4MOST – 4m Multi-Object Spectroscopic Telescope
www.4MOST.eu
Science OperationsC. Jakob Walcher (AIP)
date
“Science Operations”
• “Joint Operations Group“ (JOG): A group of people from the consortium who will run 4MOST operations in Europe.
• Separate from, but closely linked to ESO, who will run the instrument, VISTA, a public archive, select proposals, etc.
• The precursor to the JOG is called the “Operations Development Group” (ODG): talking to you now.
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Organisational view
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Science Team
ESO
4MOST Executive Board
4MOST Principal Investigator
Infrastructure Working Groups
Community Surveys
Consortium Surveys
ESO
Consortium
Community
Operations
Operations System
Science
Operations Manager
Data Management System
Consortium Helpdesk
ESO Archive (SAF)
Non-participating Surveys
Project Scientists
Joint Operations Group
On-mountain Operations
Technical support
Quality Control 1
ESO Instrument Scientist
Exposure Time Calculator Technical support
Policies Board(s)
Science Coordination Board
We are there to serve you!
We
You
Generalities / requirements
• MOS surveys covering a hemisphere in 5 years
• Consortium (“GTO”) and Community surveys
• Integrate into ESO operations model• Parallel survey execution for efficiency • 10s of millions of spectra• Public surveys
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Distinction between GTO and other surveys
• ESO requirement: No such distinction shall be made at any operations level.
• We are committed to this requirement.
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Requirements analysis for “participating” surveys• Parallel execution means
– Common observation preparations– Common selection function computation– Cross-talk on CCD, sharing of 1D spectra
• Survey sizes and duration mean– Automated observation preparation and data reduction– Accurate survey simulations for planning
• ESO instrument means– Use of ESO procedures (Phase 1,2,3, interfaces,
structure)– ESO oversight must be possible
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Principles of operations for participating surveys
• All participating surveys collaborate in the Science Team, also on science infrastructure
• Consortium Operations Group takes over tasks normally carried out by scientists
• Progress reporting and survey strategy parameterization allow ESO to exercise oversight role
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Non-participating (NP) surveys
• Some surveys may be able to fill all fibers of 4MOST within their sky area– No need for parallel observing– No common observation preparations– No common selection function computation– No cross-talk on CCD, sharing of 1D spectra– No participation in Science Team activities– Some consortium services not applicable
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Will start describing participating surveys, will highlight differences for NP surveys at end of talk.
Data levels
• Level zero (L0): raw data, calibration data, environmental data, log files.
• Level one (L1):1-dimensional, calibrated, science-ready spectra
• Level two (L2) data: products of science analysis of 1D spectra, in particular physical properties – L2 products that are to be delivered to ESO in
Phase 3 are deliverable L2 (DL2) products– Any survey may additionally generate additional L2
(AL2) products.
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How it would be if it was normal ESO operations
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Phase 3 process:!creation and publication !
of higher level data products!PI
Phase 1 process:!definition of 4MOST survey program!
ESO, community
Phase 2 process:!creation of OBs!
PI
Observing at Paranal!ESO
Target catalogues
Survey strategy OBs
Raw data
VISTA
4MOST
Data flow for participating surveys
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Definition of community surveys (ESO, proposals)
IWG work Writing papers
Definition of consortium
surveys
Phase 3 process:!creation of level 1 data products!
Consortium: Data Management System
Phase 1 process:!definition of 4MOST survey program!
ESO, consortium, community
Phase 2 process:!creation of OBs!
Consortium: Operations System
Progress tracking
Observing at Paranal!ESO
Phase 3 process B:!creation of level 2 data products!
Surveys, science team
Target catalogues
Survey strategy OBs
Raw data
1D spectra
Calibration strategy
Optimization processes
VISTA
4MOST
Submission to ESO
L2 products
Survey simulations
Creation of level 1 data products
Services for participating surveys
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Definition of community surveys (ESO, proposals)
IWG work Writing papers
Definition of consortium
surveys
Phase 3 process:!creation of level 1 data products!
Consortium: Data Management System
Phase 1 process:!definition of 4MOST survey program!
ESO, consortium, community
Phase 2 process:!creation of OBs!
Consortium: Operations System
Progress tracking
Observing at Paranal!ESO
Phase 3 process B:!creation of level 2 data products!
Surveys, science team
Target catalogues
Survey strategy OBs
Raw data
1D spectra
Calibration strategy
Optimization processes
VISTA
4MOST
Submission to ESO
L2 products
Survey simulations
Creation of level 1 data products
Science input and control
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Definition of community surveys (ESO, proposals)
IWG work Writing papers
Definition of consortium
surveys
Phase 3 process:!creation of level 1 data products!
Consortium: Data Management System
Phase 1 process:!definition of 4MOST survey program!
ESO, consortium, community
Phase 2 process:!creation of OBs!
Consortium: Operations System
Progress tracking
Observing at Paranal!ESO
Phase 3 process B:!creation of level 2 data products!
Surveys, science team
Target catalogues
Survey strategy OBs
Raw data
1D spectra
Calibration strategy
Optimization processes
VISTA
4MOST
Submission to ESO
L2 products
Survey simulations
Creation of level 1 data products
IWG2
Quality Control Scientist
IWG4,7,8,9
Preparing observations
• Operations System with components– 4MOST Facility Simulator (4FS)
• Heavy duty ETC (4FS-ETC)• Operations Simulation (OpSim)
– Observer Support Software (makes OBs)– Target and survey progress database
• IWG2 Survey Strategy– Development of requirements to survey strategy– Survey plan optimization
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Talk by R. De Jong
Taking calibration data
• Covered by regular calibration plan and L1 pipeline:– Day-time calibrations– Twilight flats– Night-time wavecal and fiber flat– Sky fibers and telluric standards– Use of Gaia targets for flux calibration
• Quality monitoring fields • Any other calibration (e.g. standard stars) have to be
submitted as (part of) OBs– Twilight calibrations (ca. half hour) are not counted – Night time calibration comes out of science time
(includes attached wavecal and fiber flat)
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Running observations
• VISTA+4MOST run by ESO TIO. • Participating surveys do not choose
conditions (e.g. seeing) per target. Exposure time adaptation to conditions, sky coverage according to survey plan.
