1 anasac meeting – may 20, 2015 p. jewell, j. hibbard, c. lonsdale cycle 1 & 2 status &...

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1 ANASAC Meeting – May 20, 2015 P. Jewell, J. Hibbard, C. Lonsdale Cycle 1 & 2 Status & Cycle 3 results

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1 ANASAC Meeting – May 20, 2015

P. Jewell, J. Hibbard, C. Lonsdale

Cycle 1 & 2 Status & Cycle 3 results

2 ANASAC Meeting – May 20, 2015

CYCLE 1, 2 STATUS

3 ANASAC Meeting – May 20, 2015

Observing ProgressNumber of Executions by Array component (Mar 11)

3

Cycle 1 Cycle 2

Start of Cycle 2

Long baselinecampaign

Start of Cycle 2

4 ANASAC Meeting – May 20, 2015

Observing ProgressNumber of Executions by Priority Grade (Mar 11)

4

Cycle 1 Cycle 2

Start of Cycle 2

Long baselinecampaign

Start of Cycle 2

5 ANASAC Meeting – May 20, 2015

NA ALMA User SupportObserving Progress (NA only, as of May 19)

6 ANASAC Meeting – May 20, 2015

Assignment of backlog that built up waiting for start of PL processing

NA caught up with initial PL backlog

Assignment of all post-LBC datasets prior to Cy3 call

NA caught up with assignments prior to Cy3 call

Steady-state goal: ~43 OUS/mo

7 ANASAC Meeting – May 20, 2015

Cycle 1 & 2 CompletionProjects

As of May 19:

8 ANASAC Meeting – May 20, 2015

Cycle 1 & 2 CompletionObsUnitSets (=datasets)

As of May 19:

9 ANASAC Meeting – May 20, 2015

Status – ALMA Telescope OperationsProject and OUS Completion Status by Executive (May 19)

10 ANASAC Meeting – May 20, 2015 10

Requested and Remaining Time L Nyman. As of March 11, all Executives

Total requested time Total remaining time

Cycle 1 Highest: 532 h Remaining = 252h (47%)Cycle 2 A+B: 1672 h Remaining = 1103h (66%)Hours remaining = as of Feb/Mar engineering time

~325hrs observed since

11 ANASAC Meeting – May 20, 2015ALMA Board meeting at SCO 11

Prediction of Completion

• As of March 11: 1355 hrs of 2200 hrs remain– ~325 hrs observed ES blocks 17-21– 13 ES block remain ~ 800 hrs (~60hr QA0 pass

per block)– Implies 230 hrs unobserved => ~90% completion

• However:– Some projects simply cannot be scheduled due to

inability to do high frequency observations (> band 7) during the day• Compact configurations, LST~0h – 5h

• Extended configurations, LST~5h – 10h

– Other projects are in oversubscribed LSTs

March 11, 2015

12 ANASAC Meeting – May 20, 2015 12

LST pressure per configuration L Nyman. As of March 11

C34-1C34-1 C34-3C34-2

C34-5C34-4

C34-7

C34-6

| | | . | |0h 5h 10h 15h 20h

LST

The black horizontal lines in the figures indicate the distribution of available time according to the current array configuration schedule

APRIL APRIL & MAY MAY

JUNE AUG & SEP

JUN, JUL, AUG, SEP

MAY?

13 ANASAC Meeting – May 20, 2015 13

LST pressure per configuration L Nyman. As of March 11

C34-1C34-1 C34-3C34-2

C34-5C34-4

C34-7

C34-6

| | | . | |0h 5h 10h 15h 20h

LST

The black horizontal lines in the figures indicate the distribution of available time according to the current array configuration schedule

APRIL APRIL & MAY MAY

JUNE AUG & SEP

JUN, JUL, AUG, SEP

MAY?

14 ANASAC Meeting – May 20, 2015 14

Prediction of Completion (best case)L. Nyman, March 11

• Cycle 1: 16 projects unlikely to be observed (52 h)– 92% completion rate

• Cycle 2: 32 projects unlikely to be observed (121 h) – 91% completion rate

• Total: 48 projects unlikely to be observed (173 h)– 91% completion rate

• Most likely 4 Cycle 2 grade A projects will be transferred to Cycle 3

March 11, 2015 ALMA Board meeting at SCO

15 ANASAC Meeting – May 20, 2015

Executive Balance – Cycle 0

16 ANASAC Meeting – May 20, 2015

Executive Balance – Cycle 1(as of Feb/Mar Engineering time)

