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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  20/04   19/04   18/04   17/04   16/04 
JL25A01 Jacob Wise - 14 20 10 -
JL25A02 Andreas Humpe 7 - - - -
JL25A04 Dan Perley 12 12 - - -
JL25A08 Dan Perley 6 - - - -
JL25A09 Dan Perley 11 6 - - -
PL23B18 Daniel Kynoch 7 - - 7 -
PL25A05 Charlotte Angus 9 18 16 38 3
PL25A06 Ian McHardy - 2 2 2 -
PL25A07 Ben Warwick 11 - 8 4 -
PL25A08 Michael Goad - 22 23 23 -
PL25A10 Umut Burgaz - - 7 - -
PL25A13b Justyn Maund 7 7 7 7 -
PL25A13c Justyn Maund 10 - - 14 -
PL25A23 Cyrielle Opitom - - - 6 -
PL25A26 Jacobus Terwel - 2 2 15 -
PL25A27 Justyn Maund - 32 - 32 -
CL25A04 Rene Damian Duffard 6 - - 6 -
CL25A05b David Aguado 14 19 18 9 -
CL25A07 Luis Goicoechea 8 - 6 8 -
CL25A08 Mireia Nievas-Rosillo - 22 - 22 -
AZ22A01 Filipp Romanov 40 30 - - -
CALIB CALIB 65 48 55 52 36
IOOStand LTOps 20 24 20 24 8
JT24B03 Chris Copperwheat - 4 4 2 2
JZ24B01 Dan Perley 8 16 13 - -
MANUAL UNKNOWN 3 6 5 6 6
MiscOpsTestA LTOps 64 64 64 64 -
MiscOpsTestC LTOps 600 - 200 16 -
NSOPrior3 Andy Newsam - - 1 3 -
NSO_Priority_1 Andy Newsam - - - 1 -
NSO_Priority_2 Andy Newsam - 7 3 1 -
NSO_Priority_3 Andy Newsam - - 4 4 -
SchedEfficiency Sebastian Buntin - - 1 7 1
SPRATArc LTOps 2 2 2 2 2
SPRATBias LTOps 20 19 20 20 20
SPRATDark LTOps 5 5 5 5 5
SPRATFlat LTOps 4 4 4 - -
Standards LT_RCS 12 48 64 - -
UNKNOWN UNKNOWN 4 4 4 4 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.