#
#  Template Checklist and Worksheet for reduction of VSOP Survey data.
#  (http://halca.vsop.isas.ac.jp/survey/template_checklist.txt)
#
#  Version 0.4  -  J. Lovell  6-October-1999
#                       - added amplitude correction factor entries
#  Version 0.3  -  J. Lovell  14-Apr-1999
#

# NOTE: Copy this file to your data reduction outputs directory (e.g
# /something/vs05a_jones) and name it "checklist.txt"
#
# Comments are given on lines beginning with a # and questions are 
# enclosed in {}'s.
# Please enter responses after the colons. 
# Multiple-line responses are OK.
# Yes/No questions may be answered with "yes", "no", "Y", "N", "y" or "n"

# An example of a completed Checklist is given in
# http://halca.vsop.isas.ac.jp/survey/checklist_eg.txt
#
# 

#---------------------------------------------------------------------------
#  Section 1 : General Information
#---------------------------------------------------------------------------

{Experiment code}        : VS10L1

{Your family name}       : Dodson
{Your given name}        : Richard

{The date you prepared this document 
(format is day-month-year, e.g 23-04-1999)} : 05-09-2004

{The name of the survey source that was observed} : J2152-7807
{The name of the calibration source(s) observed} : J0303-62

{The year the experiment took place (e.g. 1998)} : 2002
{The starting day number of the experiment}      : 91

{List the GRTs that observed} : HH CD HO MP
{List the tracking stations that took part} : UZ

{Which correlator was used to correlate the data? 
(Mitaka/Penticton/Socorro)} : Penticton

{AIPS Version used (e.g 15OCT98)} : 31DEC03
{Difmap Version used (e.g 2.3c)} : 2.3c
{Was vsop_difmap used? (yes/no)} : y

{Abstract. 
Write a brief summary of the data reduction and its outcomes} : 

No sign of HALCA fringes, but is it the orbit calculation?
Mopra still very low
I believe it is resolving on the GRT baselines.

#---------------------------------------------------------------------------
#  Section 2 : Pre-AIPS Checklist
#---------------------------------------------------------------------------

{PI letter retrieved (yes/no)} : n
{Data quality reports and plots retrieved? (yes/no)} : y
{Pre-launch 5GHz survey data retrieved? (yes/no)} : n
{Light-curve data retrieved? (yes/no)} : y

# Input files for INDXR, ANTAB and UVFLG

{Has a INDXR input file (INDXR.TXT) been created? (yes/no)} : n
{Has a ANTAB input file (ANTAB.TXT) been created? (yes/no)} : y
{Has a UVFLG input file (UVFLG.TXT) been created? (yes/no)} : n

{Any comments on Pre-AIPS file preparation?} :
used nominal_tsys.pl
#---------------------------------------------------------------------------
#  Section 3 : AIPS Output File Checklist
#
# Names of expected output file names are contained in square brackets.
#---------------------------------------------------------------------------

{PRTAN [PRTAN.LIS] (yes/no)} : y

{LISTR (optyp = 'SCAN') [LISTR.LIS] (yes/no)} : y

{DTSUM (aparm = 0) [DTSUM_0.LIS] (yes/no)} : y
{DTSUM (aparm = 1) [DTSUM_1.LIS] (yes/no)} : y

{UVPLT (u vs v) [UVPLT_UV.PS] (yes/no)} : y
{UVPLT ((u,v) distance vs time) [UVPLT_UVD.PS] (yes/no)} : y
{UVPLT ((u,v) position angle vs time).  [UVPLT_UVPA.PS] (yes/no)} : y

{VPLOT antenna weights vs time (after adjustment) [WEIGHTS.PS] (yes/no)} : n

ACCOR SNPLT (amplitude),
  {IF 1 [SN_ACCOR_1.PS] (yes/no)} : n
  {IF 2 [SN_ACCOR_2.PS] (yes/no)} : n

APCAL SNPLT (amplitude),
  {IF 1 [SN_APCAL_1.PS] (yes/no)} : y
  {IF 2 [SN_APCAL_2.PS] (yes/no)} : y

# FRING SNPLT (delay, rate, SNR), as many as necessary to document the
# clear discovery of fringes at all antennas, numbered with "nn" for
# both IFs. Do NOT include the final SN table as it is plotted later.
#
#   Format is SN_FRINGnn_DEL_i.PS, SN_FRINGnn_RAT_i.PS,
# SN_FRINGnn_SNR_i.PS for delay, rate and SNR plots respectively,
# where "i" is the IF number (1 or 2).

