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12m array7m arrayTP arrayBand 6 is the popular band, followed by Band 3 and 7.
Fraction of high frequency bands is still small.

4CIEMCE .ASE N IER

12m array7m arrayTP array

7TLBE N RTBLISSED O NONRAKR OE
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4 accepted out of 22 submitted proposals

1. ALMA-IMF: ALMA transforms our view of the origin of stellar
masses PI: Frederique Motte (EU); co-PIs: Adam Ginsburg (NA),
Patricio Sanhueza (EA), and Fabien Louvet (CL)
2. 100,000 Molecular Clouds Across the Main Sequence: GMCs as the
Drivers of Galaxy Evolution PI: Eva Schinnerer (EU); co-PIs: Adam
Leroy (NA), Guillermo Blanc (NA), Erik Rosolowsky (NA), Andreas
Schruba (EU), and Annie Hughes (EU)
3. ALCHEMI: the ALMA Comprehensive High-resolution Extragalactic
Molecular Inventory PI: Franceso Costagliola (EU); co-PIs Nanase
Harada (NA/EA) and Jeffrey Mangum (NA)
4. ALPINE: The ALMA Large Program to INvestigate CII at Early times
PI: Olivier Le Fèvre (EU); co-PIs: Andreas Faisst (NA), Daniel Schaerer(EU), John Silverman (EA), Paolo Cassata (CL), Lin Yan (NA), Peter
Capak (NA), and Matthieu Bethermin (EU)8NONRAKRNONRAKR EPTI IM SHE ILLEDIASE NBRE UASINM
N A RTDDEM AMD TMEWOECSED ARS NMNLICAK EUEMSNONRAKR EPTERSIM NBRE UASINMR NM A HI HK
CNLOESISIUE RCIEMSI IC SNOIC LNSIUASED B
DEUEKNOLEMSR SHAS HAUE SAJEM OKACE A SE SHEE TKA O NONRAK RTBLIRRINM DEADKIMENONRAKR ARJIM N NKKNV TO NBRE UASINMR N AO N AL ECEMSK CNMDTCSED VISH ,5 , N AM
NSHE NBRE UIM ACIKIS VHE E A PTICJILOKELEMSASINM IR EWOECSED SN O NUIDEB EAJSH NT H ERTKSR

9,5 , CIEMCETSOTS

Number of ALMA related presentations at the ASJ Meetings
8072706160
5040323020374139231002014 F

2015S

2015F

2016S2016F

2017S2017F

10,5 ,N JRHNORPurpose: To promote community-led ALMA science activities that will lead tostrong and competitive ALMA proposals from the EA region. Call for workshop
proposals occur twice a year (evaluated with 2 JSAC members).
2016a2016b

2017a

2017b

ALMA Deep Survey
WS 2016 (Kohno)

ALMA Stellar WS(Izumiura)

Gaseous Debris Disk WS(Higuchi)

Protoplanetary Disk(Akiyama)

Extensive CO Surveyof Nearby Galaxies
with ACA (Egusa)

ALMA WS for Solar System
Planetary Obs. (Sagawa)Star Formation with
ALMA (Tokuda)

WS on Solar System(Sagawa)Obs of Debris Disk
with ALMA (Higuchi)

Mm/THz Receiver WS(Sakai)
Scientific Potential of
ALMA Solar Obs (Shimojo)
ALMA Workshop on M83(Hirota)
Protoplanetary Disk Obs
with ALMA (Tsukagoshi)

ALMA Stellar WS (Imai)110, ,5 , CIEMCEN JRHNO• Five ALMA-JT meetings were held prior to 2012
• September 12-13, 2012, KASI, Korea• 54 participants• September 2-4, 2013, ASIAA, Taiwan• 80 participants• July 14-17, 2014, Jeju Island, Korea• 84 participants• December 8 – 11, 2015, I-site, Osaka, Japan• 107 participants• March 10-12, 2016, ASIAA, Taiwan• 110 participants• November 27-29, 2017, KASI
• 94 participants• Late 2018, Japan

12

CIEMCE ,DUIRN.NLLISSEER

ALMA boardCharges

Meeting Report

ASAC (12)- 2 f2f meeting per year
- Monthly telecons

comments, opinions
EASAC

ANASACEASAC (25)

Chilean SAC

EUcommunity

NAcommunity

EA
community

Chilecommunity

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