. XMM-Newton Science Analysis System . dataconv (sas-1.443) [xmmsas_20050815_1803-6.5.0] . Meta Index / Home Page / Dataset structure / Images / ExposureMap . Exposure maps are also products [ 2 ]. XMM-Newton SOC/SSC -- 2005-08-15

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• Node-specific Exposure Maps

As it was already mentioned, the idea behind File Juggler is rather simple: using CGI scripts as processing tools and WWW browser as user interface, display the structure and content of typical anonymous FTP server in a convenient, easily navigated form. ... My P5-133 spends about 0.025 ms on one file when doing linear search with simple criterion (690 ms for 27,000 files, search for substring among file names/descriptions with 70 hits). ... Let's now look whether we can handle 1,000,000 files. ...

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• Historical Notes
• RELATED WORK
• INTRODUCTION

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• Simulation of HST PSFs using Tiny Tim

2.1 Data Files and Suffixes . 2.2 Header Keywords . 2.3 Correlating Phase II Exposures with Data Files . 2.4 WFPC2 Paper Products . ... This chapter describes how WFPC2 data are configured and delivered and how these data products relate to the original specifications in the Phase II proposal. We describe the data format used by STScI to distribute WFPC2 observations and the meanings of the header keywords that the user is likely to find most important. ...

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• The Hubble Deep Field -- data products
• CALWF3 Release Notes
• STSDAS Version 3.10 Release Notes

20feb07 The calibration scans (see ao technical memo 2000-04 ) does two crosses (each leg 6 beam widths long) about a source. ... This model is used below to create beam maps at various azimuths, zenith angles, and frequencies. ... They are the output of the model. ... Single beam map (.ps) ( .pdf ) : This one is easier to see. Beam maps before transit (.ps) ( .pdf ). 6 beams per page. Beam maps after transit (.ps) ( .pdf ). 6 beams per page. processing: x101/070219/lbwbeammaps.pro home_~phil ...

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• http://www.naic.edu/~phil/usrproj/bs116b/jun03.html
• H I Midplane Poster for the 201st Meeting of the AAS, January, 2003
• Slide 11

... 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. ...

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• correlator:archiving [ATNF VLBI Wiki]
• correlator:records:v486g [ATNF VLBI Wiki]
• correlator:records:v277b [ATNF VLBI Wiki]

Deep Depletion of Charge Coupled Devices . ... Fibre Optic Coupling to CCDs . The MTF of CCD Sensors . ... Radiation Damage Effects in EEV CCDs . ... Initial Assessment of Low Noise Readout Techniques for High Speed CCD Image Sensors . CCD Performance Limitations Theory and Practice . ... Scientific Type CCDs: Summary of Performance Limits . ... For copies of these papers click on the contact button below: . This page last changed 19th June 1998. http://www.ccd.eev.com . 1998 EEV Ltd. ...

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• Product Folder: TC213, 1024- X 512-PIXEL CCD IMAGE SENSOR
• Product Folder(Obsolete): TC215, 1024- X 1024-PIXEL CCD IMAGE SENSOR
• CCD Technical Note

... OOF . ALMA . ... OOF Index . Zernike Polys . GBT example . ... Observed data and analysis . The observed beam maps are shown in the first row of the table below. ... We show the best-fitting aperture and the best-fitting beams as the number of Zernike orders used for the fitting is increased. A sample OOF observed data set (top row) and the results of analysis with increasing number of Zernike polynomials used to parameterise the aperture. ... In-focus beam . ... Observed beams . ...

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• Getting NVSS data products by FTP
• VLBI observations of the quasar 3C380
• A prototype build system for CASA using SCons Bojan Nikolic web pages (r. 329)

... Summary of reduced ISAAC fields . ... This data release includes eight fully reduced VLT/ISAAC fields in J,H,K s bands covering 50 arcmin 2 of the GOODS region in the Chandra Deep Field South (CDFS). ... 8 ISAAC fields) . ... The 8 ISAAC fields which are part of this data release are superimposed onto a SOFI image (J+K) (part of a previous EIS data release). ... In one case (GOODS field 11/J-band), for which not enough standard stars were available, the ZP was boostrapped from previous SOFI/EIS data...

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• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
• Celestial scribbled notes | ESO
• Feeding the Monster | ESO

Next: Model Spectra for Spectral-Fitting Up: Spectral Analysis Previous: A Quick Look at . ... For ROSAT PSPC data, this conversion is done during the on-line (SASS) processing. For IPC observations, the instrument gain varies both across the detector and in time, and is applied during off-line processing (PROS) using the BAL histogram. By default, spectra are extracted in PI bins for PSPC data and in PHA bins for IPC data. ... Special techniques are required when using Einstein IPC data. ...

