ALMA Observing Activity from 2018-03-26T17:59:00 to 2018-04-02T18:00:00
QA0 pass executions
2018-04-02
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

11:32:38

12:00:57

2017.1.01117.SI19520_a_06_TM2

Study of the first O-type 'bloated star' Sanchez-Monge EU
candidate
Revealing the internal structure of
Pereira Santaella EU
molecular outflows: spatially resolved
observations in local LIRGs

12-m

6

11:09:34

11:32:28

2017.1.00255.S

IRASF171_a_06_TM2

12-m

6

09:43:06

10:59:26

2017.1.00023.S

IRAS_205_a_07_TM1

Understanding the role of infrared
Imanishiradiative pumping in ultraluminous
infrared galaxies
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

12-m

7

09:20:43

10:58:18

2017.1.00040.S

cnd_cs76_c_07_7M

EA

7-m

7

07:40:28

09:18:41

2017.1.00040.S

cnd_cs76_c_07_7M

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

7-m

7

06:45:46

08:01:172017.1.01243.S

SONYC-Lu_a_07_TM1 Brown dwarf disks demographics

06:16:21

06:42:09

2017.1.01235.S

UGC 9618_a_07_TM1

High Resolution Survey of the Gas
and Dust Distribution in Nearby
Luminous Infrared Galaxies

Testi

EU

12-m

7

Barcos-Munoz

NA

12-m

7

05:58:55

07:28:09

2017.1.00019.S

Lupus_3__a_06_7M

05:00:08

06:13:00

2016.1.00282.S

NBv1.43_a_07_TM1

04:39:23

05:58:48

2017.1.00886.L

NGC4569_a_06_7M

04:39:08

04:59:14

2017.1.01214.S

PJ132934_a_06_TM1

04:12:20

04:36:31

2017.1.00255.S

ESO319-G_a_06_TM2

Outflow structure of the young
Plunkett
NA
protostar Lupus 3 MMS
CH+ lines in starburst galaxies at
FalgaroneEUredshift z=2~4: probes of massive
turbulent gas reservoirs
100,000 Molecular Clouds Across the Schinnerer
EU NA
Main Sequence: GMCs as the Driversof Galaxy Evolution
ALMA Study of the Hyperluminous
Yun
NA
SMGs Identified from Planck All-Sky
SurveyRevealing the internal structure of
Pereira Santaella EU
molecular outflows: spatially resolved
observations in local LIRGs

7-m

6

12-m

7

7-m

6

12-m

6

12-m

6

03:44:58

04:06:38

2017.1.01276.S

12-m

6

2017.1.00255.S

COSMOS-H_f_06_TM1 Unveiling the nature of the most HST- Wang
EA
dark galaxies at z > 4
ESO267-G_a_06_TM2 Revealing the internal structure of
Pereira Santaella EU
molecular outflows: spatially resolved
observations in local LIRGs

03:16:08

03:43:30

12-m

6

02:05:07

03:13:22

2017.1.01618.S

11.20883_a_06_TM1

01:37:47

01:55:51

2017.1.01276.S

01:10:30

02:42:28

2017.1.00379.S

01:00:06

01:22:52

2017.1.00271.S

Start (UT)

End (UT)

21:09:55

Do there exist mini-SMGs at cosmic Kusakabe
noon?
COSMOS-H_g_06_TM1 Unveiling the nature of the most HST- Wang
dark galaxies at z > 4
ngc_3256_a_06_7M
Physical properties of dense gas in an Harada
AGN-driven outflow
Ridge_ce_b_03_TP
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

EA

12-m

6

EA

12-m

6

EA

7-m

6

NA

Total Power

3

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

22:07:54

2017.1.01512.S

ALESS001_d_03_TM1

Weiss

EU

12-m

3

20:38:34

21:43:07

2017.1.01158.S

12376570_a_06_7M

Gas mass fractions in z>3 main
sequence galaxies from ALESSACA Study on the Driving
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