• Optimal way of picking next OB still being discussed (area, depth, cadence).
• NP-surveys likely to be run in visitor mode
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Talk by V. Mainieri
Processing data (L1)
• Data Management System with major components– L1 pipeline– Progress measurement – Operational Repository– Public Archive
• Instrument Scientist / Quality Control Scientist / Survey teams provide QC
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Talk by N. Walton
Processing data (L2)
• Advanced pipelines– 4MOST Selection Functions pipeline (4SP)– 4MOST Galactic Pipeline (4GP)– 4MOST eXtragalactic Pipeline (4XP)– 4MOST Classification Pipeline (4CP)
• Instrument Scientist / Quality Control Scientist / Survey teams provide QC
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Talk by N. Walton
Processing data (IWGs)
• IWGs are organizationally under operations– close coordination with L1 pipeline– make sure data flow work throughout– apply best practices for heavy duty software
systems• The work is about science analysis and
requires surveys and PSs to take interest • The human resources for IWGs – come from the surveys (e.g. postdocs)– are delegated to operations
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Infrastructure Working Groups
Data / work flowlinearly
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Observation execution
Consortium surveys preparation
4MOST instrument
software and hardware
Community surveys preparation
Survey selectionSurvey confirmation
Observation preparation
Survey program optimization
Level 1: data reduction
Level 2: data analysis Operational repository
4MOST internal and public archive
Science archive facility
OB database
Quality control
Progress monitoring and scientific exploitation
Targets,scientific
requirements
Science archive facility
Worldwide science community
per target progress
Scientific guidance
proposalsproposals
ESO
Science Team
Operations
Legend
executable OBs (sci & cal)
OB to be executed
raw data (sci & cal)
raw data (sci & cal)
reduced level 1 spectralevel 1 spectra
level 2 productslevel 1 and 2 data
level 1 and 2 datalevel 1 and 2 data
level 1 and 2 data
Merge surveys into Science Team
ESO oversight
Survey parameters, target catalogues, progress monitor
Two main interfaces
Output
Input
Input target catalogue
• Input to simulations and observations is identical (but mock for sims OK)
• Input catalogue contains following information:– Target list with ruleset per object– Template spectra for calculating Texp from ruleset– Overall Figure of Merit for survey success– Merit functions for optimization purposes
• Observations will be run according to survey plan agreed between ESO and all surveys
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Output L1 and L2 data
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Talk by N. Walton
Feedback loops
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Observation execution
Consortium surveys preparation
4MOST instrument
software and hardware
Community surveys preparation
Survey selectionSurvey confirmation
Observation preparation
Survey program optimization
Level 1: data reduction
Level 2: data analysis Operational repository
4MOST internal and public archive
Science archive facility
OB database
Quality control
Progress monitoring and scientific exploitation
Targets,scientific
requirements
Science archive facility
Worldwide science community
per target progress
Scientific guidance
proposalsproposals
ESO
Science Team
Operations
Legend
executable OBs (sci & cal)
OB to be executed
raw data (sci & cal)
raw data (sci & cal)
reduced level 1 spectralevel 1 spectra
level 2 productslevel 1 and 2 data
level 1 and 2 datalevel 1 and 2 data
level 1 and 2 data
Merge surveys into Science Team
ESO oversight
Survey parameters, target catalogues, progress monitor
QC0
Loop 1: QC0, OB validityLoop 2: per target progress Loop 3: survey progress
Services for NP surveys
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Definition of community surveys (ESO, proposals)
IWG work Writing papers
Definition of consortium
surveys
Phase 3 process:!creation of level 1 data products!
Consortium: Data Management System
Phase 1 process:!definition of 4MOST survey program!
ESO, consortium, community
Phase 2 process:!creation of OBs!
Consortium: Operations System
Progress tracking
Observing at Paranal!ESO
Phase 3 process B:!creation of level 2 data products!
Surveys, science team
Target catalogues
Survey strategy OBs
Raw data
1D spectra
Calibration strategy
Optimization processes
VISTA
4MOST
Submission to ESO
L2 products
Survey simulations
Creation of level 1 data products
Services for non-participating surveys
• Provide Observer Support Software (OpSys)– Can be used to create Observation Blocks
(alternative to P2 web interface)– Training by consortium – NP-surveys have to run themselves
• Provide reduced L1 data (DMS)– Exact same data reduction procedures as ST– Assumes calibration strategy is same as ST– L1 data contain all calibration and provenance info– QCS for feedback in case of problems
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Service NOT offered to NP-surveys
• Front-end– No operations simulations beyond online 4FS, no
support in survey strategy development – No target and progress database / completion
tracking• Back-end– No processing beyond calibrated spectra per arm,
all additional processing science-specific – No measurement of success per OB or per target
– visitor mode! – No submission of Phase 3 on behalf of NP-survey – No access to Science Team L2 pipelines
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How to get help
• ESO USD– Usual level of support as for any other instrument– May use consortium Helpdesk as back-office
• Consortium Helpdesk– Reachable through mail ([email protected]) and
through the website www.4most.eu click on help. – Open to anyone: proposers, accepted surveys and
scientists, archive users, general public.– FAQ page and glossary.– This is the preferred way to address questions from
any science user: monitored, minimizes overheads.
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