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• The AstroStat Slog Blog Archive On-line Machine Learning Lectures and Notes
• Model Spectra for Spectral-Fitting Program
• The AstroStat Slog lecture note

. Ceilidh Notes 1 --- Introduction . Ceilidh Notes 2 --- Basics . Ceilidh Notes 3 --- If and Switch . Ceilidh Notes 4 --- Loops . Ceilidh Notes 5 --- Array and structures . Ceilidh Notes 6 --- Pointers . Ceilidh Notes 7 --- Functions . Ceilidh Notes 8 --- File I/O . Ceilidh Notes 9 --- Process management . Ceilidh Notes 10 --- Questionaire . Dave.Marshall@cm.cf.ac.uk . Wed Sep 14 10:06:31 BST 1994

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• Further Data Types
• How Ceilidh works, Ceilidh Course Notes, User Guides etc.
• Low Level Operators and Bit Fields

The general structure of our network at SAI main buiding. ... MSU main campus map (Moscow, Leninskie gory). Upgrade. I did not encountered any troubles with upgrade. ... See a few upgrade notes for details. sendmail-8.7.3 for Solaris 2.5. ... See my sendmail installation page if you want a little assistance. ... See our patch installation history. inn1.4unoff4. ... Linux and DAT streamer (Usage and recommendations for Zeus). ... Gated and Linux 2.2.x (Compilation and installation). ...

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• APOD: 2003 September 12 - A Note on the Perseus Cluster
• Zen: Search for: "FTS Notes"
• The Name of the Plug-In: Notes

The course will start on Tuesday 29th April 2008 and end on Friday 6th June 2008. Lectures" will be held on Tuesdays 2-3pm and Fridays on Fridays, 9.30-10.30 and 11.00 - 12.00. ... This will not be a conventional lecture course: it is intended to be far more hands-on and practical. Notes will be posted ahead of each lecture and everyone will be expected to have read and digested them ahead of each lecture. ... Statistics Notes: Part 1 . ... Radio Astronomy Notes: Part 1 , Part 1 . ...

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• Clearing the front offices. Note the collapsed wall.
• Tea room floor. Note the unusual construction.
• Clearing the north-south hallway. Note the large fallen concrete lintel.

.

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• FAQ: "Exploration of the Earth's Magnetosphere"

... The axial support is provided by 78 air pistons. ... The transverse support is provided by 38 air pistons, supported by cantilevers from the mirror cell, that act on the mirror local center of gravity surface. ... The locations where the transverse mirror support forces should be applied to the mirror are listed in Table 1 and illustrated in Figure 1. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of the transverse support posts (black) and axial pneumatic pistons (blue...

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• Index of /arc35m/Instruments/_notes
• _notes
• Large Capacity Archival Data Storage

... Лекция 2 (40 K) | Лекция 3 (37K) | Лекция 4 (39K) | Лекция 5 (43K) | Лекция 6 (47K) | Лекция 7 (32K) | Лекция 8 (54K) | Лекция 9 (41K) | Лекция 10 (45K) | Лекция 11 (38K) | Лекция 12 (44K) | ... Postscript-файл (36 K) | ... Алгоритмическая сложность и класс P . ... Вероятностное вычисление и класс BPP . ... Идея квантового вычисления. ... Определение и простейшие свойства квантового вычисления. ... Вычисление, устойчивое к ошибкам (классическое и квантовое). ...

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• Combinatorial structures in topology (Fall 1998)
• Books (Latin z)
• Books (Latin x)

... Астронет | ... update: 9 October 2002 . ... Basic data: . ... HD 37124 b . ... 00: From astrometry Han et al (2000) claim a preliminary mass of 119 M J and inclination of 179.5 o . ... Seven New Keck Planets Orbiting G K Dwarfs. ApJ. , submitted . ... A Dynamical Analysis of the HD 37124 Planetary System. ... The Stability Analysis of the HD 82943 and HD 37124 Planetary Systems. ... Global dynamics and stability limits for planetary systems around HD 12661, HD 38529, HD 37124 and HD 160691. ...

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• Астронет > Notes for HD 82943
• Астронет > Notes for epsilon Eridani
• Астронет > Notes for HD 160691

... It is a simple 1 X finder scope that mounts to almost any telescope. ... It projects three red circles into space, allowing you to center the scope on bright stars or planets. ... In many cases it is the only finder scope you'll need. (in bright city skies, it will be more difficult to use). Place the Telrad circles between the bright stars shown around the Messier object you wish to view, and with you widest field eyepiece (usually the lowest power) you should find the Messier Object very easily. ...

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... Building subroutine libraries . ... This was particularly useful for providing global variables through COMMON blocks. ... Therefore there is a distintion between private COMMON (seen only by the subroutine library) and global COMMON, but this is a semantic distinction only. ... The distinction between private and global variables remains, but, in principle, there is a more legitiamte way to export "global" varaibles from a subroutine library than simply making the INCLUDE file globally visible. ...

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• Taurid swarm years
• Armagh Observatory
• Press Release: International Collaroration led by Armagh Astronomers

... Most HTML elements are identified in a document as a start tag, which gives the element name and attributes, followed by the content, followed by the end tag. ... To identify the document as being HTML 3.0, it is recommended that documents start with the prologue: <!doctype HTML public "-//W3O//DTD W3 HTML 3.0//EN"> . ... HTML 3.0 documents formally have the following structure: <HTML> <HEAD> head elements .. ... HTML> . ... The permitted syntax of HTML 3.0 compliant documents is specified by the...

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• The Body Element and Related Elements
• Admonishments
• The IMG (Image) Element