! BI 28 ! Hiroshi Imai et al.: ! An extremely high velocity flow in OH/IR star IRAS 19134+2131 ! ! Keyin file of the project BI 28 for dynamic scheduling. ! ! Used telescopes: ALL VLBA stations. ! At least continental 8 stataions are need. ! Core blocks in the inner 6 hours (see time scans). ! ! ================================================================ ! Preferred Dynamic Contraints. Alter [defaults] as desired. ! ================================================================ ! Equipment constraints: ! Stations. Below each station code, the "o" indicates an ! [optional] station that is to be used if it is available. ! Change "o" to "r" if the station is required or change ! "o" to "n" if the station is not to be used. ! SC HN NL FD LA PT KP OV BR MK ! o r r r r r r r r o ! Minimum number of stations [9 (6 for 3mm)]: ! May we swap PT for a single VLA antenna? [yes] ! Bands and polarizations. Below each band code, insert "R" ! if the righthand polarization is to be used, "L" if the ! lefthand polarization is to be used, "d" if dual ! polarizations are to be used, or "o" if the band is in ! your setups but scheduling should not be constrained by ! its availability. ! 90cm 50cm 20cm 13cm 6cm 4cm 2cm 1cm 7mm 3mm ! d ! Weather constraints: ! [appropriate for bands marked "L", "R", or "d" above ! and for at least the minimum number of stations] ! Date constraints: ! Preferred date(s), usually a series start [none]: October 2003 ! Excluded dates plus reason [none]: ! Preferred interval between segments in days [none]: 3 months ! Special conditions (e.g., a series with different ! spacings in time) [none]: ! ================================================================ ! ========================================================== ! ================= Cover Information ==================== ! ========================================================== ! expt = 'H. Imai: IRAS 19134+2131' expcode = BI028B version = 1 PINAME = 'Hiroshi Imai' ADDRESS1 = 'Department of Physics' ADDRESS2 = 'Kagoshima University' ADDRESS3 = '1-21-35 Korimoto, Kagoshima 890-0065' ADDRESS4 = 'JAPAN' PHONE = '81-99-285-8960' OBSPHONE = '81-99-285-8960' FAX = '81-99-285-8960' EMAIL = 'hiroimai@sci.kagoshima-u.ac.jp' OBSMODE = 'VLBA' OBSTYPE = 'VLBA' ! ========================================================== ! ============== Correlator Information ================== ! ========================================================== correl = 'Socorro' coravg = 2.0 corchan = 512 cornant = 10 corpol = 'off' corwtfn = 'uniform' cortape = DAT corship1 = 'Hiroshi Imai' corship2 = 'Department of Physics, Kagoshima University' corship3 = '1-21-35 Korimoto, Kagoshima 890-0065' corship4 = 'Japan' ! ! ========================================================== ! ================== Program control ===================== ! ========================================================== ! ! Normally SCHED will not overwrite preexisting files. ! If you want this protection, comment this following line. overwrit SUMITEM = AZ1, EL1, EARLY, TAPE1 ! ! To only process VLBA and VLA stations, uncomment the following line: dosta 'vl' ! ! ========================================================== ! =================== Tape initialization ================= ! ========================================================== !** WARNING: Check with data analysts that the following tape ** !** information is correct for YOUR project! ** ! autotape=2 tapeini / tpsta = vlba,vla1 tpdrive = 1 tpindex = 1 tplength= 17600 ndrives = 2 nheadpos= 14 density = H / !end tape initialization stuff ! ! ========================================================== ! ================== Station Catalog ===================== ! ========================================================== ! stafile = $SCHED/catalogs/stations.dat ! ========================================================== ! ==================== Source Catalog ====================== ! ========================================================== srccat / !TARGET SOURCE='IRAS1913' RA=19:15:35.215 DEC=+21:36:33.90 Vel= -30.0,-30.0,-130.0,-130.0 Epoch='J2000' / ! Coordinate determined by the VLA observation. !Fringe finder, bandpass calibrator and reference SOURCE='J1925+2106','1923+210','J1925+21' RA=19:25:59.6053696 DEC= +21:06:26.161947 EPOCH='J2000' REMARKS='USNO - Ref Frame 1998-6, Eubanks June 1998' / !Another reference SOURCE='J1910+2305','1910+230' RA=19:10:45.127113 DEC= +23:05:58.60703 EPOCH='J2000' REMARKS='Cataloged in the VLBA calibrators' / endcat / ! ========================================================== ! ============== Spectral line rest frequecies =========== ! ========================================================== lineinit / lineset='H2O' restfreq=22235.07985 / endlines / ! ========================================================== ! =================== Observing setup ==================== ! ========================================================== ! ------------------------------------------------------------- ! Setup for VLBA observations of H2O lines. ! 1.3 cm wavelength ! 8 MHz per channel 16 MHz sample rate No oversampling. ! 2 bit per sample 128 Mbps on tape No fan in or out. ! 4 channels 2 polarizations ! No phase cal. ! The frequencies will center the H2O restfrequencies. ! setinit = bi28.set / nchan = 4 samprate = 16.0 bits = 2 bbfilter = 8.0 ! 128 Mbps tpmode = 2 format = VLBA1:2 bbc = 1, 2, 3, 4 netside = U, U, U, U ifchan = R, L, R, L pcal = 'off' freqref = 22225.99 firstlo = 21500.00 freqoff = 0.0, 0.0, 8.0, 8.0 barrel=roll_off station = 'VLBA' rchan = B lchan = D / endset / ! ========================================================== ! ================= Initial Scan Information ============= ! ========================================================== LST=VLBA_PT DAY = 59710 START = 15:30:00 linename = 'H2O' DOPPLER setup = 'bi28.set' BW = 8.0, 8.0, 8.0, 8.0 ! ========================================================== ! ======================== The Scans ===================== ! ========================================================== stations = VLBA_SC, VLBA_HN, VLBA_NL, VLBA_FD, VLBA_LA, VLBA_PT, VLBA_KP, VLBA_OV, VLBA_BR, VLBA_MK ! Group of scans before core scans' SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / ! Core scans' SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=22 SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / ! Group of scans after core scans' SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:05:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=17 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / RECORD GROUP=2 REPEAT=22 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:02:00 DUR = 00:01:00 DOPSRC 'IRAS1913' / RECORD GROUP=2 REPEAT=14 SOURCE = '1910+230' GAP = 00:00:00 DUR = 00:00:30 DOPSRC 'IRAS1913' / SOURCE = 'IRAS1913' GAP = 00:00:00 DUR = 00:00:30 / SOURCE = '1923+210' GAP = 00:00:00 DUR = 00:06:00 DOPSRC 'IRAS1913' / !---------------------------------------------------------