Yamashita

EA

7-m

6

19:57:15

21:09:48

2017.1.01693.S

J032522._a_03_TM1

EA

12-m

3

19:23:40

20:38:27

2017.1.01350.S

TMC1_a_06_7M

EU

7-m

6

18:21:32

19:42:36

2017.1.00129.S

MCG-06-0_b_03_TP

Chronology of Episodic Accretion in Hsieh
Protostars - A survey of CO and H2Osnow lines
Imaging protostellar outflows Tychoniec
building a bridge between ALMA andJWSTDeep CO(J=1-0) mapping survey of Morokuma
Fornax galaxies with Morita array

EA

Total Power

3

18:16:00

19:27:56

2017.1.00202.S

SMG_C_a_03_TM1

EU

12-m

3

17:45:16

17:55:37

2017.1.00072.S

Sun_10_a_03_TP

The extent of (by far) the mostOteo
extreme starbursts in the early
Universe
How much do the cool components of Shimojo
solar X-ray jets

EA

Total Power

3

2018-04-01

contribute to the fast solar wind?
17:34:45

17:45:08

2017.1.00072.S

Sun_10_a_03_TP

17:24:16

17:34:39

2017.1.00072.S

Sun_10_a_03_TP

17:13:48

17:24:09

2017.1.00072.S

Sun_10_a_03_TP

17:03:18

17:13:40

2017.1.00072.S

Sun_10_a_03_TP

16:52:49

17:03:10

2017.1.00072.S

Sun_10_a_03_TP

16:42:20

16:52:42

2017.1.00072.S

Sun_10_a_03_TP

16:31:51

16:42:122017.1.00072.S

Sun_10_a_03_TP

16:17:07

16:27:27

2017.1.00072.S

Sun_10_a_03_TP

16:06:39

16:17:01

2017.1.00072.S

Sun_10_a_03_TP

15:56:07

16:06:32

2017.1.00072.S

Sun_10_a_03_TP

15:47:10

17:50:18

2017.1.00072.S

Sun_10_a_03_INT

15:45:43

15:56:01

2017.1.00072.S

Sun_10_a_03_TP

15:35:21

15:45:38

2017.1.00072.S

Sun_10_a_03_TP

15:22:52

15:33:13

2017.1.00072.S

Sun_10_a_03_TP

15:12:21

15:22:45

2017.1.00072.S

Sun_10_a_03_TP

15:01:49

15:12:15

2017.1.00072.S

Sun_10_a_03_TP

14:51:20

15:01:42

2017.1.00072.S

Sun_10_a_03_TP

14:40:48

14:51:122017.1.00072.S

Sun_10_a_03_TP

14:30:16

14:40:41

2017.1.00072.S

Sun_10_a_03_TP

14:19:43

14:30:08

2017.1.00072.S

Sun_10_a_03_TP

14:07:32

14:17:53

2017.1.00072.S

Sun_10_a_03_TP

13:56:27

14:07:28

2017.1.00072.S

Sun_10_a_03_TP

13:45:01

13:56:19

2017.1.00072.S

Sun_10_a_03_TP

13:43:44

15:47:05

2017.1.00072.S

Sun_10_a_03_INT

11:53:24

12:48:02

2017.1.00478.S

SDSS_J22_a_06_TM1

11:49:46

13:06:55

2017.1.01116.S

G08.670-_a_06_7M

11:04:05

11:27:52

2017.1.01085.S

NGC6907_a_07_TM1

How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
Feedback and Star Formation in
HamannExtremely Red Quasars
High Resolution Imaging of Inflow & Shirley
Infall in Massive Star-forming Clumps

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

12-m

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

Total Power

3

EA

12-m

3

NA

12-m

6

NA

7-m

6

The Excitation of Dense

NA

12-m

7

PrivonMolecular Gas Tracers in Local
Infrared Luminous Starbursts
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

