... As with previous HST instruments, the FITS header keywords in STIS data files store important information characterizing the observations and telemetry received during the observations and describe the post-observation processing of your dataset. ... Calibration information such as the calibration switches and reference files used by the pipeline and parameters derived from the calibration, such as image statistics, wavelength shifts. ... Time: 0.3 sec Number of imsets: 3 . ... Dark image correction...

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• http://www.stsci.edu/documents/dhb/web/c17_nicdata.fm3.html
• NICMOS Data Handbook
• Chapter 12: Cosmic OriginsSpectrograph (COS)

Next: System configuration Up: How to use CONSTRICTOR Previous: Preparation of parameter file Contents . ... DayNumber: Even though this number is in the data, some packet headers have the wrong number and it makes it a whole lot easier to have the user check and enter this number correctly. ... CONSTRICTOR will add a multiple of 24 hours to the time tag when the day number changes. Remember to set the StopTime to, say, 48 hours if you use a DayNumber of one less than the actual day number. ...

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• SPECPSF (V1.00) --- May00 stecf.specres --- SPECPSF (V1.00)

Next: READBACK TESTS Up: Tape Management Previous: TAPE LENGTHS and PASS Contents . ... The Mark III and VLBA systems make longitudinal recordings using many heads, all mounted on a head stack. ... Modes with 2 heads are MarkIV only. ... Bit rate: 64 Mbps 128 Mbps 256 Mbps 17600 All/High 20:32:00 10:16:00 5:08:00 17600 VLBA/Low 12:19:12 6:09:36 3:04:48 17600 Mark III/IV/Low 12:09:52 6:04:56 3:02:28 8800 VLBA/Low 6:09:36 3:04:48 1:32:24 8800 Mark III/IV/Low 6:04:56 3:02:28 1:31:14 2 Pass/head pos. ...

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• TPMODE
• difx:ivs2016extras [ATNF VLBI Wiki]
• User Parameters - Data Location & Beam Selection CentralProcessor 0.11

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Tunable Kernel Parameters? . Re : Increasing number of files in system (Simon Cooper) . Keywords: kernel tuning, file handles, Bus error . Date: Sat, 25 Oct 1997 11:25:44 GMT . From: Simon Cooper < simon.cooper@snc-net.demon.co.uk > . Sorry for the typo, my (Linux loader) lilo.conf entries are: . image=/vmlinux.safe [Newline] label=LinuxS [Newline] root=/dev/hda2 [Newline] .

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• Increasing number of files in system
• Register_*dev() can assign an unused major number.
• Program parameters

... MODULE em_ frames _module Read the file names of frames files (input and output) and events file Opening of input auxiliary and events file Select CCD/node in auxiliary file Copy of input events file header keywords to output frames file parameters read : choice of sub_tasks to execute Loop over input task parameters Read the task parameter / 1 to perform the procedure, 0 not to perform it / End ...

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Next: Inspection of results Up: *fit* - Fit Data Previous: Verbose Mode . If the number of net counts for a source is less than it is impractical to fit the data in all 34 energy bits. However, if the flux is required, then a fit must be performed first. ... Fit will then calculate the normalization of the model and xflux can be used to determine the flux and luminosity of the source from the best fit model. xs> fit rebin=yes . ...

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• Jonathan's ASC/SDS documents
• Possible Pitfalls
• Produce a spectral data set using the PROS task 'xray.xspectral.qpspec'

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...

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• Converting Arecibo Interim Correlator data into a FITS image
• pulsars
• ATOMS by Number

From XEphem running the Soft03Cmt database of 20121002, for the date and time of the observation: RA: 08:16:04.25 Dec: 27:48:13 2012-09-30 UT 09:45 UTC Measured: RA: 08:16:04.4 Dec: 27:48:12.9 Header listing for HDU #1: SIMPLE = T / This is a FITS file BITPIX = -32 / NAXIS = 2 / NAXIS1 = 4341 / NUMBER OF ELEMENTS ALONG THIS AXIS NAXIS2 = 4355 / NUMBER OF ELEMENTS ALONG THIS AXIS EXTEND = T / This file may contain ...

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• http://www.astro.louisville.edu/shared_skies/archive/select/messier/m67/20110406/tmp/m67_4s_12800iso_1302145416.axy
• CurveFitter (ImageJ API)

There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...

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• Head Litter of Minor Planet Names

Next: INFO/WAVE Up: Commands Description Previous: RECONS/WAVE . HEADER/WAVE Wavelet . Gives information about a wavelet file and write them into keywords. ... OUTPUTI[1] = number of lines of the original image . OUTPUTI[2] = number of columns of the original image . OUTPUTI[3] = number of scales of the wavelet transform . OUTPUTI[4] = algorithm number . ... OUT_A = PYR, CUB or IMA . ... IMA if the wavelet transform has the same size as the original image. ...

