Spire FTS Workshop 13th May 2010

Introduction to SPIRE Spectroscopy: a one day meeting in London

This one day workshop introduced the capabilities of the SPIRE Fourier Transform spectrometer as demonstrated during the first year of Herschel operations. During the day we gave examples of the different observing programmes that are possible with the instrument, discussed the achievable sensitivity and observing strategies and promote its use in the upcoming call for Herschel Open Time. The day consisted of a series of presentations by instrument and data processing experts as well as by users illustrating the instrument capabilities from guaranteed time programmes. The instrument and data processing experts were available to answer questions and advise on the best way of executing your proposed observing programme and discuss possible science programmes.


PDF versions and videos of the talks

Start 09:30 13th May 2010

Session 1: Basics 09:30-11:00
i) Introduction, logistics and purpose of meeting, Bruce Swinyard
ii) SPIRE Spectrometer - description, capabilities and performance, Bruce Swinyard
iii) Spectrometer Observing Modes, Ed Polehampton
11:00-11:15 Coffee Break
Session 2: Data reduction, calibration and data products
iv) FTS Data reduction pipeline and standard product description, Trevor Fulton
v) Calibration status, Tests of source models, Ed Polehampton/Bruce Swinyard
vi) Caveats and problems, Trevor Fulton
Lunch 13:00-14:00
Session 3: Example Observing programmes 14:00-15:15
vii) Example observing programmes from SDP . including caveats . so far we have identified the following topics/speakers.
A point source (VY Cma), Roger Wesson
Faint and very faint sources (Comet Christensen+), Bruce Swinyard
Sparse mapping over a small region, Glenn White
Intermediate & fully sampled mapping & wide area mapping, Ed Polehampton
15:15-15:30 Tea Beak
Session 4: 15:30-16:30 (or later)
Interactive to look at individual proposals for observing programmes . please come prepared. We will break into smaller groups dedicated to different topics (faint sources, line confusion, mapping etc) if this looks like the most efficient way of proceeding. If not then we will take the topics serially in plenary session.
Session 5: 16:30-17:00 (or later)
Summary and next steps.

Participants: