ALMA Observing Activity from 2019-06-24T17:59:00 to 2019-07-01T18:00:00
QA0 pass executions
2019-06-30
Start (UT)

End (UT)

Project CodeSchedBlock

Project Title

19:41:09

20:37:26

2018.A.00047.S

iras_071_c_03_7M

18:41:19

19:40:38

2018.A.00047.S

Start (UT)

End (UT)

11:49:43

PI

Executive

Array

Band

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

iras_065_c_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

Project Code

SchedBlock

Project Title

ExecutiveArrayBand

13:09:58

2018.1.00525.S

B1-c_a_04_7M

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

NA7-m

4

10:12:56

11:46:192018.A.00046.S

elaiss11_a_06_7M

EU7-m

6

09:20:19

10:12:47

2018.A.00047.S

DS_Aqr_b_03_7M

The host properties and environment Messiasof high-redshift radio galaxies withACA
Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

08:19:51

09:20:10

2018.A.00047.S

HM_Aqr_b_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

04:45:37

05:53:11

2018.1.00981.S

Northeas_a_03_7M

Xiong

NA7-m

3

02:28:05

03:44:39

2018.1.00981.S

Northeas_a_03_7M

Xiong

NA7-m

3

01:01:36

02:27:56

2018.1.00697.S

Nessie_F_i_03_7M

Evolutionarily Young Filamentary
Region of NGC 6334
Evolutionarily Young Filamentary
Region of NGC 6334
Do spiral-arm clouds fragment
dynamically or gravitationally?

Hacar

EU7-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArrayBand

23:15:2100:41:48

2018.1.00697.S

Nessie_F_i_03_7M

EU7-m

3

21:26:16

22:06:38

2018.A.00047.S

V510_Pup_a_03_7M

Do spiral-arm clouds fragment
Hacar
dynamically or gravitationally?
Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

21:02:38

22:26:39

2018.1.01218.S

TW_Hya_a_03_TM1

NA12-m3

20:36:43

21:21:21

2018.A.00047.S

V510_Pup_d_03_7M

Disk substructures in TW Hya:
Macias
Optically Thick or Large Grains?
Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

19:46:23

20:28:39

2018.A.00047.S

V510_Pup_c_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

19:04:35

19:45:28

2018.A.00047.S

V510_Pup_b_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

18:10:30

19:00:41

2018.A.00047.S

iras_071_b_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

17:20:48

18:09:27

2018.A.00047.S

iras_071_a_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

16:39:57

17:18:11

2018.A.00047.S

FS_CMa_b_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

15:10:41

15:52:59

2018.A.00047.S

FS_CMa_d_03_7M

Shock-induced chemistry in the CSEs Cerrigoneof late-type stars: a pilot study

NA7-m

3

13:40:07

15:10:34

2018.1.00934.S

IC348_Pe_a_06_7M

EU7-m

6

12:09:21

13:32:04

2018.1.00900.S

CI_Tau_a_03_TM1

EU12-m3

11:38:50

13:32:29

2018.1.01031.S

SNR1E010_a_07_7M

EU7-m

7

09:44:48

11:38:422018.1.01031.S

SNR1E010_a_07_7M

EU7-m

7

08:11:47

09:40:27

2018.A.00046.S

elaiss11_a_06_7M

EU7-m

6

06:59:24

07:59:47

2018.1.00659.L

U_Del_b_06_TM1

The temperature-multiplicity relation Murillo
with ALMA
Measuring the radial profile of theTazzari
maximum grain size in the 4-planet CI
Tau system
Revealing dust processing in theVogt
young supernova remnant
1E\,0102.2-72129 in the SMC
Revealing dust processing in theVogt
young supernova remnant
1E\,0102.2-72129 in the SMC
The host properties and environment Messiasof high-redshift radio galaxies withACAATOMIUM: ALMA Tracing theDecin

EU NA12-m

6

2019-06-28
PI

2019-06-27

06:41:58

08:11:38

2018.1.00101.S

G11.0970_a_03_7M

05:24:11

06:40:20

2018.1.00981.S

Northeas_a_03_7M

05:24:11

06:58:55

2018.1.01782.S

Start (UT)

End (UT)

12:28:21

Origins of Molecules In dUst-forming
oxygen-rich M-type stars
The initial gas flow towards extremely Feng
young high-mass clumps

EA7-m3NA7-m

3

AK_Sco_a_06_TM1

Evolutionarily Young Filamentary
Xiong
Region of NGC 6334
Mapping the Inner Edge of a Kepler- Czekala
Analog Circumbinary Protoplanetary
DiskNA12-m

6

Project CodeSchedBlock

Project Title

ExecutiveArray

Band

13:59:54

2018.1.00525.S

B1-c_a_04_7M

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

NA7-m

4

09:40:14

10:53:14

2018.A.00046.S

elaiss11_a_06_7M

EU7-m

6

09:21:09

11:12:32

2018.1.01135.S

NGC1068_a_03_TM1

OTHER

12-m

3

08:39:52

09:02:072018.1.00659.L

IRC-1052_c_06_TM1

EU NA12-m

608:06:56

09:40:04

2018.A.00046.S

elaiss11_a_06_7M

EU7-m

605:57:00

07:22:39

2018.1.01716.S

HD_16914_a_03_TM1

The host properties and environment Messiasof high-redshift radio galaxies with
ACAResolve SiO and methanol MegaWang
Masers in NGC 1068 by ALMAATOMIUM: ALMA Tracing the Origins Decinof Molecules In dUst-forming oxygenrich M-type stars
The host properties and environment Messiasof high-redshift radio galaxies with
ACA
Thinning the rings: 3 mm observations Maciasof the multigapped disk of HD 169142

NA12-m3

05:48:05

06:55:51

2018.1.00470.S

Proxima_n_06_7M

Millimeter Monitoring of the Closest
Planetary System - Stellar and Dust
Emission from Proxima Centauri

NA7-m

6

04:31:05

05:56:52

2018.1.01716.S

HD_16914_a_03_TM1

Thinning the rings: 3 mm observations Maciasof the multigapped disk of HD 169142

NA12-m3

04:10:41

05:42:50

2018.1.00470.S

Proxima_n_06_7M

Millimeter Monitoring of the Closest
Planetary System - Stellar and Dust
Emission from Proxima Centauri

NA7-m

6

03:04:51

04:30:57

2018.1.01716.S

HD_16914_a_03_TM1

Thinning the rings: 3 mm observations Maciasof the multigapped disk of HD 169142

NA12-m302:38:14

04:10:35

2018.1.00470.S

Proxima_n_06_7M

Millimeter Monitoring of the Closest
Planetary System - Stellar and Dust
Emission from Proxima Centauri

NA7-m

6

01:45:40

02:59:18

2018.1.01679.S

G328.255_a_03_TM1

Direct imaging of an accretion disk
Csengeriarounf the youngest O star precursor

EU12-m301:05:02

02:38:05

2018.1.00470.S

Proxima_n_06_7M

Millimeter Monitoring of the Closest
Planetary System - Stellar and Dust
Emission from Proxima Centauri

MacGregor

NA7-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArray

Band

23:16:09

00:36:34

2018.1.01851.S

G316.75-_d_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

21:37:18

22:57:47

2018.1.01851.S

G316.75-_d_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

21:32:30

22:55:29

2018.1.01218.S

TW_Hya_a_03_TM1Disk substructures in TW Hya:
Optically Thick or Large Grains?

MaciasNA12-m3

2019-06-25
PIMacGregor

MacGregor

MacGregor

2019-06-24