! BM161A: Testing spectral age derivation assumptions for CSO 1245+676 ! A. Marecki et al. ! Approved for dynamic scheduling, second priority ! 10-12 hrs dynamically scheduled around VLBA_PT LST 10.0 ! ! ================================================================ ! 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 o o o o n o o o o ! Minimum number of stations [9 (6 for 3mm)]: 7 ! May we swap PT for a single VLA antenna? [yes] ! Consult http://www.aoc.nrao.edu/~gtaylor/y1gotcha.html ! to decide. If you adopt the default, then both PT and ! VLA1 must be in the stations list in the keyin file. ! 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 ! o ! 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]: ! Excluded dates plus reason [none]: ! Preferred interval between segments in days [none]: ! Special conditions (e.g., a series with different ! spacings in time) [none]: ! ================================================================ overwrit sumitem = el1, el2, tape1, tape2, early, dwell ! ========================================================== ! ================= Cover Information ==================== ! ========================================================== version = 3 expt = 'Testing spectral age derivation assumptions for CSO 1245+676' expcode = BM161A obstype = VLBA piname = 'Andrzej Marecki' address1 = 'Torun Radio Astronomy Observatory' address2 = 'N. Copernicus Univ.' address3 = 'ul.Gagarina 11' address4 = 'PL-87-100 Torun, Poland' phone = '+48 56 611 30 32' obsphone = '+48 56 611 30 32' email = 'amr@astro.uni.torun.pl' fax = '+48 56 611 30 09' obsmode = 'Continuum with v1cm-256-8-2-L.set' correl = 'Socorro' note1 = 'Schedulable even if the weather is suitable for 15 GHz only.' ! ========================================================== ! ============== Correlator Information ================== ! ========================================================== correl = 'Socorro' coravg = 2 corchan = 16 cornant = 10 corpol = 'off' corwtfn = 'uniform' corsrcs = 'All from embedded catalog except the FF.' cortape = DAT corship1 = 'Andrzej Marecki' corship2 = 'Torun Radio Astronomy Observatory' corship3 = 'N. Copernicus Univ., ul.Gagarina 11' corship4 = 'PL-87-100 Torun, Poland' cornote1 = ' ' ! ========================================================== ! ==================== Source Catalog ===================== ! ========================================================== ! Get the sources from the embedded catalog. srccat / epoch='J2000' source='1245+676' ra=12:47:33.328 dec=67:23:16.455 / source='J1302+6902' ra=13:02:37.9246 dec=69:02:51.613 / source='J1048+7143' ra=10:48:27.6199 dec=71:43:35.93835 / endcat / ! ========================================================== ! ===================== General setup ====================== ! ========================================================== autotape = 2 !year = 2003 !month = 5 day = 59465 lst = VLBA_PT start = 04:30:00 stations = SC, HN, NL, FD, LA, PT, KP, OV, BR, MK setup $SCHED/setups/v1cm-256-8-2-L.set ! ========================================================== ! ======================== The Scans ===================== ! ========================================================== ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. ! Time for readback test gap=2:00 source = J1048+7143 dur 120/ ! Secondary phase cal. gap=0 source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Fringe finder scan source= 3C273B dwell 5:00 / ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. ! Time for readback test gap=2:00 source = J1048+7143 dur 120/ ! Secondary phase cal. gap=0 source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Fringe finder scan source= 3C273B dwell 5:00 / ! Primary phase cal. ! Time for readback test gap=2:00 source = J1048+7143 dur 120/ ! Secondary phase cal. gap=0 source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. ! Time for readback test gap=2:00 source = J1048+7143 dur 120/ ! Secondary phase cal. gap=0 source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! Secondary phase cal. source = J1302+6902 dwell 60/ group = 2 repeat 15 source = 1245+676 dur 60/ source = J1302+6902 dur 60/ ! Primary phase cal. source = J1048+7143 dwell 120/ ! ========================================================== ! ===================== End of schedule ================== ! ==========================================================