10:12:30

11:40:06

2017.1.00040.S

cnd_cs76_e_07_TP

EA

Total Power7

10:02:26

11:03:59

2017.1.01243.S

CRBR15_a_07_TM1

Brown dwarf disks demographics

09:26:14

10:53:06

2017.1.01355.L

W43-MM2_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Testi

EU

12-m

7

Motte

CL EA EU NA

7-m

6

09:24:49

10:02:10

2017.1.01545.S

HD_13961_a_06_TM1

08:40:55

10:11:58

2017.1.01355.L

W43-MM3_a_06_TP

The first molecular line inventory inhybrid disks
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Henning

EU

12-m

6

Motte

CL EA EU NA

Total Power6

08:11:39

09:24:35

2017.1.01243.S

SONYC-Lu_a_07_TM1 Brown dwarf disks demographics

08:08:02

09:25:21

2017.1.00886.L

NGC6300_a_06_7M

Testi

EU

12-m

7

EU NA

7-m

6

07:29:04

08:40:48

2017.1.00040.S

cnd_cs54_d_06_TP

EA

Total Power

6

06:56:37

08:06:07

2016.1.00639.S

MSDM_29._a_07_TM1 Physical Properties of Galaxies that Martin
Ionize the Universe
IRAS_162_a_07_TM1 A comprehensive inventory of
Wampfler
nitrogen isotopic ratios in a nascentsolar system
IRAS_162_a_07_7M
A comprehensive inventory of
Wampfler
nitrogen isotopic ratios in a nascentsolar system
BRI1202-_b_05_TM1
Water, water everywhere, Nor a drop Lehnert
to drink: Solving the riddle of the mostluminous water emitters known

NA

12-m

7

05:59:57

06:53:34

2017.1.01565.S

EU

12-m

7

05:28:00

07:14:43

2017.1.01565.S

EU

7-m

7

04:32:58

05:34:43

2017.1.01516.S

EU

12-m

5

03:53:15

05:13:35

2017.1.00886.L

NGC4569_a_06_7M

EU NA

7-m

6

04:29:32

2017.1.01516.S

BRI1202-_b_05_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Water, water everywhere, Nor a drop Lehnert
to drink: Solving the riddle of the mostluminous water emitters known

03:23:43

EU

12-m

5

02:18:00

02:53:09

2017.1.00022.S

IRAS_121_a_05_TM1

AGN feedback and molecular line flux Imanishi
ratios in luminous infrared galaxies

EA

12-m

5

02:14:13

03:46:32

2017.1.00379.S

ngc_3256_a_06_7M

EA

7-m

6

01:31:22

02:17:45

2017.1.00022.S

IRAS_085_a_05_TM1

Physical properties of dense gas in an Harada
AGN-driven outflow
AGN feedback and molecular line flux Imanishi
ratios in luminous infrared galaxies

EA

12-m

5

01:19:05

02:13:36

2017.1.00527.S

G09.v10._i_06_7M

The molecular gas and resolved star- Oteo
formation law in low-redshift SMGs

EU

7-m

6

00:21:15

01:11:39

2017.1.00379.S

ngc_3256_a_06_7M

Physical properties of dense gas in an Harada
AGN-driven outflow

EA

7-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:45:32

00:42:10

2017.1.00478.S

SDSS_J08_a_06_TM1

Hamann

NA

12-m

6

14:32:05

16:02:26

2017.1.01621.S

el_gordo_a_03_7M

Basu

EU

7-m

3

14:09:46

15:37:23

2017.1.01158.S

VV642_a_06_TP

Feedback and Star Formation in
Extremely Red Quasars
ALMA reveals the full extent of theearliest known merger shock
ACA Study on the Driving
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

Yamashita

EA

Total Power

6

13:16:10

14:20:07

2017.1.00510.S

SGP38326_a_04_TM1

Oteo

EU

12-m

4

12:34:54

14:09:20

2017.1.01355.L

W43-MM3_a_06_TP

The ISM of the most luminous
starbursts in the early Universe
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power

6

12:16:31

13:44:51

2017.1.01355.L

G010.62_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

7-m

6

11:20:39

12:44:06

2017.1.00793.S

G14.225S_a_06_TM1

Are Magnetic Fields Dynamically
Zhang
Important in Massive Star Formation ?

