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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  25/04   24/04   23/04   22/04   21/04 
JL25A01 Jacob Wise 4 - - 4 -
JL25A03 Andreas Humpe - 8 - - -
JL25A04 Dan Perley - 16 16 16 -
JL25A05 K-Ryan Hinds - - - 5 -
JL25A08 Dan Perley - - - 12 -
JL25A09 Dan Perley 12 14 16 10 -
PL23B18 Daniel Kynoch - - 7 - -
PL25A01 Peter Clark - 10 - - -
PL25A05 Charlotte Angus 9 18 29 11 -
PL25A07 Ben Warwick 7 - - 12 -
PL25A08 Michael Goad - 23 - 25 -
PL25A13b Justyn Maund - - - 7 -
PL25A13c Justyn Maund 4 - 4 - -
PL25A16 Dimple - - 10 - -
PL25A27 Justyn Maund - 32 - 32 12
CL25A03b David Jones - 12 9 - -
CL25A04 Rene Damian Duffard - - 100 6 -
CL25A05b David Aguado 16 7 13 16 -
CL25A07 Luis Goicoechea 4 6 4 - -
CL25A08 Mireia Nievas-Rosillo - 28 - - -
AZ22A01 Filipp Romanov 11 - 15 - -
CALIB CALIB 53 52 37 46 -
DL12A02 Martin Altmann - 12 12 - -
IOOFringe LTOps 7 - - - -
IOOStand LTOps 14 28 14 28 -
JT24B03 Chris Copperwheat 2 9 - 2 -
JT25A02 Chris Copperwheat - 6 - - -
JZ24B01 Dan Perley 8 - - 8 -
MANUAL UNKNOWN 3 6 6 3 -
MiscOpsTestA LTOps 64 64 64 64 32
MiscOpsTestC LTOps 1299 - 120 200 778
MopStand LTOps 40 160 40 - -
NSOPrior1 Andy Newsam - - - 1 -
NSO_Priority_3 Andy Newsam 1 - 1 1 -
SPRATArc LTOps 2 2 2 2 -
SPRATBias LTOps 20 20 20 20 -
SPRATDark LTOps 5 5 5 20 -
SPRATFlat LTOps 4 4 4 4 -
SPRATStand LTOps 20 38 35 32 -
Standards LT_RCS 4 12 24 12 -
UNKNOWN UNKNOWN 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.