ALMA Observing Activity from 2019-05-27T17:59:00 to 2019-06-03T18:00:00
QA0 pass executions
2019-06-03
Start (UT)

End (UT)

Project CodeSchedBlock

Project Title

11:34:57

13:17:192018.1.01670.S

SPT0113-_a_08_7M

09:40:11

11:34:482018.1.01670.S

08:42:20

10:17:34

07:05:52

PI

Executive

Array

Band

Building a sample of [NII] 122 and 205 Cunningham
micron emission lines in high-z dusty
star forming galaxies

NA7-m

8

SPT0020-_a_08_7M

Building a sample of [NII] 122 and 205 Cunningham
micron emission lines in high-z dusty
star forming galaxies

NA7-m82018.1.01687.S

Ser-emb1_a_08_TP

EU

Total Power808:41:37

2018.1.01687.S

Ser-emb1_a_08_TP

EU

Total Power806:25:12

08:15:50

2018.1.01670.S

SPT2146-_a_08_7M

Resolving the complete outflow
Zhang
density and kinematics structures byobserving [CI] (1-0)
Resolving the complete outflow
Zhang
density and kinematics structures byobserving [CI] (1-0)
Building a sample of [NII] 122 and 205 Cunningham
micron emission lines in high-z dusty
star forming galaxies

NA7-m

805:29:40

07:05:45

2018.1.01687.S

Ser-emb8_a_08_TP

EU

Total Power

805:01:4205:39:22

2018.1.00994.S

IRASF_17_b_08_7M

EA7-m

803:50:4405:01:08

2018.1.00994.S

Arp220_b_08_7M

EA7-m

803:38:07

05:29:35

2018.1.01687.S

HH108_a_08_TP

EU

Total Power

802:20:48

03:37:59

2018.1.01259.S

BGPS3474_a_06_TP

Resolving the complete outflow
Zhang
density and kinematics structures byobserving [CI] (1-0)
CI(1-0) and CO(4-3) survey for nearby Michiyama~40 U/LIRGs- Band8 ACA standalone observation CI(1-0) and CO(4-3) survey for nearby Michiyama~40 U/LIRGs- Band8 ACA standalone observation Resolving the complete outflow
Zhang
density and kinematics structures byobserving [CI] (1-0)
Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NA

Total Power

601:27:07

02:11:54

2018.1.00318.S

PDR_in_O_a_08_TP

Yamagishi

EA

Total Power

800:41:14

02:40:54

2018.1.00633.S

HD121191_a_08_7M

Revealing the overall picture ofcarbon atoms in the ideal planeparallel PDR Oph-A[C I] observations toward gaseousdebris disks with ACA

Higuchi

EA7-m

8Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:59:18

01:26:58

2018.1.00318.S

PDR_in_O_a_08_TP

EA

Total Power

8

23:11:4200:41:04

2018.1.00994.S

IC_4280_a_08_7M

EA7-m

8

22:50:38

23:59:11

2018.1.00697.S

Nessie_F_h_03_TP

EU

Total Power

3

21:08:21

22:01:52

2018.1.00994.S

IRAS_F10_b_08_7M

EA7-m

8

20:22:05

21:02:14

2018.1.00994.S

NGC_3110_b_08_7M

EA7-m

8

17:35:09

19:28:082018.1.01023.S

rostad1_a_07_7M

Revealing the overall picture ofYamagishi
carbon atoms in the ideal planeparallel PDR Oph-A
CI(1-0) and CO(4-3) survey for nearby Michiyama~40 U/LIRGs- Band8 ACA standalone observation Do spiral-arm clouds fragment
Hacar
dynamically or gravitationally?
CI(1-0) and CO(4-3) survey for nearby Michiyama~40 U/LIRGs- Band8 ACA standalone observation CI(1-0) and CO(4-3) survey for nearby Michiyama~40 U/LIRGs- Band8 ACA standalone observation Star-birth in Irradiated Environments: Sahai
Free-Floating EGGs in the Rosette

NA7-m

7

15:34:33

17:27:21

2018.1.01023.S

rostad1_a_07_7M

Star-birth in Irradiated Environments: Sahai
Free-Floating EGGs in the Rosette

NA7-m

7

13:30:35

14:32:37

2017.A.00054.S

NGC_346_l_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

6

12:27:59

13:30:27

2017.A.00054.S

NGC_346_q_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

6

11:20:53

12:20:13

2017.A.00054.S

NGC_346_f_03_7MACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

3

10:20:34

11:20:13

2017.A.00054.S

NGC_346_d_03_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

3

2019-06-02

07:20:20

08:37:28

2018.1.01259.S

BGPS3474_a_06_TP

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power6

07:14:44

08:31:11

2018.1.01804.S

IRDC_G35_a_03_7M

OTHER

7-m

3

06:06:13

07:20:122018.1.01259.S

BGPS6120_a_06_TP

Are supersonic linewidths in massive Yuestar formation regions intrinsicallysubsonic?
Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power605:53:30

07:14:39

2018.1.01804.S

IRDC_G35_a_03_7M

OTHER7-m

3

04:48:02

06:06:05

2018.1.01259.S

BGPS3474_a_06_TP

Are supersonic linewidths in massive Yuestar formation regions intrinsicallysubsonic?
Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power604:29:07

05:53:23

2018.1.01851.S

G316.75-_b_03_7MThe impact of O-type stars on gas
dynamics: The case of the G316.75
massive-star forming ridge

Watkins

EU7-m

3

03:31:28

04:47:55

2018.1.01259.S

BGPS3474_a_06_TP

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power

603:04:43

04:29:00

2018.1.01851.S

G316.75-_b_03_7M

The impact of O-type stars on gas
dynamics: The case of the G316.75
massive-star forming ridge

EU7-m

3

01:42:48

03:31:21

2018.1.00215.S

P1_a_04_TP

The sequential star formation towards Feng
the IR bright rim of an HII bubble

EATotal Power

4

01:39:52

03:04:35

2018.1.01851.S

G316.75-_b_03_7M

The impact of O-type stars on gas
dynamics: The case of the G316.75
massive-star forming ridge

Watkins

EU7-m

3

00:02:27

01:26:01

2018.1.01243.S

Southern_a_03_7M

A detailed map of the variation ofdensity, temperature and photodissociated gas across the Carina
Nebula

Garay

CL7-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArray

Band

14:52:27

15:54:53

2017.A.00054.S

NGC_346_w_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

6

13:01:28

14:03:56

2017.A.00054.S

NGC_346_aj_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

6

11:51:24

12:53:39

2017.A.00054.S

NGC_346_y_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

6

10:48:42

11:51:16

2017.A.00054.S

NGC_346_as_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

609:41:40

11:07:02

2018.1.01259.S

BGPS6310_b_06_TP

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NA

Total Power608:23:14

09:41:33

2018.1.00101.S

G28.5413_a_03_TP

The initial gas flow towards extremely Feng
young high-mass clumps

EA

Total Power

308:04:40

09:21:03

2018.1.01804.S

IRDC_G35_a_03_7M

OTHER

7-m

3

07:01:58

08:23:072018.1.00862.S

G5_b_06_TP

NA

Total Power

606:43:26

08:04:33

2018.1.01804.S

IRDC_G35_a_03_7M

OTHER

7-m

305:36:51

07:01:51

2018.1.01259.S

BGPS3053_b_06_TP

Are supersonic linewidths in massive Yuestar formation regions intrinsicallysubsonic?
Perfect Twins? Excited Molecular Gas Ott
Clumps Symmetric to Sgr A*
Are supersonic linewidths in massive Yuestar formation regions intrinsicallysubsonic?
Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power

605:22:28

06:43:18

2018.1.01804.S

IRDC_G35_a_03_7M

OTHER7-m

3

04:21:13

05:36:44

2018.1.01091.S

M17_a_06_TP

Are supersonic linewidths in massive Yuestar formation regions intrinsicallysubsonic?
Mapping M17: the best galactic
Reiterlaboratory for measuring the role

NATotal Power

6Watkins

2019-06-01

of photoionizing feedback
04:00:04

05:20:33

2018.1.01851.S

G316.75-_a_03_7M

The impact of O-type stars on gas
dynamics: The case of the G316.75
massive-star forming ridge

Watkins

EU7-m

3

03:00:53

04:21:06

2018.1.00862.S

G5_b_06_TP

NA

Total Power

602:08:35

03:29:082018.1.01851.S

G316.75-_a_03_7M

Perfect Twins? Excited Molecular Gas Ott
Clumps Symmetric to Sgr A*
The impact of O-type stars on gas
Watkins
dynamics: The case of the G316.75
massive-star forming ridge

EU7-m

301:50:05

03:00:45

2018.1.00697.S

Nessie_F_g_03_TP

Hacar

EUTotal Power

301:07:43

02:08:28

2018.1.00473.S

J133947._a_06_7M

Do spiral-arm clouds fragment
dynamically or gravitationally?
Mapping CO emission in galaxies
from the JINGLE survey

