ALMA Observing Activity from 2024-03-25T17:59:00 to 2024-04-01T18:00:00
QA0 pass executions
2024-04-01
Start (UT)

End (UT)

Project CodeSchedBlock

Project Title

15:45:55

16:09:40

2023.1.00443.S

PS1J0000_a_06_TM1

15:28:52

15:45:04

2023.1.00443.S

15:02:31

15:18:16

14:39:40

PI

Executive

Array

Band

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources at
z>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m

6

PS1J0006_a_06_TM1

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources atz>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m62023.1.00443.S

DESJ0020_a_06_TM1

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources at
z>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m6

14:55:23

2023.1.00443.S

PS1J2256_a_06_TM1

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources at
z>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m6

14:19:35

14:35:36

2023.1.00443.S

HSCJ2255_a_06_TM1

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources atz>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m

6

14:05:02

15:15:102023.1.01150.S

G034.13_a_06_TPA Survey of Infall in the Very Early
Morii
Stages of High-Mass Star Formation

EATotal Power

6

13:39:54

14:16:15

2023.1.00334.S

RXJ1842._a_07_TM2

Measuring accurate gas masses forthe exoALMA planet-forming disks

Trapman

NA12-m7

13:19:00

13:34:16

2023.1.00443.S

PS1J2222_a_06_TM1

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources atz>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m

6

12:55:08

13:18:31

2023.1.00443.S

HSCJ2223_a_06_TM1

Delivering the Needed Large Samples Bouwensof Extremely High SFR Sources atz>6 to Characterize Early
Stellar+Black-Hole GrowthEU12-m6

12:52:55

14:04:54

2019.1.01400.S

W28_c_06_TP

A Quest for the Formation Mechanism Sanoof Molecular Filaments

EATotal Power

611:40:32

12:52:47

2019.1.01400.S

W28_c_06_TP

A Quest for the Formation Mechanism Sanoof Molecular Filaments

EATotal Power

611:25:33

12:32:54

2023.1.00038.S

G+0.693_a_01_TM1

EU12-m1

10:32:04

11:40:26

2023.1.01246.S

SerpS-MM_a_03_TPEU

Total Power

3

10:11:20

11:19:03

2023.1.00038.S

G+0.693_a_01_TM1

EU12-m1

09:09:50

10:31:59

2023.1.01515.S

DHNb61_a_06_TP

Complex organic imaging towards
MartinG+0.693-0.027, the ISM COMs
Rossetta Stone
The cold chemistry of protostellar hot Jorgensen
corinos
Complex organic imaging towards
MartinG+0.693-0.027, the ISM COMs
Rossetta Stone
Detailed observations of theEnokiya
magnetically intertwined Double Helix
Nebula in the Galactic CenterEATotal Power608:50:52

09:53:15

2023.1.01327.S

EA12-m4

08:32:43

09:09:442023.1.01246.S

EUTotal Power

3

07:48:10

08:50:49

2023.1.00329.S

W44_SW_2_a_04_TM1 Propagation of cosmic rays inNobukawa
molecular clouds interacting with asupernova remnant
SerpS-MM_a_03_TP
The cold chemistry of protostellar hot Jorgensen
corinos
ACT-CL_J_a_03_TM1 High-Resolution SZ Study of aDi Mascolo
Potential Phoenix-like Galaxy Cluster

EU12-m3

07:21:04

08:32:37

2023.1.01246.S

SerpS-MM_b_03_TPEU

Total Power

306:33:43

07:40:41

2023.1.00329.S

ACT-CL_J_a_04_TM1

The cold chemistry of protostellar hot Jorgensen
corinos
High-Resolution SZ Study of aDi Mascolo
Potential Phoenix-like Galaxy Cluster

EU12-m4

05:16:40

06:28:23

2023.1.00202.S

Northern_a_03_TP

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

NATotal Power

3

05:09:18

06:08:37

2023.1.01668.S

RXJ1347._c_01_TM1

One-percent precision measurement Kitayamaof the Sunyaev-Zel'dovich Effect

EA12-m104:25:25

05:16:36

2023.1.00052.S

Region1_a_03_TP

The effect of the massive stellar
feedback across the Carina

NATotal Power

3Rebolledo

Nebula Complex
03:49:01

04:55:19

2023.1.01668.S

RXJ1347._a_01_TM1

One-percent precision measurement Kitayamaof the Sunyaev-Zel'dovich Effect

EA12-m1

03:13:20

04:25:212023.1.00202.S

Northern_a_03_TP

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

NATotal Power3

01:06:40

01:55:482023.1.00202.S

Northern_a_03_TP

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

NA

Total Power

300:13:03

01:03:59

2023.1.00052.S

Region1_a_03_TP

The effect of the massive stellar
feedback across the Carina NebulaComplex

Rebolledo

NA

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:22:20

00:40:092023.1.00527.S

OrionKL-_a_01_TM1

EA

12-m

1

22:09:23

23:21:54

2023.1.00527.S

EA

12-m

1

20:47:18

22:00:212023.1.00527.S

EA12-m1

20:00:15

20:16:51

2023.1.01066.S

Decouple ion RRLs of Helium,
Lee
Carbon, and Oxygen in the Orion KLM42 region
OrionKL-_a_01_TM1
Decouple ion RRLs of Helium,
Lee
Carbon, and Oxygen in the Orion KLM42 region
OrionKL-_a_01_TM1
Decouple ion RRLs of Helium,
Lee
Carbon, and Oxygen in the Orion KLM42 region
SVA1_COA_a_04_TM1 Growing Brighest Cluster Galaxies: a Webb
statistical study of the molecular fuelat early times