NA

12-m

6

11:02:24

11:59:23

2017.1.00180.S

6334_-_M_a_06_7M

Define the physic of high-mass starformation from the cold Hershel
sources of the NGC6334

CL

7-m

6

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

2018-03-31

Louvetcomplex
10:51:58

12:15:22

2017.1.01355.L

G012.80_a_06_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

10:17:14

10:48:15

2017.1.00040.S

cnd_cs54_d_06_TP

10:11:53

11:20:32

2017.1.00793.S

09:27:54

11:01:30

08:35:42

Motte

CL EA EU NA

Total Power

6

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power6

G14.225S_a_06_TM1

Are Magnetic Fields Dynamically
Zhang
Important in Massive Star Formation ?

NA

12-m

6

2017.1.01355.L

G010.62_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

7-m

6

10:11:46

2017.1.00793.S

G14.225S_a_06_TM1

Are Magnetic Fields Dynamically
Zhang
Important in Massive Star Formation ?

NA

12-m

6

07:56:47

09:27:47

2017.1.00661.S

NGC6334I_a_04_7M

BroganNA7-m

4

07:49:54

08:26:49

2017.1.01355.L

G008.67_a_06_TM1

Testing predictions of stellar cluster
formation in NGC6334I
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

12-m

6

07:43:54

08:55:18

2017.1.00040.S

cnd_cs54_d_06_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power6

07:08:44

07:47:53

2017.1.01355.L

G328.25_a_06_TM1

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

12-m

6

06:34:30

07:08:38

2017.1.01355.L

G327.29_a_06_TM1

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

12-m

6

06:22:49

07:56:39

2017.1.00716.S

G340.39_a_06_7M

A survey of prestellar, high-mass
clump candidates: constraining
models of high-mass star formation

Sanhueza

EA

7-m

6

05:46:54

06:32:40

2017.1.00510.S

UR56917_a_04_TM1

EU

12-m

4

04:29:09

05:31:08

2017.1.01020.S

D3a-1550_a_04_TM1

The ISM of the most luminous
Oteo
starbursts in the early Universe
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

04:21:00

05:37:04

2017.1.00886.L

NGC4569_a_06_7M

EU NA

7-m

6

03:21:08

04:29:02

2017.1.01020.S

zC-40056_a_04_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

02:46:10

04:10:57

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

01:58:45

03:05:58

2017.1.01020.S

D3a-1550_a_04_TM1

Mapping Molecular ISM in the Whole Koda
Disk of M83
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

00:56:33

02:21:51

2017.1.00230.S

NGC_2903_a_03_7M

Dense Gas Tracers, Star Formation, Leroy
Cloud Properties, and Galaxy
Structure in Five Nearby Spiral
Galaxies

NA

7-m

3

00:39:16

01:41:31

2017.1.00893.S

C-C-451_a_03_TM1

SUPER-ALMA v2: gas fractions and Mainieri
depletion timescales in AGN hosts at
z~2

EU

12-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

22:04:27

22:37:36

2017.1.01100.S

SPT0348-_c_03_TM1

An Unprecedented Census of the
Molecular ISM in Starburst Galaxies
at the End of Cosmic Reionization

Aravena

CL

12-m

3

21:34:54

22:32:01

2017.1.00271.S

Ridge_NW_b_03_TP

Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

21:11:44

21:55:122017.1.01100.S

SPT0348-_c_03_TM1

An Unprecedented Census of the
Molecular ISM in Starburst Galaxies
at the End of Cosmic Reionization

Aravena

CL

12-m

3

20:59:08

22:26:26

2017.1.00765.S

TMC1A_a_04_7M

Harsono

EU

7-m

4

20:10:11

21:11:38

2017.1.00138.S

Large-scale infalling envelopes
through cold gas tracers
CANDELS__c_03_TM1 Wide ASPECS: Bridging the gap
between targeted observations andmolecular deep fields