Regional Share: 33.8% 33.8% 22.5% 10.0% (<5%)✓

17 ANASAC Meeting – May 20, 2015

• At increased ES observing frequency and efficiencies, Data reduction is straining resources at the ARCs– JAO is streamlining processes– NA is hiring more staff

• While TP observing has begun, TP data reduction path has still not been proven and distributed to ARCs

• No group-level data combination has been performed; “best practices” not established– NAASC is doing this individually via helpdesk & in-person

visits (6 cases). About to roll out a CASAguide

Cycle 1 & 2 Status: Challenges

18 ANASAC Meeting – May 20, 2015

CYCLE 3 RESULTS

19 ANASAC Meeting – May 20, 2015

ALMA Proposal Cycles

• Cycle 0: Sep 2011-Dec 2012 (990 proposals, 500h)• Cycle 1: Jan 2013-May 2014 (1131 proposals, 800h)• ~300 hrs transferred into Cycle 2

• Cycle 2: Jun 2014-Oct 2015 (1382 proposals, 1700 h)• Cycle 3 – Deadline was April 23• PRP meetings: June 22-26, 2015 (in Osaka, JP)• Communication of Outcome of Review Process: August

2015• Start of Cycle 3: October 1, 2015 – Start of yearly cycles

20 ANASAC Meeting – May 20, 2015

Cycle 3 Proposal ProcessImprovementsSeveral improvements were made to assist investigators

– Cycle 3 Array schedule published in Proposers Guide– Document improvements

• Better explanations of multiple pointing and multiple tuning choices

• Improved calibration chapter in the Technical Handbook

– Helpdesk and Knowledgebase• “Cycle 3 News” top-level menu item on SP points to KB article

that accumulates known issues • Included graphics for some KB articles• Helpdesk staffed for entire week prior to deadline, and 72h of

continuous “follow-the-sun” emergency department (twice that of Cycle 2)

– Questionnaire released much sooner, closing end May• 340 replies to date

21 ANASAC Meeting – May 20, 2015

22 ANASAC Meeting – May 20, 2015

23 ANASAC Meeting – May 20, 2015

Cycle 3 Observing Capabilities and Policies• Cycle 3 begins 1 October. • Cycle 3 is no longer Best Efforts for standard proposals

– New category: Non-standard = Bands 8, 9 10 or baselines > 2.5 km

• With Cycle 3, ALMA begins a 12 month proposal cycle• Supplement to C (filler) projects: low frequency and under-subscribed LST

ranges• Capabilities for Cycle 3 (new / extended capabilities marked in red):

– At least thirty-six 12-m antennas in the main array, and ten 7-m antennas and two 12-m antennas (for single-dish maps) in the ACA.

– Receiver bands 3, 4, 6, 7, 8, 9, & 10 (wavelengths of about 3.1, 2.1, 1.3, 0.87, 0.74, 0.44, and 0.35 mm, respectively).

– Baselines up to 2 km for Bands 8, 9 and 10. – Baselines up to 5 km for Band 7. – Baselines up to 10 km for Bands 3, 4, & 6.– Both single field interferometry and mosaics.– Spectral-line observations with all Arrays and continuum observations with the 12-m

Array and the 7-m Array. TP Array use is limited to spectral line observations in Bands 3 to 8.

– Polarization (on-axis, continuum in Band 3, 6 and 7, no spectral line, no ACA, no mosaics, no circular polarization).

– Mixed correlator modes (both high and low frequency resolution in the same observation).

– The maximum observing time per proposal, as estimated by the OT, is 100 hours.

24 ANASAC Meeting – May 20, 2015

Proposal Submission for Cycle 3

1612 Proposal codes were assigned by the deadline on April 23, 2015 from around the world

25 ANASAC Meeting – May 20, 2015

Helpdesk Support• More complete coverage in week up to deadline• 365 tickets in total (178=49% for NA)

25

26 ANASAC Meeting – May 20, 2015

Cycle 3 Proposal Submission

• 1582 unique proposals (+14%) requesting 9037 hrs on the 12-m Array – 5.7 hrs per proposal– Oversubscription by hours = 4.3– 76% / 24% hrs requested “standard” / “non-

standard”• 1122 individual PIs and 3608 PI+Co-Is from 47

countries

27 ANASAC Meeting – May 20, 2015

Cycle 3 Proposal Statistics

28 ANASAC Meeting – May 20, 2015

Proposal ProcessFuture improvements

• Improvements to KB articles, including graphics• Revision of Primer and “Did You Know” flyer to include updated

and more accessible example observations• Videos to explain some of the more complex setups• More information on use of simulators with more examples

Starting the Cycle 4 planning earlier in the cycle if the data reduction schedule allows

29 ANASAC Meeting – May 20, 2015

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