WilsonNA7-m6Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArrayBand

11:39:12

12:41:28

2017.A.00054.S

NGC_346_u_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mappingEU7-m

6

10:35:57

11:38:02

2017.A.00054.S

NGC_346_ap_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mapping

EU7-m

6

10:25:24

11:21:482018.1.00101.S

G34.7798_a_03_TP

The initial gas flow towards extremely Feng
young high-mass clumps

EATotal Power309:33:21

10:35:48

2017.A.00054.S

NGC_346_ay_06_7M

ACA Observatory Project: SMC Band Agliozzo
6 CO and continuum mappingEU7-m

608:55:54

10:25:172018.1.01259.S

BGPS6310_b_06_TP

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power608:15:56

09:33:122017.1.00523.S

I19220_a_03_7M

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

EA7-m

3

07:01:35

08:55:47

2018.1.00215.S

P1_a_04_TP

The sequential star formation towards Feng
the IR bright rim of an HII bubble

EATotal Power

406:58:22

08:15:48

2017.1.00523.S

I19220_a_03_7M

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

EA7-m

3

05:50:3307:01:27

2018.1.00697.S

Nessie_F_f_03_TP

Hacar

EUTotal Power

304:52:09

06:17:13

2018.1.01851.S

G316.75-_a_03_7M

Do spiral-arm clouds fragment
dynamically or gravitationally?
The impact of O-type stars on gas
dynamics: The case of the G316.75
massive-star forming ridge

Watkins

EU7-m

3

04:38:34

05:49:22

2018.1.00697.S

Nessie_F_f_03_TP

Hacar

EU

Total Power

303:28:37

04:38:02

2018.1.00697.S

Nessie_F_i_03_TP

Hacar

EUTotal Power

303:02:07

04:22:36

2018.1.01851.S

G316.75-_a_03_7M

Do spiral-arm clouds fragment
dynamically or gravitationally?
Do spiral-arm clouds fragment
dynamically or gravitationally?
The impact of O-type stars on gas
dynamics: The case of the G316.75
massive-star forming ridge

WatkinsEU7-m

302:19:13

03:28:30

2018.1.00697.S

Nessie_F_i_03_TP

Hacar

EUTotal Power

302:01:27

03:02:00

2018.1.00473.S

J133947._a_06_7M

WilsonNA7-m601:09:14

02:17:312018.1.00697.S

Nessie_F_i_03_TP

Hacar

EUTotal Power

300:41:57

02:01:22

2018.1.01833.S

GL_555_a_06_7M

Do spiral-arm clouds fragment
dynamically or gravitationally?
Mapping CO emission in galaxies
from the JINGLE survey
Do spiral-arm clouds fragment
dynamically or gravitationally?
The disks around low-mass stars inthe solar neirborhoodCaceres

CL7-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArray

Band

22:55:56

00:21:312018.1.01003.S

VelaC-CR_a_06_7M

The Role of Magnetic Fields within
FisselDense Molecular Filaments in Vela C

NA7-m

6

10:20:37

11:26:072018.1.00101.S

G34.7798_a_03_TP

The initial gas flow towards extremely Feng
young high-mass clumps

EATotal Power3

08:42:15

10:20:30

2018.1.00299.S

G28_a_03_TP

Infall in the very early stages of high- Contreras
mass star formation

EUTotal Power

3

2019-05-31

2019-05-30

08:41:33

09:58:41

2017.1.00523.S

I19220_a_03_7M

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

EA

7-m

3

07:05:01

08:39:51

2018.1.00215.S

P1_a_04_7M

The sequential star formation towards Feng
the IR bright rim of an HII bubble

EA7-m

4

06:25:18

08:07:58

2018.1.00299.S

G10_a_03_TP

Total Power

3

05:38:38

07:03:14

2018.1.01142.S

PSZ1_031_a_04_7M

7-m

4

05:31:07

06:19:05

2018.1.00299.S

G10_a_03_TP

Total Power3

04:13:52

05:38:312018.1.01142.S

PSZ1_031_a_04_7M

7-m

4

04:05:35

05:28:00

2018.1.01171.S

NGC_6300_a_03_TP

Total Power

302:53:29

04:13:45

2018.1.01851.S

G316.75-_a_03_7M

Infall in the very early stages of high- Contreras
EUmass star formation
Exploring the molecular gas andGonzález López CL
continuum emission in giant
gravitational arcs
Infall in the very early stages of high- ContrerasEUmass star formation
Exploring the molecular gas andGonzález López CL
continuum emission in giant
gravitational arcs
An ACA Survey of Dense Gas Across, Leroy
NA
the Nearest, Brightest Southern
Galaxy Disks
The impact of O-type stars on gas
Watkins
EUdynamics: The case of the G316.75
massive-star forming ridge