Decarli

EU

12-m

3

Motte

2018-03-30

11:18:40

12:12:05

2017.1.01355.L

W51-E_a_03_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

11:12:03

12:12:02

2017.1.01704.S

B28539_a_03_7M

10:32:04

11:36:08

2017.1.00594.S

HD181327_a_03_TM1

08:27:39

09:46:33

2017.1.01355.L

07:52:47

09:04:07

07:09:43

Motte

CL EA EU NA

Total Power3

A systematic survey of dense gas
Svobodakinematics and filamentary flows inmassive quiescent clumps
Probing non-uniform dust production Olofsson
rate in a young debris disk

NA

7-m

3

CL

12-m

3

G012.80_a_06_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power6

2017.1.00729.S

M17_SW_a_03_TM1

McGuire

NA

12-m

3

08:27:31

2017.1.01355.L

G012.80_a_06_TP

Unlocking the Potential of the Most
Definitive Molecular Tracer of UVEnhancement: l-C3H+
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power

605:33:53

06:51:37

2017.1.00886.L

NGC4571_b_06_TP

EU NA

Total Power

605:30:13

06:54:31

2017.1.00079.S

M83_e_03_7M

NA

7-m

3

05:21:23

06:15:27

2017.1.01694.S

NAv1.195_a_03_TM1

EU

12-m

3

04:23:33

05:14:41

2017.1.01694.S

NAv1.195_a_03_TM1

EU

12-m

3

04:14:29

05:32:25

2017.1.00886.L

NGC4571_b_06_TP

EU NA

Total Power

604:04:21

05:29:01

2017.1.00079.S

M83_e_03_7M

NA

7-m

3

03:07:07

04:15:00

2017.1.00893.S

C-C-451_a_03_TM1

EU

12-m

3

00:14:45

01:07:36

2017.1.00893.S

CID-247_a_03_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Mapping Molecular ISM in the Whole Koda
Disk of M83
A dense molecular gas survey at high Oteo
redshift
A dense molecular gas survey at high Oteo
redshift
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Mapping Molecular ISM in the Whole Koda
Disk of M83
SUPER-ALMA v2: gas fractions and Mainieri
depletion timescales in AGN hosts at
z~2
SUPER-ALMA v2: gas fractions and Mainieri
depletion timescales in AGN hosts at
z~2

EU

12-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

21:54:17

22:31:23

2017.1.00271.S

Ridge_ce_b_03_TP

Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

21:22:10

22:23:42

2017.1.00138.S

EU

12-m

3

20:59:26

22:29:00

2017.1.00230.S

CANDELS__c_03_TM1 Wide ASPECS: Bridging the gap
Decarlibetween targeted observations andmolecular deep fields
NGC_1672_a_03_7M
Dense Gas Tracers, Star Formation, Leroy
Cloud Properties, and Galaxy
Structure in Five Nearby Spiral
Galaxies

NA

7-m

3

20:36:58

21:44:21

2017.1.00271.S

Ridge_ce_b_03_TP

Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

19:57:09

20:52:31

2017.1.00161.L

ngc253_f_03_TM1

EA EU NA12-m

3

19:19:49

20:49:33

2017.1.00230.S

NGC_1672_a_03_7M

ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
Dense Gas Tracers, Star Formation, Leroy
Cloud Properties, and Galaxy
Structure in Five Nearby Spiral
Galaxies

NA

7-m

3

19:15:21

20:36:51

2017.1.00129.S

FCC44_a_03_TP

Deep CO(J=1-0) mapping survey ofFornax galaxies with Morita array

EA

Total Power

3

19:01:39

19:57:02

2017.1.00161.L

ngc253_f_03_TM1

EA EU NA12-m

3

17:55:24

19:01:33

2017.1.00161.L

ngc253_b_03_TM1

EA EU NA12-m

3

17:54:30

19:15:13

2017.1.00129.S

FCC32_a_03_TP

ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
Deep CO(J=1-0) mapping survey of Morokuma
Fornax galaxies with Morita array

