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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  31/05   30/05   29/05   28/05   27/05   26/05 
JL25A01 Jacob Wise - - - 4 - -
JL25A05 K-Ryan Hinds - - - 5 - -
JL25A11b Beth Garton - - 18 - - -
JQ25A01 Omand.Conor - 32 - - - -
PL23B18 Daniel Kynoch - 7 - - - -
PL25A03 Gavin Ramsay - - - 7 - -
PL25A04 Charlotte Angus - - 7 - - -
PL25A06 Ian McHardy 2 2 - - - 2
PL25A07 Ben Warwick 2 - - 11 - -
PL25A08 Michael Goad 22 25 - - - -
PL25A12 Thomas Moore 24 - - - - -
PL25A13c Justyn Maund - 4 4 4 - -
PL25A16 Dimple - 10 - - - -
PL25A19 Shubham Srivastav - 8 - - - -
PL25A26 Jacobus Terwel - 7 13 16 - -
CL25A04 Rene Damian Duffard - 7 7 - - -
CL25A05a David Aguado 9 - - - - -
CL25A05b David Aguado 5 - - 8 - -
CL25A07 Luis Goicoechea - 6 8 - - -
CL25A08 Mireia Nievas-Rosillo - - 26 17 - 20
AZ22A01 Filipp Romanov - - 34 - - -
CALIB CALIB 30 48 60 63 - -
DL12A02 Martin Altmann - - - 20 - -
IOOFringe LTOps - - - - - 14
IOOStand LTOps 7 35 20 28 - -
JZ24B01 Dan Perley - 9 - - - -
MANUAL UNKNOWN 2 6 6 4 2 -
MiscOpsTestZ LTOps - - 100 100 100 200
MopStand LTOps - - - 40 - -
NSOPrior1 Andy Newsam 1 - - - - -
NSO_Priority_1 Andy Newsam - - 1 - - 8
NSO_Priority_2 Andy Newsam - - - 8 - -
NSO_Priority_3 Andy Newsam - - 3 1 - -
SPRATArc LTOps 2 2 2 2 - -
SPRATBias LTOps 20 20 20 17 - -
SPRATDark LTOps 4 4 4 4 - -
SPRATFlat LTOps - 4 4 4 - 4
SPRATStand LTOps 40 39 - 18 - -
Standards LT_RCS - 120 - 8 - 144
UNKNOWN UNKNOWN 4 4 4 7 1 -

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.