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5421. Home Page for the ASSIST
The ASSIST implements a uniform graphical interface to software and information for the X Window System. ... 1996, E. Mandel and M. S. Ackerman, The ASSIST: Unified Management of Public and Private Information , published in Astronomical Data Analysis Software and Systems V (ed. George H. Jacoby and Jeannette Barnes) . 1996, E. Mandel and M. S. Ackerman, The ASSIST: Bringing Software and Information Together for Scientists , published in Science Information Systems Newsletter, issue 13 ) ...
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Ссылки http://hea-www.harvard.edu/RD/assist/index.html -- 2.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/assist/ -- 2.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/assist/index.html -- 2.9 Кб -- 01.10.2012
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/assist/ -- 2.9 Кб -- 01.10.2012
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5422. The galaxy M100
An image of the grand design of spiral galaxy M100 obtained with NASA's Hubble Space Telescope resolves individual stars within the majestic spiral arms. ... Hubble has the ability to resolve individual stars in other galaxies and measure accurately the light from very faint stars. This makes space telescope invaluable for identifying a rare class of pulsating stars, called Cepheid Variable stars embedded within M100's spiral arms. ... 617) 495-7062 . Fax: (617) 495-7356 . ...
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Ссылки http://hea-www.harvard.edu/~juda/ism/m100.html -- 4.5 Кб -- 01.10.2012
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5423. Known SAOtng bugs and limitations
The following bug and limitations are known. Please send new bug reports, comments, suggestions to: saotng@head-cfa.harvard.edu: . ... When the raw data is being transferred to SAOtng by the external file access program, the GUI performance can slow down noticeably. When a cursor shape is changed (e.g. from circle to rectangle) using the (Button 3) marker menu inside the cursor, the button press actions inside the cursor become confused. ... This causes problems with discrete colormaps. ...
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Ссылки http://hea-www.harvard.edu/RD/saotng/bugs.html -- 3.2 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/saotng/bugs.html -- 3.2 Кб -- 01.10.2012
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5424. Converting the XPA API to 2.0
This document describes tips for converting from xpa 1.0 (Xt-based xpa) to xpa 2.0 (socket-based xpa). ... The changes are straight-forward and almost can be done automatically (we used editor macros for most of the conversion). ... Also change first 2 arguments from XtPointer to void *. ... Change NewXPACommand() to XPAcmdNew(), with the new calling sequence: xpa = NewXPACommand(toplevel, NULL, prefix, NULL); is changed to: xpa = XPACmdNew(xclass, name); . ... Go to XPA Help Index ...
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Ссылки http://hea-www.harvard.edu/RD/xpa/convert.html -- 4.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/xpa/convert.html -- 4.9 Кб -- 01.10.2012
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5425. Changes For Users from XPA 1.0 and 2.0
This document describes changes that will affect users who migrate from XPA 1.0 to XPA 2.0. There have been a few changes that affect users who upgrade XPA from version 1.0 to version 2.0. ... For the SAOtng program, this means that you must explicitly specify the access point, i.e.,: cat foo.fits | xpaset SAOtng fits . ... xpaset SAOtng . By default, xpaset, xpaget, etc. now wait for the server callback to complete; i.e., the old -W is implied (and the switch is ignored). ...
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Ссылки http://hea-www.harvard.edu/RD/xpa/changes.html -- 2.8 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/xpa/changes.html -- 2.8 Кб -- 01.10.2012
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5426. Welcome to the SAOtng Help Facility
SAOtng is the new and improved version of the popular SAOimage display program. ... SAOtng supports direct display of IRAF images and FITS images (and easily can support other file formats), multiple frame buffers, region/cursor manipulation, several scale algorithms, many colormaps, and easy communication with external analysis tasks. ... FITS Primary Images . FITS Image Extensions . FITS 3D Images . ... The Images Menu . ... Adding New Accelerator Buttons . Adding New Analysis Routines . ...
