ALMA Observing Activity from 2016-08-22T17:59:00 to 2016-08-29T18:00:00
QA0 pass executions
2016-08-29
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

01:35:38

02:36:14

2015.1.01439.S

IRAS_F16_a_03_TE

Start (UT)

End (UT)

Project Code

18:20:26

18:45:33

18:11:33

PI

Executive

Array

Band

UNVEILING MERGER-INDUCED
Saito
SHOCKS IN MOLECULARHYDROGEN EMITTING GALAXIES(MOHEGs)

EA

12-m

3

SchedBlock

Project Title

Executive

Array

Band

2015.1.01140.S

ngc3628_a_03_TP

EA

Total Power

3

18:44:56

2015.1.00287.S

IRAS_131_c_03_TE

NA12-m3

17:24:08

18:17:58

2015.1.01140.S

ngc3628_a_03_TP

EA

Total Power

3

16:49:23

17:42:17

2015.1.00329.S

PG_1004+_a_03_TE

NA12-m3

14:18:38

15:16:13

2015.1.00094.S

OrionBN-_a_03_TE

NA12-m3

13:24:18

14:30:58

2015.1.01025.S

TUKH122_a_03_7M

EA7-m

3

13:02:13

14:17:34

2015.1.01130.S

SNR_J045_a_03_TE

EA

12-m

3

11:51:23

13:09:48

2015.1.01025.S

TUKH122_a_03_7M

EA7-m

3

11:21:35

12:33:40

2015.1.00543.S

GOODS-S_d_06_TE

Do galaxies lose molecular gas more Tsaithan expected?
The Almost Forgotten Local UltraSliwa
Luminous Infrared Galaxy: IRAS
13120-5453
Do galaxies lose molecular gas more Tsaithan expected?
Do Optically-Luminous PG QSOs in Evansthe Local Universe Reside in
Molecular Gas-Rich Hosts?
Surveying the Seeds of Star
DunhamFormation: Starless Cores in Orion B
North
Investigating the dyncamics of a
Ohashithermal starless core in the Orion Acloud.
Molecular gas associated with theFujii
LMC Supernova remnants
Investigating the dyncamics of a
Ohashithermal starless core in the Orion Acloud.
Towards a census of star-formation Elbaz
since z~6 with ALMA-1.1mm

EU12-m

610:46:51

11:20:56

2015.1.00591.S

NGC_1052_a_03_TEEU12-m

3

10:37:45

11:50:49

2015.1.00094.S

OrionBN-_a_03_7M

NA7-m

3

10:10:43

10:46:10

2015.1.01207.S

DL_Tau_a_06_TE

Molecular Gas Structures in Elliptical Vila Vilaro
Galaxies
Surveying the Seeds of Star
DunhamFormation: Starless Cores in Orion BNorthDiagnozing Protoplanet Formation in Nomura
Protoplanetary Disks

EA12-m609:35:45

10:00:25

2015.1.01207.SCY_Tau_a_06_TE

Diagnozing Protoplanet Formation in Nomura
Protoplanetary Disks

EA12-m609:18:43

10:36:54

2015.1.00956.S

NGC_1672_a_06_7M

NA7-m

608:22:04

09:34:04

2015.1.00543.S

GOODS-S_d_06_TE

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Towards a census of star-formation Elbaz
since z~6 with ALMA-1.1mm

EU12-m607:56:49

09:15:12

2015.1.00956.S

NGC_1672_a_06_7M

NA7-m

606:54:16

08:08:27

2015.1.00543.S

GOODS-S_c_06_TE

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Towards a census of star-formation Elbaz
since z~6 with ALMA-1.1mm

EU12-m605:13:17

05:46:57

2015.1.00199.S

WISE_J00_a_06_TE

Proving the AGN feedback in theextremely IR-bright Dust Obscured
Galaxies

Toba

EA

12-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

ExecutiveArray

Band

10:55:37

12:12:39

2015.1.01339.S

HG2894_a_06_7M

Identifying the transition phase of the Olmiclump mass function toward the IMF

EU7-m

609:16:12

10:34:34

2015.1.00956.S

NGC_1672_a_06_7M

NA7-m

608:09:01

09:26:34

2015.1.00016.S

B0218+35_a_07_TE

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
A search for extragalactic argonium, Müller
ArH+, a probe of the very atomic
diffuse interstellar medium