{Number of times preliminary FRING solutions were plotted
 (i.e maximum value of nn)} : 2

{Post-FRING CALIB SNPLT,
   Phase:
   IF 1 [SN_CALIB_PHA_1] (yes/no)} : y
  {IF 2 [SN_CALIB_PHA_2] (yes/no)} : y
  {Delay:
   IF 1 [SN_CALIB_DEL_1] (yes/no)} : y
  {IF 2 [SN_CALIB_DEL_2] (yes/no)} : y
  {Rate:
   IF 1 [SN_CALIB_RAT_1] (yes/no)} : y
  {IF 2 [SN_CALIB_RAT_2] (yes/no)} : y
  {SNR:
   IF 1 [SN_CALIB_SNR_1] (yes/no)} : y
  {IF 2 [SN_CALIB_SNR_2] (yes/no)} : y

{Post-calibration VPLOT (amp and phase, with channel averaging)
   IF 1 [VPLOT.PS] (yes/no)} : y
  {IF 2 [VPLOT_AP_2.PS] (yes/no)} : n


{Post-calibration POSSM (amplitude and phase, at least one 5 to 10 min
integration spectrum per tracking pass, indexed with nn = 01, 02, 03, ...),
   IF 1 [POSSM.PS] (yes/no)} : y
  {IF 2 [POSSM01_AP_2.PS] (yes/no)} : n

{Output TASAV FITS file (containing all 'multisource' cal tables)
   [VS10L1_DODSON_TASAV.FITS] (yes/no)} : y

{Calibrated and spectrally averaged FITS data files (one for each source),
   [J2152-78.VS10L1.UVF] (yes/no)} : y

#---------------------------------------------------------------------------
#  Section 4 : Supplementary files
#
# Were any files created, other than those listed, to document the data
# reduction?  If so, please list them below using as many (File, Description)
# groups as required.
#---------------------------------------------------------------------------

#---------------------------------------------------------
{File}        :
{Description} : Survey run file
#---------------------------------------------------------

#---------------------------------------------------------------------------
#  Section 5 : AIPS data-reduction notes
#
# The format is as follows:
#
# Task : the name of the task that is run or other operation performed
# ADVERBs : a list of the relevant non-default adverbs
# Input CL : the input calibration table used (if any) in running the task
# Input SN : the SN table that was used (if any)
# Output SN : the SN table produced (if any)
# Output CL : the CL table produced or modified (if any)
# Comments: any comments on the results of the operation
#
# Use as many of the (Task, ADVERBs, Comments, Input CL, Input SN,
# Output SN, Output CL) groups as required.
#---------------------------------------------------------------------------