7-m

3

02:41:59

04:04:27

2018.1.01171.S

NGC_6300_a_03_TP

Total Power3

01:28:51

02:53:21

2018.1.01142.S

PSZ1_031_a_04_7M

7-m

4

01:20:0902:38:17

2018.1.01171.S

NGC_6300_a_03_TP

Total Power

300:01:11

01:24:34

2018.1.01243.S

Southern_a_03_7M

An ACA Survey of Dense Gas Across, Leroy
NA
the Nearest, Brightest SouthernGalaxy Disks
Exploring the molecular gas andGonzález López CL
continuum emission in giant
gravitational arcs
An ACA Survey of Dense Gas Across, Leroy
NA
the Nearest, Brightest Southern
Galaxy Disks
A detailed map of the variation ofGarayCL
density, temperature and photodissociated gas across the Carina
Nebula7-m

3Start (UT)

End (UT)

Project Code

SchedBlockProject Title

ExecutiveArrayBand

13:48:18

15:26:312018.1.00525.S

B1-c_a_04_7M

Linking large- and small-scale organic Bergner
chemistry in Solar-type protostars

NA7-m

4

10:04:31

11:23:25

2018.1.01259.S

BGPS5623_b_06_7M

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NA7-m

6

09:53:14

11:07:40

2018.1.01259.S

BGPS6120_a_06_TP

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NATotal Power

608:33:47

09:53:072018.1.01091.S

M17_b_06_TPNA

Total Power

608:30:09

10:04:24

2018.1.00215.S

P1_a_04_7M

Mapping M17: the best galacticReiterlaboratory for measuring the role ofphotoionizing feedback
The sequential star formation towards Feng
the IR bright rim of an HII bubble

EA7-m

4

07:12:14

08:33:41

2018.1.00862.S

G5_b_06_TPNA

Total Power

607:10:27

08:30:03

2018.1.01259.S

BGPS4449_b_06_7M

Perfect Twins? Excited Molecular Gas Ott
Clumps Symmetric to Sgr A*Probing the Structure and Chemistry Wilkinsof Previously Unexplored Giant
Molecular Clouds

NA7-m605:55:18

07:10:192018.1.01259.S

BGPS3474_b_06_7M

Probing the Structure and Chemistry Wilkins
of Previously Unexplored Giant
Molecular Clouds

NA7-m

6

04:30:49

05:55:11

2018.1.01142.S

PSZ1_031_a_04_7M

7-m

4

04:00:32

05:28:41

2018.1.00850.S

G028.67+_a_03_TP

Total Power

3

03:10:24

04:30:422018.1.01851.S

G316.75-_a_03_7M

Exploring the molecular gas andGonzález López CL
continuum emission in giant
gravitational arcs
From filaments to cores: Dynamics in Barnes
EUinfrared dark clouds
The impact of O-type stars on gas
Watkins
EUdynamics: The case of the G316.75
massive-star forming ridge

7-m

3

02:48:25

04:00:25

2018.1.00299.S

G341.03_a_03_TPEU

Total Power

301:46:13

03:06:172018.1.00940.S

A1835_a_03_7M

Infall in the very early stages of high- Contreras
mass star formation
SZ observations of 3 Cool-Core
Mroczkowski

EU7-m

3

2019-05-29
PIClusters on the Sloshing Spectrum
01:36:35

02:48:18

2018.1.00299.S

G341.03_a_03_TP

Infall in the very early stages of high- Contreras
mass star formation
SZ observations of 3 Cool-Core
Mroczkowski
Clusters on the Sloshing Spectrum

EU

Total Power

300:31:56

01:46:06

2018.1.00940.S

A1835_a_03_7M

EU7-m

300:29:30

01:33:38

2018.1.00697.S

Nessie_F_f_03_TP

Do spiral-arm clouds fragment
dynamically or gravitationally?

Hacar

EU

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:25:28

00:29:24

2018.1.00697.S

Nessie_F_i_03_TP

Hacar

EU

Total Power

3

22:53:52

00:17:27

2018.1.01243.S

Southern_a_03_7M

Do spiral-arm clouds fragment
dynamically or gravitationally?
A detailed map of the variation ofdensity, temperature and photodissociated gas across the Carina
Nebula

Garay

CL7-m

3

20:51:13

22:10:13

2018.1.01243.S

Southern_a_03_7M

A detailed map of the variation ofdensity, temperature and photodissociated gas across the Carina
Nebula

Garay

CL7-m

3

19:27:31

20:51:04

2018.1.01243.S

Southern_a_03_7M

A detailed map of the variation ofdensity, temperature and photodissociated gas across the Carina
Nebula

Garay

CL7-m

3

2019-05-28