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Date: Tue, 27 Mar 2001 09:56:56 -0800 (PST)
From: VLBI Operator <vlbiop@drao.nrc.ca>
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To: VSOG <vsog@vsop.isas.ac.jp>
cc: VLBI Operator <vlbiop@drao.nrc.ca>,
   Glen Langston - GREEN BANK GRT <glangsto@nrao.edu>,
   Kenta Fujisawa - USUDA GRT <kenta@vsop.isas.ac.jp>,
   Kevin Miller <kjmiller@jpl.nasa.gov>,
   Huang Xinyong - SHANGHAI GRT <xhuang@center.shao.ac.cn>,
   VLBI Friend Account <vlbifriend@bootes.hartrao.ac.za>,
   John Reynolds <jreynold@atnf.CSIRO.AU>,
   University of Tasmania VLBI Account <vlbi@phys.utas.edu.au>,
   Bill Scott - UofC <bill@ras.ucalgary.ca>
Subject: Exp. VS01s PI Letter
Message-ID: <Pine.SUN.3.96.1010327095225.6633B-100000@sol>
MIME-Version: 1.0
Content-Type: TEXT/PLAIN; charset=US-ASCII
Status: RO


  ==========================================================================
  PI INFORMATION LETTER FROM PENTICTON S2 CORRELATOR FOR EXPERIMENT VS01s
  ==========================================================================


  PI:       The VSOP Survey Program, Hirabayashi Lab.                       

  Address:  Institute of Space and Astronautical Science,                   
            3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510                 
            JAPAN                                                           
                                                                            

  Phone:    81-427-59-8340                                                  
  EMAIL:    vsog@vsop.isas.ac.jp                                            
  Fax:      81-427-59-8340                                                  


Dear PI:

This letter is to inform you of some of the details of the correlation and
analysis of your experiment 'VS01s'.  Your contact person at the correlator is:

   Rob Shanks
   Tel: (250) 493-2277
   Fax: (250) 493-7767
   email: Rob.Shanks@nrc.ca

and is the person who correlated your experiment.  You can also contact
the University of Calgary Radio Astronomy Lab for assistance with data
reduction and imaging using AIPS and DIFMAP.

The data package that we are sending you contains this letter and the FITS
data tape in the format requested in the VS01s.sum file.  Additionally,
there are a number of files on the University of Calgary ftp server that will
be of interest to you.  All files are available via anonymous ftp, with the 
exception of the .dqa1 and .gz files, which are restricted access only.
These files include:

	VS01s_DQA1.txt -- ASCII *summary* file of single baseline fringe
	                  search results.
	VS01s.dqa1 -- ASCII file of single baseline fringe search results.
	VS01s.ps -- postscript plot of experiment station playback times.
	VS01s_DQA1.ps.gz -- gzipped postscript file of plots of single baseline
	                  fringe search results.  This includes plots of phase
	                  cal extracted at the correlator and available in your
	                  FITS data.
	VS01s.log -- log file generated by the correlator.
	VS01s.comments -- comments extracted from station log files.
	VS01s.tsys -- Tsys data extracted from station log files.  This is not
	              formatted to read into AIPS but is provided as auxillary
	              information if Tsys files are not otherwise available.

In addition, since this is Space VLBI data there may be times when delay
discontinuities occur on space baselines (VSOP_SC) -- due to tracking station
handovers and 'clock setting events' at individual tracking stations
resulting from momentary loss of downlink lock.  These will show up as glitches
or delay jumps in the VSOP_SC phase cal data and in the fringe fits results.
For convenience, all times across which fringe fitting should not be done
are at the end of this file in a format ready to be read in by AIPS' INDXR.
The tracking passes are as follows:

		'MADRD_TS' 2000-337-12:15:13 --> 2000-337-16:33:32
		'TDBIN_TS' 2000-337-06:57:56 --> 2000-337-11:08:14

...and periods of downlink loss are as follows:

		337-10:00:42.810 -> 337-10:01:06.400
		337-10:08:03.910 -> 337-10:08:33.400
		337-11:06:13.910 -> 337-13:24:55.000

You will have approximately 3 weeks from today (Mon Mar 26 11:11:33 PST 2001) 
to look at the data and request recorrelation if there is a problem.
Recorrelation requests will only be *considered* if the data is bad and it can
be traced to the correlator or if there is a valid scientific reason (such
as a change of correlation parameters or change of source coordinates).
PLEASE LOOK AT THE DATA AS SOON AS POSSIBLE SINCE YOUR FEEDBACK TO THE MISSION
IS IMPORTANT.  Please contact the UofC RAL as soon as you are satisfied with
the data so that re-cycling of VLBI tapes can occur with your input in a
timely manner.

