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Quicklook

Most science data obtained on the telescope are available here about five minutes after the exposure is complete. Data here are quicklook reductions only. They may not use the most up to date calibrations and have not undergone any detailed quality control inspection. Exactly what data formats are available as QUICKLOOKs varies between instruments. See the descriptions for each instrument at the foot of the page.

ProposalUser Name  11/07   10/07   09/07   08/07   07/07   06/07 
JL25A01 Jacob Wise - - - - 7 -
JL25A08 Dan Perley - - - - 8 -
JL25A09 Dan Perley - - - - 31 40
JL25A11b Beth Garton - - - - 18 -
PL23B18 Daniel Kynoch - - - - - 7
PL25A07 Ben Warwick - - - - 12 -
PL25A25 Rob Eyles-Ferris - - - - - 24
CL25A04 Rene Damian Duffard - - - - 9 -
CL25A05a David Aguado - - - - 9 29
CL25A07 Luis Goicoechea - - - - - 6
AZ22A01 Filipp Romanov - - - - 10 -
CALIB CALIB - - - - 22 21
IOOStand LTOps - - - - 28 21
LTCollim LTOps - - - - - 2
MANUAL UNKNOWN - - - 2 6 -
MiscOpsTestA LTOps - - - - 128 128
MopStand LTOps - - - - - 240
NSOPrior3 Andy Newsam - - - - 2 2
NSO_Priority_1 Andy Newsam - - - - - 1
NSO_Priority_2 Andy Newsam - - - - 5 -
NSO_Priority_3 Andy Newsam - - - - 5 7
SPRATArc LTOps 2 2 2 2 2 -
SPRATBias LTOps 20 20 20 20 20 -
SPRATDark LTOps 4 4 4 4 4 -
SPRATFlat LTOps - - - - - 4
SPRATStand LTOps - - - - 20 9
UNKNOWN UNKNOWN 6 10 10 8 4 -

Which data formats are available as QUICKLOOKs varies between instruments.

  • IO:O : Generally all data observed are available here fully reduced.
  • RISE : Only a sparsely sampled subset, not every frame taken, will appear here due to the high data rate from this instrument.
  • SPRAT : All data will be available here, including the full, wavelength-calibrated, extracted spectrum. Typically only the 'normalized flux' version will be available with the absolute flux calibrated version added during the full reduction next working day.
  • MOPTOP : Only a sparsely sampled subset, not every frame taken, will appear here due to the high data rate from this instrument. It is intended to be sufficient to confirm the group has been observed and check the pointing is correct. Using just four rotor positions (1-4) it is possible to measure polarisation, assuming the target is bright enough to be detected in single, unstacked frames.

For all instruments, final reductions are available from the searchable data archive and Recent Data web pages next working day.