ALMA Operations the role of the European ALMA Regional Centre Plans for cycle 1
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1 ALMA Operations the role of the European ALMA Regional Centre Plans for cycle 1 Paola Andreani
2 ALMA Operations Sites in Chile Antenna Operations Site (AOS) Operation Support Facility (OSF) 60 MB/s (peak) array scheduling + operations! quick-look, maintenance and repair 6 MB/s (average) issues of calls! PRC process! SB checks! pipeline data reduction! quality assessment! Population of the archive Santiago Central Office (SCO) Paola Andreani
3 High-level concepts for Science Operations Observations only in service observing mode with flexible (dynamic) scheduling.! Observations 24h/day interrupted by maintenance periods.! All observations executed in the form of scheduling blocks (SBs).! Default output: reliable images, calibrated according to the calibration plan.! The Joint ALMA Observatory (JAO) is responsible for the data product quality.! All science and calibration raw data are captured and archived.! Users interface is provided by the ALMA Regional Centres (ARCs)
4 ALMA Science Operations sites OSF, Santiago and the ARCs *Cvlle *Garching *Tokyo *ALMA site *Santiago
5 ALMA Operations: Three ALMA Regional Centres - ARCs Enhanced User Services NAASC Satellite EU ARCs EU ARC (ESO) NA ARC Enhanced services are needed to provide advanced user support, algorithm development, student programs, EPO, grants ARCs provide user interface, archive, software tools data delivery Astronomers on duty NAOJ Joint ALMA Observatory EA ARC JAO (Science Operations) provides: Array operations Scheduling of projects Execution of observations Data quality assurance and trend analysis Calibration plan maintenance Delivery of data to the archives Archive operations Pipeline operations
6 The ESO Paola Andreani
7 ARCs duties Commissioning/Astronomers on duty turnos (observing ES cycle 0 and on) Phase I: science portal, helpdesk, users documents, emergency helpdesk 72hrs before submission Proposal Review Process: Technical assessment (Chile workshops) Technical secretaries Phase II: preparajon of SBs (+documents, policies), contact scienjsts Data quality process: Assistance during quality assurance 2 (QA2) QA3 (feedback to JAO) Archive + Data delivery PI data reducjon help Paola Andreani
8 Phase I JAO issues CfP ARCs: user support + science portal ALMA DATA FLOW! Proposal Review Process: JAO + ARCs assistance Technical Feasibility JAO + ARCs Phase II ARCs: prepare SBs Contact scientists: PIs Data delivery ARCs Archive Long Term Queue JAO Quality Assurance: JAO + ARCs assistance Dynamical Scheduler: Short Term Queue Astronomer on duty (JAO+ARCs) Paola Andreani
9 ALMA Road Map Proposal Planning Help from documents in the SP (Primer, Technical Handbook, Guides, etc) Proposal PreparaJon (Phase I) Use of the ALMA Observing Tool Proposal Review Process Ranked according to scienjfic merit up to regional share No carryover from cycle 1 to cycle 2 Observing PreparaJon (Phase II) Observing plan (SBs) prepared by ARCs according to PIs wishes ObservaJons Schedule (according to weather/configurajons/etc) Post- observing/data ReducJon Quality assurance (JAO/ARCs) CASA package (- > ARC nodes)
10 The Science Portal: entry point to ALMA operations and users support User automajcally re- directed to regional SP
11 The helpdesk is the entry point to the EU ARC (ESO+nodes) See Evanthia s presentajon Contacts with the users done through the helpdesk. i.e. need face- to- face support? Use the Helpdesk.
12 The European ARC network! The European ARC! More in Martin s presentation ALMA Community days, Garching June The Atacama 2012! Large sub-millimetre Array Paola Andreani
13 Cycle 1 Operations Early Science through Cycle 1 (until construction and commissioning complete)! Priority is given to completion of the array: the time is shared with Commissioning activity.! Projects not carried over from Cycle 1 to later cycles! 12-month proprietary rights applicable to all ALMA data but Cycle 1 projects will not block later observations of the same targets with enhanced capabilities.! Scheduling of SBs done by the dynamic scheduler, used in manual mode! Data quality assurance done on best effort basis! No guarantee that the project will be completed! 13
14 Start of Cycle 1: Jan 1, 2013 Cycle 1 Length of Cycle 1: Nominally 10 months (finishes on Oct 31, 2013, followed by 2 month engineering period) Number of hours for observajons: Propose that the percent of Jme dedicated to science operajons increases from 33% in Cycle 0 to 60% in Cycle 1, i.e. 60% of the available Jme aber subtracjng engineering Jme and Jme lost due to weather and technical problems - in total about 800h + 800h ACA (maximum). Note: InauguraJon is expected to take place in March 2013 during Cycle 1 Paola Andreani
15 Cycle 1 observing modes the two main observing modes will be: single- - - field interferometry mosaics. Single- - - field interferometry : enhanced capability for dealing with muljple sources in a given region of the sky Mosaic: Maximum number of points: 150 per SB (150 per science goal) Spectral sweep: not offered Paola Andreani
16 AddiJonal LimitaJons Maximum number of sources per proposal (surveys): users can request to observe up to 15 individual sources in a single Science Goal, provided that the sources: (1) are not separated by more than 15 degrees on the sky (If sources are separated by more than 15 degrees on the sky there will be only one source per science goal) (2) can be observed with one spectral setup (placement and properjes of spectral windows), (3) can be observed with no more than five separate velocijes that all fall within the same receiver band. Paola Andreani
17 AddiJonal LimitaJons Maximum number of spectral setups per proposal (spectral surveys): Maximum 5 setups per Science Goal (SG) Maximum 5 SG s per proposal, i.e. in total a maximum of 25 spectral setups per proposal This gives a maximum number of 75 sources per proposal (if they are within 15 degrees in the sky) or 5 sources per proposal for sources separated by more than 15 degrees. Paola Andreani
18 Cycle 1 Programmes Standard Programmes ToO DDT Time crijcal observajons can be done with a scheduling fuzziness of 1-2 weeks Large Programmes will NOT be offered in Cycle 1 Highly rated Cycle 1 projects not observed in Cycle 1 will NOT be transferred to Cycle 2 Paola Andreani
19 Cycle 1 Jmeline April 3 : Announcement May 15: Deadline for submission of NoJces of Intent May 31: Call for proposal and opening of the archive July 13: Proposal submission deadline July 25- September 13: science assessments October: MeeJng of the science panels Mid October: Technical assessment Mid November: PI nojficajon and start of Phase II January 1 st : start of cycle 1 observajons February: Engineering period End October: end of cycle 1 Paola Andreani
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