#---------------------------------------------------------
{Task}      : FITLD
{ADVERBs}   : clint = 0.25
            digicor = -1
            delcorr = -1
{Input CL}  :
{Input SN}  :
{Output SN} :
{Output CL} :
{Comments}  :
#---------------------------------------------------------
{Task}      : INDXR
{ADVERBs}   : cparm = 0, 0, 0.25;
{Input CL}  :
{Input SN}  :
{Output SN} :
{Output CL} : 1
{Comments}  :
#---------------------------------------------------------
{Task}      : ANTAB
{ADVERBs}   : infile='antab.txt'
{Input CL}  :
{Input SN}  :
{Output SN} :
{Output CL} :
{Comments} :
#---------------------------------------------------------
{Task}      : APCAL
{ADVERBs}   :
{Input CL}  :
{Input SN}  :
{Output SN} : 1
{Output CL} :
{Comments}  :
#---------------------------------------------------------
{Task}      : CLCAL
{ADVERBs}   : refant=1;
{Input CL}  : 1
{Input SN}  : 1
{Output SN} :
{Output CL} : 2
{Comments}  : Amplitude calibration solutions applied.
#---------------------------------------------------------
{Task}      : FRING
{ADVERBs}   : dparm 2,400,400,0.5,0;aparm(7)=0.1;solint 5,10,15;refa 2/3
{Input CL}  :
{Input SN}  :
{Output SN} : 2,3,4,5
{Output CL} :
{Comments}  :
#---------------------------------------------------------
{Task}      : UVFLG
{ADVERBs}   : flagv 1;ante 1;reason 'maser off';ante 4;timer
                        0 07 0 0 7 25 42/0 7 37 5 0 7 43 27
{Input CL}  :
{Input SN}  :
{Output SN} : 
{Output CL} :
{Comments}  : No ceduna & mopra off source a bit
#---------------------------------------------------------
{Task}      : FRING
{ADVERBs}   : dparm 2,60,60,0.5,0;aparm(5)=1/0;solint 5;refa 3;ante -5
{Input CL}  :
{Input SN}  :
{Output SN} : 6,7
{Output CL} :
{Comments}  : no HALCA, tight search for the GRTs. Mopra poor
#---------------------------------------------------------
{Task}      : SNEDT/CLCAL
{ADVERBs}   : opc 'calp';interp 'poly';intp 3
{Input CL}  : 2
{Input SN}  : 7
{Output SN} : 8
{Output CL} : 3
{Comments}  :
#---------------------------------------------------------
{Task}      : FRING
{ADVERBs}   : dparm 2,60,20,0.5,0;ante -5 0;solint 10/5;aparm(5)=0/1
{Input CL}  : 3
{Input SN}  :
{Output SN} : 9,10,11,12
{Output CL} :
{Comments}  :
#---------------------------------------------------------
{Task}      : SNEDT/CLCAL
{ADVERBs}   : opc 'calp';interp 'ambg'
{Input CL}  : 3
{Input SN}  : 11
{Output SN} : 13
{Output CL} : 4
{Comments}  :
#---------------------------------------------------------
{Task}      : KRING
{ADVERBs}   : cparm 0.5,100,30,0.5,0;dofit 5;ante -4 0;
              solint 10/5;solm 'rd'/''
{Input CL}  : 4
{Input SN}  :
{Output SN} : 14,15,16,17
{Output CL} :
{Comments}  : No fringes
#---------------------------------------------------------
{Task}      : SPLIT
{ADVERBs}   : aparm(1)=2 0;
{Input CL}  : 4
{Input SN}  :
{Output SN} :
{Output CL} :
{Comments}  : Av within IF
#---------------------------------------------------------
{Task}      : FITTP
{ADVERBs}   :
{Input CL}  :
{Input SN}  :
{Output SN} :
{Output CL} :
{Comments}  : Data written out for analysis in Difmap
#---------------------------------------------------------------------------
#  Section 6 : Antenna-based amplitude corrections
#-------------------------------------------------------------------------
# Corrections applied with CLCOR in AIPS to correct for antenna-based
amplitude
# errors.
# Separate antenna names and correction factors by commas or spaces.
# e.g
#
# {Antenna name list} :            HALCA, HO,  HH,  MP,  KA
# {Amplitude correction factors} : 1.0,   1.6, 1.3, 1.0, 1.0
#
{Antenna name list} : MP, HO, HH, HALCA, CD
{Amplitude correction factors} : 5.0, 1, 1, 1,1 

#-------------------------------------------------------------------------
#  Section 7 : Difmap data reduction notes
#---------------------------------------------------------------------------

{Phase Selfcal applied? (yes/no)} : n
{Global Amplitude Selfcal applied? (yes/no)} :  n

{Amplitude Selfcal applied on non-global timescales? (yes/no)} : n
{Modelfit made and saved using the vs_final_mod macro? (yes/no)} : y
{Image made and saved using the vs_final_img macro? (yes/no)} : n

{Comments on Difmap processing.
Include the global amplitude offsets that were applied if gscal was
used} :

Mopra is low, and needs scaling up by about 5, which is acceptable as
the HO-HH MO-HH baselines are almost identical. J0303-68 Agrees for
this. 

Once this is done a simple Guassian can be fit, which would imply that
the space fringes would resolve.

# If GSCAL was used, report amplitude correction factors here. If GSCAL
# was used more than once, report the CUMULATIVE factor here (e.g if gscal
# reported a gain factor of 1.11 for HALCA the first time and 0.95 the
# second time, the overall gain correction is 1.11 * 0.95 = 1.05.
# Separate antenna names and correction factors by commas or spaces.
# e.g
#
# {Antenna name list} :            HALCA, HO,  HH,  MP,  KA
# {Amplitude correction factors} : 1.0,   1.6, 1.3, 1.0, 1.0
#
{Antenna name list} :
{Amplitude correction factors} :

#---------------------------------------------------------------------------
# Do not delete or alter anything past this line
{VSOP Survey Checklist and Worksheet version} : 0.4
#---------------------------------------------------------------------------