EU12-m7

07:45:06

08:59:35

2015.1.00925.S

NGC_1566_b_06_7M

CL7-m

6

04:04:16

04:34:17

2015.1.01083.S

RXJ1852._a_07_TE

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Planetary Formation in the late-phase Morinoof classical T Tauri stars located atCrA west

EA12-m7

2016-08-27
PI

2016-08-26

03:49:19

04:29:38

2015.1.00601.S

mosaic2_a_03_TP

G351.77--0.51: ridge formation caught Leurini
in the act
Understanding the Disk Wind from HD Klaassen
163296The Extreme Kinematics of Ionized Royster
Gas in the Central Half Parsec of theGalaxy
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
Survey of CO Snow Lines in Solar
Qi
Nebula Analogues
Understanding the Disk Wind from HD Klaassen
163296
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
Understanding the Disk Wind from HD Klaassen
163296EU

Total Power

303:15:32

04:40:02

2015.1.00023.S

HD_16329_a_06_7M

EU7-m

603:04:15

04:01:34

2015.1.01342.S

sgra_a_07_TE

NA12-m7

02:50:35

03:30:58

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

302:05:40

02:48:36

2015.1.00601.S

mosaic1_a_03_TP

EU

Total Power

301:50:38

02:58:33

2015.1.00678.S

AS_209_a_07_TE

NA12-m

701:44:59

03:07:02

2015.1.00023.S

HD_16329_a_06_7M

EU7-m

601:24:1202:04:35

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

300:40:13

01:23:14

2015.1.00601.S

mosaic1_a_03_TP

EU

Total Power

300:26:29

01:42:35

2015.1.00023.S

HD_16329_a_06_7M

EU7-m6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:58:05

00:38:37

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

23:56:56

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

3

22:13:03

23:26:04

2015.1.01406.S

A1689-zD_a_06_TE

EU

12-m

6

20:54:23

21:39:14

2015.1.00956.S

NGC_4254_b_06_TPNA

Total Power

620:34:46

21:43:44

2015.1.01406.S

A1689-zD_a_06_TE

EU12-m6

18:55:01

20:04:22

2015.1.01406.S

A1689-zD_a_06_TE

EU12-m6

18:31:42

20:24:01

2015.1.00656.S

Western__a_08_7M

NA7-m

8

17:29:27

18:38:14

2015.1.01406.S

A1689-zD_a_06_TE

EU12-m6

16:15:07

17:18:25

2015.1.01320.S

G09.97_a_04_TE

EU12-m4

15:12:58

16:33:49

2015.1.00357.S

G286_5_a_06_7M

NA7-m

6

14:25:27

15:30:33

2015.1.00612.S

W0831+01_a_08_TE

G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
Anomalously faint [CII]from a merger Watson
at z=7.60
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Anomalously faint [CII]from a merger Watson
at z=7.60
Anomalously faint [CII]from a merger Watson
at z=7.60
Testing Basic PDR Physics inHartigan
Carina's Western Wall
Anomalously faint [CII]from a merger Watson
at z=7.60
Dissecting starbursts at z=3.6 through Omont
multi-line H2O imaging
Kinematics of Massive Star Cluster in TanFormation
Observations of the [Cii]Emission Line Assefin Hot, Dust-Obscured Galaxies

