Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

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Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO

Transcript of Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

Page 1: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

Cycle-3 Capabilities and the OT

Andy Biggs

ALMA Regional Centre, ESO

Page 2: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

New ALMA capabilities for Cycle 3

• Band 10• Baselines up to 10 km• FDM full polarization• Total Power in Bands 9 and 10 (probably)• 40 12-m array antennas (probably)• DiffGainCal

– Band-2-Band transfer– Bandwidth switching

Page 3: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Band 10

• Frequency coverage: 787-950 GHz (381-316 μm)• Angular resolution: ≈ 520-40 mas• OT will assume 40 12-m array antennas

– Actual number may be smaller

• Receiver temperature– Specification was 230 K (DSB) over 80% of band– OT will probably use a better figure

• 1st octile of PWV across whole band– 0.452 mm

• No mosaics (hot off the press!)

Page 4: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Band-10 Transmission

Page 5: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Long baselines

• Defined broadly as > 1.5 km• Baselines up to 10 km will be available• Available configurations will be band-dependent

– B3, 4 and 6: ≤ 10 km– B7: ≤ 5 km– B8, 9 and 10: ≤ 1.5 km

• Reminder: ALMA will extend out to 16 km, eventually• Phase calibrator cycle times will depend on

– Band– Frequency

Page 6: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Array selection

• This will be similar to Cycle 2• OT will automatically choose arrays based on

– Angular resolution– Largest Angular Scale

• Up to two 12-m configurations are allowed• “Long baselines” are fairly restricted

– Only have one 12-m configuration– No ACA

• No TP if MRS(12m) < LAS < MRS(7m)– This is new

• ACA times will remain a multiple of the 12-m time

Page 7: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Full polarization

• Cycle 2– Only TDM default frequencies were allowed– Bands 3, 6 and 7

• Cycle 3– TDM and FDM at arbitrary frequencies– All FDM bandwidths will be available (1875-62.5 MHz)– Still only Bands 3, 6 and 7

• Still on-axis only (single pointings)• Only linear polarization officially supported• Only one tuning per SG• 3-hour minimum time estimate will remain

Page 8: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Total Power at Bands 9 and 10

• Single dish sideband separation now possible– Data reduction and analysis has been demonstrated

• “Spectral line” only– No nutator or “fast scanning” mode for continuum

• May be dropped– Band-8 TP may also be dropped (flux calibration issues)

Page 9: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Sesame name resolver

• The OT has a “resolve” function for field sources– Positions/velocities automatically entered based on source

name

• Previous interface had some problems– Queried multiple servers– ESO shut the NED server we were using– How it worked was quite opaque (and dangerous)

• Now using Sesame (by Simbad)– Searches Simbad and NED– One interface so easier to maintain– Must enter a recognised source name

• Science Archive already uses this

Page 10: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Antenna beamsize

• OT has always assumed 1.2 λ / D• This will change to 1.13 λ / D

– TP SB generation had already been changed

• More mosaic pointings will result

Page 11: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Correlator modes

• No change...• Except for full polarization equivalents of existing FDM• Reminder of existing capabilities

– 4 independent basebands (TDM or FDM)– 4 spws per baseband (all must have same spectral resolution)

• For the future...– Multi-resolution modes– Over-sampling (twice Nyquist)– Different quantizations (3 and 4-bit)– 32.5 MHz-wide spws

Page 12: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Spectral Scan overlaps

• Cycle-2 OT assumed zero overlap for max. coverage• Quality of edge channels can be poor

– Ringing

– Bad Tsys measurements

– This is in addition to the TDM channels that are usually flagged

• An overlap will therefore be enforced in Cycle 3– Only a few TDM channels– Bandwidth dependent

Page 13: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Time estimates

• All tunings will stay in one SB– Will be observed in separate SBs though– Time estimates will be corrected using a fudge factor

• OT will not include DiffGainCals• Time estimates quantized by subscan duration

– Subscan duration defaults to 30s– Reduced if a large number of pointings are being observed– Integer number of mosaics

• Larger minimum on-source time?– Currently set to 2 minutes over all sources– 150 sources are allowed -> 20 s each

Page 14: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

“Experimental” modes

• Were defined as projects that couldn’t be pipelined– A maximum of 25% of such projects was envisaged– However, definition is slowly expanding...

• Current list– Bands 8, 9 & 10– Bandwidth switching projects– Full polarization– Spectral Scans– Long baselines (> 1.5 km)– Ephemeris observations– Non-standard calibrations

• Will be indicated to PI on cover sheet

Page 15: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

Miscellaneous

• Lots of bug fixes and small improvements• TJ will remain in OT and per SG

– Format has been improved– Copy and paste/drag and drop will work

• Ability to import and export pointing positions per source• No “point source” button• Improved time estimate dialogue• Improved time constraint interface• Multiple rectangular mosaics• And much, much more!!!

Page 16: Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.

ARC Retreat 2014 – Cycle 3 Capabilities and the OT

OT Cycle-3 Timeline

• 30 Sep– Deadline for input

• 1 Dec– Deadline for final (small) changes– Some capabilities might be dropped

• 15 Dec– Code freeze

• Jan/Feb– Test, test, test

• 23 Mar– Deployment