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. ...

... Up: Science Data Pipelines . ... The Chandra Automatic Data Processing System (AP) requires quick access to previously generated data. ... This archive interface layer includes an archive request queue, a data archiving server (darch), and an archive ``cache''. ... In our implementation, the cache is actually a directory where the data files reside, as shown in Figure 1 . ... If the data products are not in the cache, then the pipeline retrieves the files from the archive database. ...

Sternberg Astronomical Institute, Moscow University The idea behind this project 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. ... search through file/directory names, descriptions and README files; . ... The current goal of FTPdig project is to build University-wide network of ftp servers unified by the same interface and database. ...

... HST . ... Instructions on how to retrieve reference files . ... Data . ... The retrieval of Reference Files is a little more complicated than retrieving HST data. ... Reference Files are retrieved via the HST Archive site as follows: . In the form enter only the first nine characters of the file name followed by an asterisk. ... Override the retrieval options: In the Retrieval Options window next to your Archive username and password go to the bottom of the "Retrieval Options" window. ...

... Then you need to set the environment variable tpool to point to the directory you intend to unload the data into. As a safety precaution when you are getting data off tape you should run disk_master , it needs sc_td as a command line argument in this case. ... The tape number it requires is the nrst number (usually 0) and typically you will want to unload all systems with no clipping, no skipping and to create a summary file. ... Back to the Filterbank data reduction page. ...

Organization of the Data Processing in the Interball Project. ... Interball Data Archive contains data produced during Interball mission: raw data, data files produced by express-analysys and preprocessing systems, orbit and attitude data files, key physical parameters, Magion-4,5 subsatellites data files and other types of data. Express-analysys data is available for Interball participants within 1 day after telemetry session, level 1 processed data - within 2 weeks. ... Attitude data files . ...

... Parent Directory - drift.jpg 2009-11-04 18:24 82K m42 _10sx2.png 2007-02-24 01:55 9.0M m42 _10sx2_log.jpg 2007-02-24 01:59 55K m42 _10sx2_log.png 2007-02-24 02:00 690K m42 _10sx2_log_masked.jpg 2007-02-24 02:06 45K m42 _10sx2_log_masked.png 2007-02-24 02:05 292K m42 _19.jpg 2009-11-04 18:24 22K m42 _19_stellar_profile.jpg 2009-11-04 18:24 86K m42 _rvb_log.jpg 2009-09-22 10:42 109K ...

The FITS archive & data processing pipelines . HyperLeda home | ... The goal of the HyperLeda FITS archive project (HFA) is to gather data (in the FITS format ) and to document them in a manner that allow an automatic pipeline processing. ... The archived data are broad band images (BBI), long-slit spectra (LSS) and extracted spectra (SPE) plus their associated template and calibration files. ... The Library of Medium Resolution Spectra of Galaxies (ie. resolution = 1000 to 3000) . ... HyperLeda . ...

... Archives . ... Quote of the Week, Aug 23, 2007 . Aug 22nd, 2007| 08:55 pm | ... An Isochrone Database and a Rapid Model for Stellar Population Synthesis by Li and Han . This paper emphasize the binary population: CMD fitting with the binary population synthetic model outperformed to the single population model. ... They fitted their isochrone database to M67 and NGC 1868 with the gT-grid and concluded that the database of binary stellar populations fitted the color magnitude diagrams better. ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

... Public . Science . ... Science Users Information > Observing with ESO Telescopes > Observing Tools and Services > Archives and Catalogues . ... Public Surveys . Publications with ESO Data . ... Large Programmes . ... Public Surveys Programmes . ... The following Archives and Catalogues can be helpful for proposal preparation and for preparing an observing run. ... For a comprehensive overview of the on-line ESO/ST-ECF archives and catalogues please refer to the Science Archive Facility . ...