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Ссылки http://hea-www.harvard.edu/RD/saotng/help.html -- 5.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/saotng/help.html -- 5.9 Кб -- 01.10.2012
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5427. Editing Text
Next: Listing and Printing Files, Up: Using IRAF Previous: Parameters . Editing text on the screen . The history of recent commands can be edited using the command ehist. ... The editor is set in the login.cl file or in the loginuser.cl file. cl > ehist # Calls the last command # and leaves you in the editor # <cr> executes the command once you have edited it. cl > ehist imcnts # calls for editing (as above) the most recent # command beginning with ``imcnts''. ... Moving text on the screen . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node9.html -- 5.5 Кб -- 01.10.2012
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5428. Parameters
... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node8.html -- 5.0 Кб -- 01.10.2012
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5429. Help
... A help command is provided. cl > help pros will give an overview of useful help tasks and files in the PROS/XRAY packages. cl > help package-name will give one line of explanation for each of its tasks or packages. cl > help task-name will give detailed information about that task. ... Lists tasks and subpackages of the current package cl > ?? Lists all tasks and subpackages currently loaded cl > bye # Unloads the current package, returning to the previous one . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node7.html -- 3.7 Кб -- 01.10.2012
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5430. Using IRAF
Next: Help Up: IRAF/PROS Previous: Bringing up IRAF . A comprehensive introduction to the IRAF system can be found in A Users Introduction to the IRAF Command Language . ... To list the available commands, type ? ... To run a command or load a package, type its name. Type `bye' to exit a package, or `logout' to get out of the CL. ... The system is composed of `packages', each itself composed of packages and commands (`tasks'). ... Packages can be unloaded by typing bye . ... Help . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node6.html -- 7.3 Кб -- 01.10.2012
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5431. Bringing up IRAF
... 1. create a user directory from which IRAF will be run (called `myiraf' in these examples). This will contain the user set-up specifications and other IRAF-related subdirectories. 2. create an image directory in a disk partition where there is enough space to contain large files (image arrays). ... This creates a file ( login.cl ) which executes the set-up each time a new IRAF session is started. mkiraf should be run every time there is a new release of IRAF. ... edit the login.cl file. ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node5.html -- 6.1 Кб -- 01.10.2012
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5432. Summary of Tasks in this Section
Next: Bringing up IRAF Up: IRAF/PROS Previous: IRAF/PROS . Task . ... Package Needed . list contents of current package . list contents of all loaded packages . ... language* . ... edit last command . ... edit parameter file . ... edit image file headers . ... display help file for specific task or package . ... list parameters for specific task . ... list packages loaded . ... edit .qp file headers . ... Next: Bringing up IRAF Up: IRAF/PROS Previous: IRAF/PROS rsdc@cfa.harvard.edu . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node4.html -- 6.8 Кб -- 01.10.2012
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5433. IRAF/PROS
... The Post-Reduction Off-line Software (PROS) is a portable x-ray analysis software system designed to run under NOAO's Image Reduction and Analysis Facility (IRAF). The PROS system provides IRAF users with tasks that will properly access the x-ray data. ... Similarly many IRAF tasks will be useful for x-ray data. ... The IRAF system, previous to the development of the PROS software, provided many of the features needed to analyze generic astronomical data, optical data in particular. ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node3.html -- 7.9 Кб -- 01.10.2012
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5434. General Introduction
Next: IRAF/PROS Up: PROS USERS GUIDE Previous: Contents . This guide is designed to aid the new user in deriving scientific results from reduced x-ray data using the SAO PROS software system which runs under IRAF as package ``xray". ... If you are using the IRAF/PROS system at SAO, you will find the siteguide , by Belinda Wilkes, a useful guide to site-specific procedures. ... Spatial analysis . ... Next: IRAF/PROS Up: PROS USERS GUIDE Previous: Contents rsdc@cfa.harvard.edu . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node2.html -- 7.3 Кб -- 01.10.2012
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5435. Contents
Next: General Introduction Up: PROS USERS GUIDE Previous: PROS USERS GUIDE . ... Summary of Tasks in this Section . ... IRAF/PROS Files . ... DATA I/O . ... ROSAT data and PROS . ... QPOE Utilities . Summary of Tasks in this section . qpcopy* - Manipulation of PROS/IRAF data files . ... qpsort* -- Sort a QPOE file . ... qprotate* -- Rotate a QPOE image about the origin . ... qpappend* -- Append a list of input qpoes to produce a single qpoe file . ... Image Display . ... Spectral Analysis . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node1.html -- 10.9 Кб -- 01.10.2012
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5436. http://hea-www.harvard.edu/~pgreen/SOC/9.html
... The Chandra COSMOS Survey 2. ... Evidence that Compton-thick and Compton-thin obscured AGN have two physically different origins on different scales are presented and the implications for surveys and AGN evolution are discussed. oral . Monday: Type I and II AGN, Absorption, XBONGs, Tuesday: AGN correlation functions, LSS, environments . ... Monday: X-ray luminosity functions and evolution, Tuesday: AGN correlation functions, LSS, environments . ...
