3 rd rsih&swa workshop – morelia, mexico – 20 october 2015 ips common data format v1.0...
TRANSCRIPT
3rd RSIH&SWA Workshop – Morelia, Mexico – 20 October 2015
IPS Common Data Format v1.0 (IPSCDFv1.0) - Official Launch!
M.M. Bisi ([email protected]) (1),
and The world-wide IPS community..
(1) RAL Space, Science and Technology Facilities Council, Rutherford Appleton Laboratory, Harwell Oxford, Didcot,
Oxfordshire, OX11 0QX, England, UK
Outline
Why?
Outline of IPSCDFv1.0
Where we are
Final steps
Are We Agreed and Open Discussions?
Why?
Why There are multiple IPS-capable systems with a variety of
analysis methods, data products, and ways in which data are
presented.
This makes it complicated for the non-IPS specialist to use and
understand without full hands-on interaction with the
observatory/data provider.
No clear distinction is made between single- and multi-site
obtained velocity values and what they might mean to the end
used/scientist looking to exploit the IPS result(s).
Because of the above, IPS is hugely under exploited.
Outline of IPSCDFv1.0
Outline (1)
Currently several of us have been experimenting with sub-
versions of the following plain-text ASCII format (although
exact character counts for each parameter/column need to be
explicitly agreed upon for uniformity still):
Date Start-UT System Cent.
Obs. Freq. Obs. Bandwidth Source
RA-J2000 DC-J2000 Limb
Dist. Lat. PA Elong. Vel.
V-err g-value g-err Method
Vel. V-err g-value g-err
Method
Outline (2)
Proposed addition of the source size on the sky which will
complete the plain-text ASCII format as the IPS Common Data
Format v1.0 (IPSCDFv1.0) for full implementation and use by
all:
Date Start-UT System Cent.
Obs. Freq. Obs. Bandwidth Source
Src. Size RA-J2000 DC-J2000 Limb
Dist. Lat. PA Elong. Vel.
V-err g-value g-err Method
Vel. V-err g-value g-err
Method
Where we are
Where are we? STELab and UCSD have been baselining the beta-testing
precursor to IPSCDFv1.0 in that almost all the parameters are
included with the exception of the radio source size on the sky
for the most part (ordering and column sizes need checking).
MEXART have started to implement this precursor format.
Not yet tested, as far as I am aware, is the output of two different
velocity values in the format (multi-site and then single site).
Others (as far as I am aware) have yet to start producing data for
sharing in this format but are willing to do so (where sufficient
data and results are available) once we have “frozen” the format.
Final Steps
What now? Add in the source-size option – this can be a null value (-999),
an estimate for the source on the sky at that particular observing
frequency, or an actual observed/determined size on the sky
(dependent upon the observatory’s needs/capabilities) as well as
set the column widths needed.
Provide data as openly as possible (with whatever constraints
you need to put on the use of the data) in this plain-text
ASCII format.
Promote the format where possible at meetings/conferences/
workshops and to let the wider community have exposure to IPS,
its capabilities, and its usefulness on its own and alongside other
data/data products/models/etc…
Are We Agreed and Open Discussions?
Are we agreed? (I hope so…)
Over to you all…
Are We Agreed and Open Discussions?