If the data is bad or not scientifically acceptable due to problems at
acquisition time, you must contact the VSOG to request re-observation of the
radio source.  If the data is good, then in accordance with mission policy,
18 months after it is released from the correlator, it will be available to
any PI on a request basis.

Good luck with your data!

=================================
Correlator PR/Data analyst notes:
=================================

Fringes to all GRTs and to spacecraft.

HO did not take part due to a hydrolics problem on site.

HH recorded ch2 as RCP so ch2 could not be correlated with anything. Fringes
were found in ch1.

RZ tracking pass, 2000-337-12:15:13 --> 2000-337-16:33:32, did not overlap
with any GRT observations so could not be correlated. Pass started at 12:15
but Data Valid flag was not set until 13:24.

A 200ns discontinuity appears in delay on TZ baselines at 10:15 UTC.

MP recorded both channels with a 1st LO of 4824MHz LSB centered on 4816MHz.
Were able to correlate lower 8MHz of this band with ch1(4800-4816MHz) from 
other stations and the upper 8MHz with ch2(4816-4832MHz).

Your FITS tape(s) incl: 1 FITS files, 82359360 bytes total

Participating GRTS: CD, HH, MP, SH


==================
POINTS OF CONTACT:
==================

---Correlator---
	Operations email: vlbiop@hia.nrc.ca
	Operations Manager (Sean Dougherty): Sean.Dougherty@hia.nrc.ca
	Tel: (250) 493-2277 (~16:00 to 24:00 UT)
	Fax: (250) 493-7767
	Web: http://www.drao.nrc.ca
	Anonymous ftp: ftp.drao.nrc.ca /pub/vsop
	Address:
		Attn: Space VLBI
		Dominion Radio Astrophysical Observatory
		Hertzberg Institute of Astrophysics
		National Research Council of Canada
		White Lake Road (P.O. Box 248)
		Penticton, B.C. Canada V2A 6K3

---University of Calgary RAL---
	Bill Scott: bill@ras.ucalgary.ca
	Russ Taylor: russ@ras.ucalgary.ca
	Tel: (403) 220-7424
	Fax: (403) 289-3331
	Web: http://www.ras.ucalgary.ca
	ftp: cougar.ras.ucalgary.ca
	public directories: /pub/vsop/<OBSCODE>
	restricted directories: /usr/home/vsopobs/vsop/<OBSCODE>
	(contact Bill Scott for restricted access permissions)
	Address:
		Attn: Bill Scott/Russ Taylor
		Physics and Astronomy Department
		University of Calgary
		2500 University Dr. NW,
		Calgary, Alberta, Canada T2N 1N4

---The VSOG (VSOP Science Operations Group)---
	email: vsog@vsop.isas.ac.jp
	S2 Scheduler: Ian Avruch (avruch@halca.vsop.isas.ac.jp)
	Tel: +81-427-59-8346 (8am to 6pm JST)
	Fax: +81-427-69-8949
	Web: http://www.vsop.isas.ac.jp
	(Web site contains schedule information, experiment status
	 details, HALCA calibration data and data reduction info.)
	Address:
		ISAS, 3-1-1 Yoshinodai, Sagamihara
		Kanagawa 229, Japan

---AIPS/Data Reduction---
	VSOP Data Reduction Exploder (VDR): vdr@aoc.nrao.edu -- for general help
	and exchange of information regarding VSOP data reduction.
	'Designated AIP': daip@aoc.nrao.edu -- for reporting bugs in AIPS.


!
! Start of Formatted entries for input to AIPS' INDXR.
! These epochs are times across which fringe fitting should not be done.
! They include all tracking station handovers and clock setting events.
!
SUBARRAY = 1 /
337 10:00:42.810
337 10:08:03.910
337 11:06:13.910
/


-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-
Rob Shanks              email:Rob.Shanks@nrc.ca
VLBI Data Controller    DRAO, Penticton BC 
phone:(250)493-2277     fax:(250)493-7767
+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+-+


