From nss@space.mit.edu Thu Mar 13 16:19:08 1997 Received: from space.mit.edu by wiwaxia AA21036; Thu, 13 Mar 97 16:19:07 EST Received: by space.mit.edu AA21215; Thu, 13 Mar 97 16:19:05 EST From: Norbert Schulz Subject: xrcfdata To: crc@space.mit.edu (Claude Canizares), dd@space.mit.edu (Dan Dewey), dph@space.mit.edu (Dave Hunnemoerder), wise@space.mit.edu (Mike Wise), hermanm@space.mit.edu (Herman Marshall), jhk@space.mit.edu (Joel Kastner), dsd@space.mit.edu (Dave Davis), davis@space.mit.edu (John Davis), kaf@space.mit.edu (Kathryn Flanagan), baluta@space.mit.edu, houck@space.mit.edu (John Houck) Date: Thu, 13 Mar 97 16:19:05 EST X-Mailer: ELM [version 2.3 PL11] Status: R Folks, All ACIS-2C phase 2/F eventlists and related data are on disk now. The disk is here at MIT on space.mit.edu The data are in '/starburst/d2/aqlc1' for days 970218 to 970303 and '/starburst/d2/aqlc2' for days 970304 to 970311 Since I did the backup on /bulk/aqlc on mashine AQLC2 on XRCF 2nd floor I also copied a lot of low byte trash with it. I cleaned some, but not all of it. The data*.fits files in /starburst/d2/aqlc1 are example bias.files for all ccds and window modes. File data_F-I2C-RC-72.002s5.0104.fits is something for everybody to take home and frame. File fam_positions.dat in /starburst/d2/aqlc2 are the actual FAM positions during the sub-pixel tests. How to find data: EXAMPLE: 'ls /starburst/d2/aqlc1/970221' lists "FOO FOOBAR R-I2C-PI-9.006 R-I2C-PI-9.006A catalog.gz ftp.txt.gz" Forget about everything that doesn't look like a TRW-ID, which leaves two directories, " R-I2C-PI-9.006 R-I2C-PI-9.006A" The one with an "A" is usually a repeat at a later time with different input parameters 'ls /starburst/d2/aqlc1/970221/R-I2C-PI-9.006' lists an index_file, which cats all the event list names (used by the PSU quicklook) the avarage bias file (R-I2C-PI-9.006s1_bias_avg.fits.gz), and a data directories named after all the used sequence numbers, which in this case are s1 and s2 and s101, *.1 to *.6 belong to a single run but were hacked during processing. s2 and s101 are new data aquisitions after either aborting or extending s1 'ls /starburst/d2/aqlc1/970221/R-I2C-PI-9.006/s1.1' finally lists "R-I2C-PI-9.006s1.1_evts.fits.gz R-I2C-PI-9.006s1.1_hk.fits.gz R-I2C-PI-9.006s1.1_oc_stat.dat.gz" the actual data. The scientific data are in R-I2C-PI-9.006s1.1_evts.fits. PLEASE: If you don't use the PSU quicklook software, copy the eventlists onto a disk of your choice, it better not be one of mine, and THEN mess around as you wish, ok! Have fun, Norbert From nss@starburst.mit.edu Tue Jul 15 15:29:28 1997 Received: from space.mit.edu by wiwaxia AA06733; Tue, 15 Jul 97 15:29:26 EDT Received: from starburst.mit.edu by space.mit.edu AA24370; Tue, 15 Jul 97 15:29:19 EDT Received: (from nss@localhost) by starburst.mit.edu id PAA01959; Tue, 15 Jul 1997 15:29:18 -0400 (EDT) From: Norbert Schulz Message-Id: <199707151929.PAA01959@starburst.mit.edu> Subject: xrcfdata To: crc@starburst.mit.edu (Claude Canizares), dd@starburst.mit.edu (Dan Dewey), dph@starburst.mit.edu (Dave Hunnemoerder), wise@starburst.mit.edu (Mike Wise), hermanm@starburst.mit.edu (Herman Marshall), jhk@starburst.mit.edu (Joel Kastner), dsd@starburst.mit.edu (Dave Davis), davis@starburst.mit.edu (John Davis), kaf@starburst.mit.edu (Kathryn Flanagan), baluta@starburst.mit.edu (Chris Baluta), houck@starburst.mit.edu (John Houck) Date: Tue, 15 Jul 1997 15:29:18 -0400 (EDT) X-Mailer: ELM [version 2.4ME+ PL25 (25)] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII Content-Transfer-Encoding: 7bit Status: R Hi Folks, I updated the xrcf data archive on /starburst for MIT/ASC: all ACIS-2C and HST data are on /starburst/d2 aqlc1 and aqlc2 are the ACIS-2C data that already existed before PHASE_G are all ACIS-2C data from the mid-April run PHASE_H are all ACIS HST data from the ACIS flight testing PHASE_Hr are the reprocessed phase H HST data (updated as reprocessing continues) all ACIS flight telemetry data are on /starburst/d3 mcc1 - 4 currently contain erv-/arv-/.qdp formatted telemetry data of all the science runs in phase H. Currently the runs are NOT yet broken up into single test IDs. During time I will try to break all the science runs into single test IDs and have the arv-format converted into the L1-output format. Since this is a short cut to overcome the tele-decom problems at SAO for the time being, we may not do this conversion for all data sets but the ones of immediate interest. I can't promise any time scale to get the conversion done, but in case there is immediate need to look at telemetry data, I will find a way to look at them at request. Joel also knows, how to deal with arv-formats. have fun, Norbert