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• Setting, Storing, and Retrieving the CCD Keywords
• Setting, Saving, and Retrieving CCD Keywords
• Input and Output

markback -- mark regions in the background for performing statistics on markback association . association . calnicb style association input file with list of images to be processed and co-added. number . labels boxes with numbers on image display . ... Only the first 2 boxes will be used by asncombine. nmem . image in association to use for marking the boxes. markback displays one image of an association (the nmem'th image), and allows the to mark nbox regions on the image display. ...

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• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
• ASNPHOT (Nov98) --- nictools --- ASNPHOT (Nov98)

... We assume that an instantaneous starburst occured in the region of the Galactic center, with half of the stars (in number) being formed in binaries. The total mass of the stars formed during the starburst was taken to be , as indicated by the Tamblyn & Rieke (1993) analysis. ... In fact, the number of stars in IRS 16 estimated by Tamblyn & Rieke (1993) is uncertain within a factor of 2, but this is actually of no importance as long as we only use relative numbers of different X-ray source species. ...

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• Restrictions on the Scenario Parameters
• Initial Distributions of Binary Parameters
• Number of accreting X-ray binaries of selected types

... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

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• TUI:Scripts:Built In Scripts:NICFPS:Data Cube
• what to do with the trace data
• DIS Keywords

... An international panel of experts led by NOAA and sponsored by NASA has released a new prediction for the next solar cycle. Solar Cycle 24 will peak, they say, in May 2013 with a below-average number of sunspots. ... Predicting the behavior of a sunspot cycle is fairly reliable once the cycle is well underway (about 3 years after the minimum in sunspot number occurs), but p rior to that time the predictions are less reliable. ... International Year of Astronomy, Ireland National Node . ...

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• SCL Sfit Genetic Commands
• IAJ: Contents - Volume 23 Number 2
• Hard disks

... The Multiple Extension FITS (MEF) file interface is an IRAF library providing facilities for general file operations upon FITS multi-extension files. ... The Multiple Extensions FITS (MEF) interface consists of a number of routines to mainly read a FITS Primary Data Unit or an Extension Unit and manipulate the data at a file level. ... Read the FITS header of a MEF file that matches the EXTNAME or EXTVER keyword values or if not specified, read the extension number `group'. ... The header filename. ...

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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• NICMOS Calibration Pipeline: Processing Associations of Exposures
• Pipeline Calibration for STIS

System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

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• NAG's Fortran 90
• SunSoft
• Naughty Number Nine

... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...

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• Zen: GiST internals
• SAI phone numbers
• Number of Supernovae discovered by amateurs since 1957.

... Content Model: Optional list header (LH), followed by one or more list items (LI) . An ordered list typically is a numbered list of items. ... The numbering style is left to associated style sheets, e.g. whether nested lists contribute to a compound item number, e.g. "3.1.5", or whether numbers are rendered as arabic, upper or lower case roman numerals or using the numbering scheme appropriate to the language context. ... CLASS . ... The CLEAR attribute allows you to move down unconditionally: . ...

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• Headings
• Previewing files
• Viewing manual pages

... PhD 1974 in Astrophysics, . ... Head of the Department of Theoretical Astrophysics, . Department Number . 01 (Theoretical Astrophysics) . ... Astro Space Center . ... Telephone Number . 7(095) 333 1535 . FAX Number . 7(095) 333 2378 . ... lukash@dpc.asc.rssi.ru ...

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• Kurt Vladimir, ASC
• Quantum Astrophysics Department of ASC of LPI Vladimir G. Kurt, ASC
• Novikov Igor Dmitrievich, Astro Space Center (ASC)

COSMIC DATA FUSION S.L. Bridle Astrophysics Group, Cavendish Laboratory, U.K. I will discuss our work on cosmic data fusion: the comparison and combination of various cosmological data sets to estimate cosmological parameters. ... References: Bridle, Eke, Lahav, Lasenby, Hobson, Cole, Frenk, and Henry, 1999, MNRAS, 310, 565 Bridle, Zehavi, Dekel, Lahav, Hobson and Lasenby, MNRAS, sub- mitted (astro-ph/0006170) 1 ...

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• http://www.mrao.cam.ac.uk/~rachael/compphys/examples/cell_list.f90
• http://www.mrao.cam.ac.uk/~anthony/latex/Newman.ps
• OptInt PmWiki : PmWiki / Page Directives