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Ссылки http://hea-www.harvard.edu/~pgreen/SOC/9.html -- 6.4 Кб -- 01.10.2012
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5437. http://hea-www.harvard.edu/~pgreen/SOC/7.html
... Monday: Type I and II AGN, Absorption, XBONGs, Tuesday: AGN correlation functions, LSS, environments . ... The AGN content of the COSMOS: the XMM-Newton view . The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS) is expected to be an important step forward in the study of the physics and evolution of AGN, especially for what concern high redshift obscured quasars. ... Monday: X-ray luminosity functions and evolution, Tuesday: AGN correlation functions, LSS, environments . ...
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Ссылки http://hea-www.harvard.edu/~pgreen/SOC/7.html -- 6.5 Кб -- 01.10.2012
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5438. http://hea-www.harvard.edu/~pgreen/SOC/5.html
... Chandra Observation of DEEP2 Galaxy Groups and Clusters . ... Monday: 'Normal' Galaxies, Tuesday: Cluster Formation and Evolution . ... Statistics of galaxy groups in ultradeep XMM surveys. ... What can multiwavelength observations tell about cluster/group formation as well as galaxy evolution? ... I will present results from a Chandra study of eight low-redshift clusters that has systematically measured the AGN fraction in clusters and describe their spatial, kinematic, and host galaxy...
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Ссылки http://hea-www.harvard.edu/~pgreen/SOC/5.html -- 10.7 Кб -- 01.10.2012
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5439. http://hea-www.harvard.edu/~pgreen/SOC/4.html
... Clustering of AGN and QSOs at z=1 . Using galaxies from the DEEP2 Redshift Survey and AGN from the AEGIS/Chandra survey and QSOs from SDSS, I present the cross-correlation function of AGN/QSOs and 'normal' galaxies at z=1. Using the known clustering of DEEP2 galaxies, this leads to an estimate of the bias and typical host dark matter halo mass of AGN/QSOs as a function of X-ray luminosity, which constrains AGN formation models. oral . ... Tuesday: AGN correlation functions, LSS, environments . ...
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Ссылки http://hea-www.harvard.edu/~pgreen/SOC/4.html -- 9.0 Кб -- 01.10.2012
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5440. http://hea-www.harvard.edu/~pgreen/SOC/2.html
... This sample outnumbers previous medium X-ray surveys. ... Preliminary results confirm the presence of Fe-K emission in the stacked X-ray spectra of obscured and unobscured AGN. oral . ... Monday: Type I and II AGN, Absorption, XBONGs, Tuesday: AGN correlation functions, LSS, environments . ... Monday: Type I and II AGN, Absorption, XBONGs, Tuesday: Cluster Formation and Evolution . ... XBONGS in the XBootes Field . ... Monday: Type I and II AGN, Absorption, XBONGs, Tuesday: Groups and Interactions ....
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Ссылки http://hea-www.harvard.edu/~pgreen/SOC/2.html -- 15.3 Кб -- 01.10.2012
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