NA12-m4

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArray

Band

14:03:14

15:21:26

2023.1.01101.S

NGC7319_a_03_7M

Maeda

EA7-m

3

12:36:31

14:03:11

2021.1.00960.S

4C23.56_a_04_7M

ACA CO(1-0) mapping of Stephan's
QuintetDetecting extended [CI] emission inthe 4C23.56 protocluster at z=2.5

LeeEU7-m

4

11:30:00

12:38:18

2023.1.00038.S

G+0.693_a_01_TM1

MartinEU12-m1

09:55:37

11:04:562023.1.00040.S

G31.41+0_a_03_TM1

Complex organic imaging towards
G+0.693-0.027, the ISM COMs
Rossetta Stone
Angular momentum in hub-filament
systems: Deciphering signatures ofrotation and global collapse.

Beltran

EU12-m3

09:30:10

10:50:45

2023.1.00467.S

G28.28-0_a_03_7M

EA7-m

3

08:48:57

09:54:34

2023.1.00329.S

ACT-CL_J_a_04_TM1

What is the trigger of the chemical
Taniguchi
diversity around massive young stellar
objects?
High-Resolution SZ Study of aDi Mascolo
Potential Phoenix-like Galaxy Cluster

EU12-m4

07:56:09

09:29:34

2023.1.01464.S

2MASX_J1_b_05_7M

NA7-m

5

07:45:01

08:53:19

2023.1.01246.S

SerpS-MM_a_03_TPEU

Total Power

3

07:41:23

08:48:53

2023.1.00329.SACT-CL_J_a_04_TM1

Identifying the Brightest Continuum Rose
Sources Accessible to ALMA with theACA
The cold chemistry of protostellar hot Jorgensen
corinos
High-Resolution SZ Study of aDi Mascolo
Potential Phoenix-like Galaxy Cluster

EU12-m4

06:34:15

07:41:19

2023.1.00329.S

ACT-CL_J_a_04_TM1

High-Resolution SZ Study of aDi Mascolo
Potential Phoenix-like Galaxy Cluster

EU12-m4

06:29:28

07:52:26

2023.1.01493.S

NGC4321_a_03_7M

7-m

3

05:24:38

06:23:27

2023.1.01668.S

RXJ1347._c_01_TM1

Resolving N2H+(1-0) emission for the Jimenez-Donaire EU
first time across the galaxy disk ofM100
One-percent precision measurement Kitayama
EAof the Sunyaev-Zel'dovich Effect

12-m

1

05:06:38

06:29:24

2023.1.01493.S

NGC4321_a_03_7M

7-m

3

04:25:06

05:24:132023.1.01668.S

RXJ1347._c_01_TM1

Resolving N2H+(1-0) emission for the Jimenez-Donaire EU
first time across the galaxy disk ofM100
One-percent precision measurement Kitayama
EAof the Sunyaev-Zel'dovich Effect

12-m

1

03:43:40

05:06:34

2023.1.01493.S

NGC4321_a_03_7M7-m

3

02:20:34

03:43:35

2023.1.01493.S

NGC4321_a_03_7M

Resolving N2H+(1-0) emission for the Jimenez-Donaire EU
first time across the galaxy disk ofM100
Resolving N2H+(1-0) emission for the Jimenez-Donaire EU
first time across the7-m

32024-03-31

2024-03-26

galaxy disk of M100
01:19:00

02:24:57

2023.1.00882.S

Spiderwe_a_01_TM2

Physics of the cold circumgalactic
Emontsmedium in the Spiderweb: new high-z
science with ALMA Band-1

NA12-m1

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

ExecutiveArrayBand

21:36:06

22:46:072023.1.00213.S

J0459.6-_a_03_TM1

The Sunyaev-Zel'dovich effect toward Kitayama
a distant galaxy cluster at z=1.7

EA

12-m

3

19:32:55

20:34:19

2023.1.01425.S

SMC_Bar_l_03_7M

Investigation of the molecular
Chenenvironment that caused fewer highmass stars in the Small Magellanic
CloudEU

7-m

3

18:28:33

19:32:422023.1.01425.S

SMC_Bar_l_03_7M

Investigation of the molecular
Chenenvironment that caused fewer highmass stars in the Small Magellanic
CloudEU7-m

3

2024-03-25
PI