... Archives . ... People . ... The 2 Megasecond Chandra observations of the Southern Deep Field , which have been processed, reduced, and mosaiced. ... There are many more, I am sure, and if people find any particularly good ones, please point them out in the comments! ... Comment ( RSS ) | ... I haven?t had time to really study the data in the book, but I hope it useful. http://www.astro.ubc.ca/people/jvw/ASTROSTATS/index.html#chapter1 07-15-2008, 1:31 pm . ... Comments RSS . ... Chandra Blog . ...

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 . ...

Archive to extract from isn't specified . You are now in the [/] directory . [ Archive home | Shortcuts | Files | Directory tree | New files | Search | Help ] . Send your questions and comments . This software archive is being maintained by Sergey Ayukov . This HTML file was generated by FileJuggler package

... 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. ...

... 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 () . ...

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 . ...

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: . ...

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