EA

Total Power

3

17:53:19

19:19:42

2017.1.01621.S

el_gordo_a_03_7M

EU

7-m

3

16:09:36

17:36:122017.1.01621.S

el_gordo_a_03_7M

EU

7-m

3

15:28:40

16:35:13

2017.1.00161.L

ngc253_b_03_TM1

ALMA reveals the full extent of theBasuearliest known merger shock
ALMA reveals the full extent of theBasuearliest known merger shock
ALCHEMI: the ALMA Comprehensive Martin
High-resolution

EA EU NA

12-m

3

2018-03-29
PI

MorokumaExtragalactic Molecular Inventory
14:42:27

16:09:28

2017.1.01621.S

el_gordo_a_03_7M

ALMA reveals the full extent of theBasuearliest known merger shock
ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
DEATH STAR: DEtermining Accurate Ramstedt
mass-loss rates of THermally pulsing
AGB STARs
Caught in the act - the formation of a Eales
cluster core at z~4
IBISCO-south: mapping feeding and Feruglio
feedback in an unbiased sample oflocal AGNHigh Resolution Imaging of Inflow & Shirley
Infall in Massive Star-forming Clumps

EU

7-m

3

14:08:53

15:14:42

2017.1.00161.L

ngc253_b_03_TM1

EA EU NA12-m

3

13:53:10

14:31:27

2017.1.00595.S

IRC-3039_a_06_7M

EU

7-m

6

12:59:21

14:07:23

2017.1.00033.S

Source_6_c_03_TM1

EU

12-m

3

12:28:16

12:56:25

2017.1.01439.S

igrj1937_a_06_TM1

EU

12-m

6

12:24:09

13:52:29

2017.1.01116.S

G33.738-_a_03_7M

NA

7-m

3

11:18:59

12:09:59

2017.1.01355.L

W51-E_a_03_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

Total Power3

11:02:37

11:56:59

2017.1.00523.S

I19368_a_03_TM1

Gas accretion onto dense cores from Lu
early to late evolutionary phases ofmassive filamentary clouds

EA

12-m

3

10:34:57

12:07:36

2017.1.01355.L

G010.62_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

7-m

6

10:07:06

11:02:30

2016.1.00345.S

IRAS_185_a_03_TM2

The Disk/FLow System in the Massive HofnerProtostar IRAS 18566+0408

NA

12-m

3

09:56:18

11:18:05

2017.1.01355.L

G353.41_a_06_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

Total Power6

09:16:40

10:34:49

2017.1.01380.S

Oph-D_a_03_7M

EU

7-m

3

09:01:44

09:56:20

2017.1.00523.S

I18308_a_03_TM1

Are dense cores formed throughPinedashocks? An observational test in
Ophiuchus
Gas accretion onto dense cores from Lu
early to late evolutionary phases ofmassive filamentary clouds

EA

12-m

3

08:18:39

09:54:20

2017.1.01355.L

G337.92_a_06_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

Total Power6

07:59:14

08:54:37

2017.1.00523.S

I18308_a_03_TM1

Gas accretion onto dense cores from Lu
early to late evolutionary phases ofmassive filamentary clouds

EA

12-m

3

07:05:36

08:30:28

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

06:58:38

08:18:32

2017.1.01355.L

G353.41_a_06_TP

Mapping Molecular ISM in the Whole Koda
Disk of M83
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

Total Power

6

06:47:04

07:57:22

2017.1.01542.S

G339.88-_a_03_TM1

Rosero

NA

12-m

3

05:38:45

06:45:43

2017.1.01542.S

G339.88-_a_03_TM1

Rosero

NA

12-m

3

05:26:02

06:58:31

2017.1.01355.L

G327.29_a_03_TP

Outflow and Infall to Massive
Protostars
Outflow and Infall to Massive
Protostars
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power

