map. ... The line plot at the bottom of the image is a horizontal cut through the center of the map. ... The bottom image is the uv amplitudes of the beam map. ... Page 1 bottom uv map of beam : the vertical scale in in db's. Page 2 top Cuts through uv data map : where u=0 (green) and v=0 (black). ...

AMM, 81 (1974) 490: THE DERIVATIVE SONG Words by Tom Lehrer -- Tune: "There'll be Some Changes Made" You take a function of x and you call it y, Take any x-nought that you care to try, You make a little change and call it delta x, The corresponding change in y is what you find nex', And then you take the quotient and now carefully Send delta x to zero, and I think you'll see That what the limit gives us, if our work all checks, Is what we call dy/dx, It's just dy/dx.

... This report provides background information about the Armagh Observatory and a summary of the Observatory's principal achievements in research and other areas during the reporting period, which is the Calendar Year 2002. ... Calendar Year . ... 66,000 . ... 134,000 . ... Apart from maintaining the level and quality of astronomical research carried out at the Observatory, the key task for the year is to continue to work with the DCAL to widen the Observatory's access to research development funds. ...