... The ISO post­mission archive (PMA) is being designed to fully ex­ ploit this legacy by providing access to the data across the Internet. It will provide an on­line service to the data, supporting documentation and software through a WWW interface which has the goals of being friendly for the novice user, flexible for the expert and rapid for everybody. ... Archived product or OFRP The ISO Post­Mission Archive 441 BROWSE FORM RESULTS FORM SHOPPING BASKET USER REGISTRATION RETRIEVAL FORM Figure 3. ...

... Description of e-Mail Commands . Abstract and Paper preparation for Put . ... Physics hep-th @ xxx.lanl.gov High Energy Physics - Theory, 8/91 hep-lat @ xxx.lanl.gov High Energy Physics - Lattice, 2/92 hep-ph @ xxx.lanl.gov High Energy Physics - Phenomenology, 3/92 cond-mat @ xxx.lanl.gov Condensed Matter, 4/92 astro-ph @ xxx.lanl.gov Astrophysics, 4/92 gr-qc @ xxx.lanl.gov General Relativity Quantum Cosmology, 7/92 nucl-th @ xxx.lanl.gov Nuclear Theory, 10/92 chem-ph @ ...

OptInt PmWiki . Pm Wiki / . Edit Page | ... MROI Delay Line Design Contract . ... AP local page . ... Backup and Restore . ... Your wiki installation contains some unique data in the following directories: . local/ Local configuration scripts cookbook/ Recipes obtained from the Cookbook pub/ Publicly accessible files wiki.d/ Wiki pages uploads/ Uploaded files (attachments) . A good backup plan will include periodically archiving these directories or at bare minimum local/ and wiki.d/ . ...

. Name . Last modified . Size . Description . Parent Directory . - . astronomy_calendar/ . 2004-03-06 16:10 . - . etudes_about_scientists/ . 2001-12-24 15:21 . - . fire_enthusiasts/ . 2001-12-20 21:24 . - . galaxies/ . 2002-11-22 13:50 . - . making_telescope_at_home/ . 2001-12-20 21:07 . - . return_from_space/ . 2001-08-29 13:13 . - . telescopes_for_amateur_astronomers/ . 2001-01-09 11:45 . - .

RTT150 . ... HEAD IKI . This page is a search interface through RTT150 observationsdatabase which is stored at IKI. According to the agreement between participantsof RTT150 project, observational data fully belong to the institution which hascarried out this observation for one year, are available to all three partiesinvolved (IKI, KSU and TUG) during the second year and become freely accessibleto the whole astronomical community starting two years after observation date. ...

... Panchuk V.E. Database "Stellar Spectra" consists of following main units: . ... obtained with various modifications of high resolution echelle-spectrometers at the 6-m telescope. ... Using the spectra obtained at BTA in combination with high resolution echelle-spectrometers LYNX and PFES , Chentsov E.L., Klochkova V.G. and Panchuk V.E. prepare now the next spectral atlas. ... The CATALOGUE of spectral photoplates obtained at the Main Stellar Spectrograph of the 6m telescope. ...

... Display (spectra, total power). ... Using the data archive. ... entering cmds, editing cmd lines, input from files, batch, run. constants, variables,arrays, structures, operators, procedures, functions. programming in idl . ... A user would call arch_gettbl() to input the table (or a subset of it). corfindpat() can create subsets of the table. arch_getdata() or arch_getonoff() can be used to read in the spectra. ... input the data (spectra) for a subset of the archive table: arch_getdata () . ...

. To create an archive file use the command: tar cvf tarfile_name .tar filenames ( directory_name ) . The command options cvf modify the way the tar command works. See the manual page for details. By convention the name of a tarfile archive ends in .tar . When you create a tarfile of a directory all the subdirectories are added; this can result in very large tarfiles. These should be compressed to reduce their size. Tip ... Examples .

Zeiss-1000 "Sky140" TV-camera current JPEG-image and FITS -file [ Click here to reload with images icons ] . ch3_0.jpeg . ...