3

04:57:57

06:22:27

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

04:30:00

05:32:00

2017.1.00518.S

IRAS_162_a_03_TM1

EU

12-m

3

04:13:00

05:25:54

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power3

04:11:13

04:28:10

2017.1.01572.S

4C_21.35_a_03_TM2

NA

12-m

3

03:16:24

04:09:43

2017.1.00893.S

CID-970_a_03_TM1

EU

12-m

3

02:59:36

04:12:52

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power

3

02:51:01

04:13:52

2017.1.00771.S

NGC4038_a_03_7M

EU

7-m

3

02:22:56

03:16:172017.1.00893.S

CID-970_a_03_TM1

EU

12-m

3

Motte

Motte

Motte

Motte

Mapping Molecular ISM in the Whole Koda
Disk of M83
C-C-Complexity in solar massvan Dishoeck
protostars; pushing the limit
A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
ALMA Observations of Resolved
Meyer
Extragalactic Jets in a Critically
Unsampled Spectral Window
SUPER-ALMA v2: gas fractions and Mainieri
depletion timescales in AGN hosts at
z~2
A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Adjusting the Reception of The
Sliwa
Antennae: A Clear Look at GMCs in a
Major Merger
SUPER-ALMA v2: gas fractions
Mainieriand depletion timescales in AGN
hosts at z~2
Recovering Extended Structures in
Ueda
Merger RemnantsSUPER-ALMA v2: gas fractions and Mainieri
depletion timescales in AGN hosts at
z~2

01:39:19

02:59:29

2017.1.01003.S

AM_1158-_b_03_TP

NA

Total Power3

01:29:23

02:22:49

2017.1.00893.S

LID-1852_a_03_TM1

EU

12-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

19:10:19

20:36:172017.1.00129.S

FCC44_a_03_TP

Deep CO(J=1-0) mapping survey ofFornax galaxies with Morita array

Morokuma

EA

Total Power

3

18:34:39

19:40:36

2017.1.00161.L

ngc253_b_03_TM1

ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
ALMA reveals the full extent of theBasuearliest known merger shock
Deep CO(J=1-0) mapping survey of Morokuma
Fornax galaxies with Morita array

EA EU NA12-m

3

18:07:05

18:46:49

2017.1.01621.S

el_gordo_a_03_7M

EU

7-m

3

17:44:34

19:10:01

2017.1.00129.S

FCC32_a_03_TP

EA

Total Power

3

17:38:30

18:34:18

2017.1.00161.L

ngc253_e_03_TM1

ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
ALMA reveals the full extent of theBasuearliest known merger shock
ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
Dense Gas Tracers, Star Formation, Leroy
Cloud Properties, and Galaxy
Structure in Five Nearby Spiral
Galaxies

EA EU NA12-m

3

16:40:20

18:06:58

2017.1.01621.S

el_gordo_a_03_7M

EU

7-m

3

16:08:50

17:09:05

2017.1.00161.L

ngc253_e_03_TM1

EA EU NA12-m

3

16:07:14

17:31:04

2017.1.00230.S

NGC_0628_a_03_TP

NA

Total Power

3

15:03:35

16:30:122017.1.01621.S

el_gordo_a_03_7M

ALMA reveals the full extent of theearliest known merger shock
A unique and massive z=4.3
protocluster from the South Pole
Telescope 2500 deg^2 survey
ACA Study on the Driving
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

Basu

EU

7-m

3

14:43:43

15:58:23

2017.1.00273.S

spt2349-_b_03_TM1

Chapman

NA

12-m

3

14:33:01

15:56:22

2017.1.01158.S

VV642_a_06_TP

Yamashita

EA

Total Power

6

13:39:51

15:03:02

2017.1.00687.S

G038.95-_a_03_7M

From filaments to cores: Dynamics in Barnes
infrared dark clouds
A unique and massive z=4.3
Chapmanprotocluster from the South Pole
Telescope 2500 deg^2 survey
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

