Cycle-3 Capabilities and the OT Andy Biggs ALMA Regional Centre, ESO.
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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.](https://reader036.fdocuments.us/reader036/viewer/2022081002/56649e925503460f94b97a56/html5/thumbnails/1.jpg)
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.](https://reader036.fdocuments.us/reader036/viewer/2022081002/56649e925503460f94b97a56/html5/thumbnails/2.jpg)
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
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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!)
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ARC Retreat 2014 – Cycle 3 Capabilities and the OT
Band-10 Transmission
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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
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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
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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
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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)
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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
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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
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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
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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
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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
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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
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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!!!
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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