... Version 2.11.1 - 2008-05-15 (CB) ----------------------------- Ammended the test-harness to fix time-out failure in low-momory mode on some systems ( SPR 6460) =========================== Version 2.11 - 2008-05-07 (CB) ----------------------------- Modified a format statement in omsrclistcomb_mod.f90 to stop WHITE being truncated to WHIT Version 2.10 - 2008-05-02 (CB) ----------------------------- Updated documentation ... Attribute "OBS_ID" added to output source-list file (fixes SPR 2660...

... A total of 19 standard observing bands are defined at the VLA. ... The tables below describe the bands. ... VLA STANDARD BANDS - VLA SYNTHESIZER SETTINGS VLABAND VLAFEAB VLAFECD VLASYNA VLASYNB FLUKEA FLUKEB FEFILT CC 0.00 0.00 3860.1 3810.1 100.00000 200.00000 0000 UU 19.60 19.60 3610.1 3660.1 100.00000 200.00000 0000 KK 17.60 17.60 3860.1 3810.1 100.00000 200.00000 0000 LL - 3.20 - 3.20 3639.9 3560.1 100.00000 200.00000 0000 XX 13.40 13.40 3939.9 3889.9 ...

... DEVELOPER** -- Don Chance **MODIFICATION HISTORY** -- o Initial implementation 9/21/00 o Changed calendar lead time to 2 weeks. drc 2/27/01 o Modified for T-11 calendar building. drc 9/10/01 o Correct 'most recent ephem' query for normal ephems only. mdr 2/17/15 o code cleanup. drc 12/7/15 #*********************************************************************** from abstract_ check import abstract_ ...

Next: Interactive Editing of Up: Management of Tables Previous: Displaying Tables . Elements in a table can be inserted, changed , and deleted . These functions are all performed by the WRITE/TABLE or COPY commands (See Table 5.4). The element to be modified must be defined by giving its column and row location. ... Table: Commands to Modify a Table . ... All commands that do not change a table element will only use the subset selected. ... Table: Commands to Transfer Table Data . ...

... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...

Changed FITS time keywords to observatory standard and TAI: . Changed DATE-OBS from UTC date (yy-mm-dd) to TAI date and time (yy-mm-ddthh:mm:ss.sss) . Removed UTC-OBS; it was UTC time (hh:mm:ss.sss) . Added TIMESYS=TAI . AVAILMIN and AVAILMAX are now in TAI instead of UTC . Added IMAGETYP to FITS headers. ... Changed "expose stop" to halt the exposure sequence after the current exposure is finished normally (instead of aborting immediately and discarding the current exposure). ...

This page was created by the IDL library routine mk_html_help . ... mk_html_help . at the IDL command line prompt. ... to calculate CHIANTI line intensities and continua, to create a synthetic spectrum. ... WRITTEN : Ver.1, 7-Nov-01, Giulio Del Zanna (GDZ) and Peter Young (PRY) MODIFICATION HISTORY: V.2, 7-Nov-01, GDZ . Fixed a small bug (now the spectrum plot is always plotted within the widget), and modified the option to add continua. ... Added extended details in the ascii output spectrum. ...

... Astrophysics Group . ... Optical Interferometry . OIFITS: A Data Exchange Standard for Optical (Visible/IR) Interferometry . ... OIFITS is a standard for exchanging calibrated, time-averaged data from astronomical optical interferometers , based on the FITS Standard (OIFITS is a registered FITS convention ). ... The OIFITS standard is used in the biennial optical interferometry Imaging Beauty Contests: . ... A data exchange standard for optical (visible/IR) interferometry. ...