EU

7-m

3

13:18:07

14:32:49

2017.1.00273.S

spt2349-_b_03_TM1

NA

12-m

3

12:59:25

14:29:23

2017.1.01355.L

W43-MM3_a_06_TP

CL EA EU NA

Total Power

6

11:56:34

12:59:58

2017.1.01355.L

G010.62_a_06_TM1

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

12-m

6

11:51:58

12:51:00

2017.1.00040.S

cnd_cs43_d_05_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power5

11:09:33

12:36:49

2017.1.01355.L

W43-MM2_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

7-m

6

10:30:03

11:24:13

2017.1.00040.S

cnd_cs54_b_06_TM1

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

12-m

6

10:13:31

10:29:44

2016.1.00209.S

OO_Ser_a_06_TM2

EA

12-m

6

10:03:19

11:37:16

2017.1.01355.L

W43-MM3_a_03_TP

Multi-scale disk and envelope
Takamikinematics around the most extremely
accreting young stars
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

Total Power3

09:49:25

11:09:26

2017.1.01355.L

G008.67_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

7-m

6

09:19:55

10:13:18

2017.1.00040.S

cnd_cs54_a_06_TM1

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

12-m

6

08:14:17

09:19:45

2017.1.01355.L

G010.62_a_06_TM1

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

12-m

6

07:16:11

08:17:31

2017.1.00180.S

6334_-_M_a_06_7M

Define the physic of high-mass starformation from the cold

LouvetCL

7-m

6

2018-03-27

Motte

Motte

Motte

07:05:33

08:11:14

2017.1.00518.S

IRAS_162_a_03_TM1

06:35:35

08:05:11

2017.1.01355.L

G328.25_a_03_TP

05:50:23

07:14:34

2017.1.00079.S

M83_e_03_7M

05:48:14

06:55:25

2017.1.01616.S

SN2011ke_a_03_TM1

05:19:10

06:29:25

2017.1.00886.L

NGC4689_b_06_TP

04:34:59

05:46:29

2017.1.01109.S

SDSS_J13_a_04_TM1

04:23:19

05:48:01

2017.1.00079.S

M83_e_03_7M

04:03:47

05:16:39

2017.1.00815.S

NGC_4321_a_03_TP

03:16:39

04:19:26

2017.1.00560.S

PKS-1017_a_04_TM1

02:50:42

04:03:19

2017.1.00815.S

NGC_4321_a_03_TP

02:50:06

04:13:06

2017.1.00815.S

NGC_4321_a_03_7M

Start (UT)

End (UT)

Project Code22:23:52

23:40:11

21:24:48

Hershel sources of the NGC6334
complex
C-C-Complexity in solar mass
protostars; pushing the limit
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

van Dishoeck

EU

12-m

3

Motte

CL EA EU NA

Total Power

3

Mapping Molecular ISM in the Whole Koda
Disk of M83
Superluminous Supernova HostKim
galaxies in CO - Assessing Molecular
Gas in Nascent Starbursts

NA

7-m

3

CL

12-m

3

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
How universal are surprisingly
Bezansonsignificant molecular gas reservoirs inmassive post-starburst galaxies at
z~0.6?

EU NA

Total Power

6

NA

12-m

4

Mapping Molecular ISM in the Whole Koda
Disk of M83
A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Unveiling dusty star-forming galaxies Arrigoni Battaia
and probing multiple AGN within a
giant Lyman-alpha nebula at z=3.167

NA

7-m

3

NA

Total Power

3

EU

12-m

4

A Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
A Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results

Gallagher

NA

Total Power

3

Gallagher

NA

7-m

3

SchedBlock

Project Title

PI

Executive

Array

Band

2017.1.00823.S

Cloud_6_a_03_7M

How do GMCs start to form massive Ochsendorf
stars? An ALMA survey of young,massive star forming GMCs in the
LMC

NA

7-m

3

22:26:25

2017.1.00138.S

EU

12-m

3

20:20:04

21:31:20

2017.1.00271.S

CANDELS__c_03_TM1 Wide ASPECS: Bridging the gap
Decarlibetween targeted observations andmolecular deep fields
Ridge_ce_b_03_TP
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

20:14:53

21:16:33

2017.1.00138.S

CANDELS__c_03_TM1 Wide ASPECS: Bridging the gap
between targeted observations andmolecular deep fields

EU

12-m

3

2018-03-26

Decarli