23:10:55

CL12-m8

13:04:47

14:22:09

2015.1.01339.S

HG2894_a_06_7M

Identifying the transition phase of the Olmiclump mass function toward the IMF

EU7-m

6

12:32:07

13:46:25

2013.1.00338.S

IRAS_085_a_07_TE

EU

12-m

7

11:35:20

12:27:56

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

11:19:15

12:35:31

2015.1.01008.S

HOPS-088_a_06_7M

NA7-m

6

10:53:01

12:14:37

2015.1.01093.S

Perseus__a_06_TEEA

12-m610:39:41

11:32:08

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

310:14:09

11:17:192015.1.00340.S

MC27_a_06_7M

EA7-m

609:47:45

10:38:072015.1.00925.S

NGC_1300_b_06_TP

CL

Total Power608:56:37

10:11:30

2015.1.00340.S

MC27_a_06_7M

EA7-m

608:52:41

10:41:55

2015.A.00018.S

SXDF-NB1_a_08_TE

EA

12-m

8

06:11:23

07:51:17

2015.1.00997.S

SDSS_J01_a_07_7M

EU7-m

705:42:20

06:02:33

2015.1.01147.S

I_ZW_a_1_03_TE

Rotating and expanding gas inBujarrabal
protoplanetary nebulae
Investigating the dyncamics of aOhashi
thermal starless core in the Orion Acloud.
Mapping Infall in Filamentary
MegeathEnvironments: A Study of three Orion
Class 0 Protostars
Unviased Chemical Survey ofSakai
Protostellar Sources in Perseus
Investigating the dyncamics of aOhashi
thermal starless core in the Orion Acloud.
Investigating the dynamical interaction Tokuda
at the formation of a multiple starsystemPromoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Investigating the dynamical interaction Tokuda
at the formation of a multiple starsystem[OIII]line kinematics of a Lya emitter Inoueat z=7.2
Extreme quasar feedback in the early Maiolino
UniverseCO Imaging of Ultraluminous
Kohno

EA12-m3

2016-08-25
PIInfrared QSO Hosts
04:01:35

04:40:36

2015.1.01535.S

K3-50A_a_07_TE

Revealing a new population of UC-HII Baez Rubio
regions with maser RRLs
Identification of the Centrifugal Barrier Oyaof the Infalling Rotating Envelope inthe Hot Corino Source IRAS 162932422

EU12-m702:38:41

03:40:24

2015.1.01060.S

IRAS_162_a_06_TEEA12-m601:31:14

02:53:22

2015.1.00023.S

HD_16329_a_06_7M

Understanding the Disk Wind from HD Klaassen
163296EU7-m

6Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

11:21:49

12:30:56

2015.1.01522.S

J050644-_a_03_TE

EU

12-m

3

10:15:14

10:59:11

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power3

09:55:52

11:17:34

2015.1.01522.S

J050644-_a_03_TE

EU

12-m

3

08:45:13

09:55:27

2015.1.01129.S

SXDS1_13_a_03_TE

EA12-m306:44:48

08:04:33

2015.1.01129.S

SXDS1_13_a_03_TE

EA12-m305:00:3606:14:07

2015.1.01129.S

SXDS1_13_a_03_TE

EA12-m304:23:05

04:59:54

2015.1.00587.S

CIG1044_a_03_TE

EU

12-m

303:15:2503:49:39

2015.1.01147.S

IRAS_F23_a_03_TE

EA12-m303:07:47

03:43:40

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

302:46:45

03:12:52

2015.1.01147.S

IRAS_F22_a_03_TE

EA

12-m

302:25:44

03:07:17

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

301:36:1502:07:45

2015.1.01439.S

ngc6240_b_04_TE

Polarimetric observations of aGalluzzi
complete sample of radio sources
Investigating the dyncamics of aOhashi
thermal starless core in the Orion Acloud.
Polarimetric observations of aGalluzzi
complete sample of radio sources
Molecular clumps in a star-forming
Ohtagalaxy at z~1.4
Molecular clumps in a star-forming
Ohtagalaxy at z~1.4
Molecular clumps in a star-forming
Ohtagalaxy at z~1.4
Why do isolated galaxies host red
Verdespseudobulges?
Montenegro
CO Imaging of Ultraluminous Infrared Kohno
QSO Hosts
G351.77--0.51: ridge formation caught Leurini
in the act
CO Imaging of Ultraluminous Infrared Kohno
QSO Hosts
G351.77--0.51: ridge formation caught Leurini
in the act
UNVEILING MERGER-INDUCED
Saito
SHOCKS IN MOLECULARHYDROGEN EMITTING GALAXIES(MOHEGs)

EA

12-m

4

00:25:29

01:09:10

2015.1.01439.S

IRAS_F16_b_03_TE

UNVEILING MERGER-INDUCED
Saito
SHOCKS IN MOLECULARHYDROGEN EMITTING GALAXIES(MOHEGs)

EA

12-m

3Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:54:13

00:32:56

2015.1.00601.S

mosaic1_a_03_TPEU

Total Power

3

23:49:19

00:21:25

2015.1.01439.S

ngc6240_b_03_TE

G351.77--0.51: ridge formation caught Leurini
in the act
UNVEILING MERGER-INDUCED
Saito
SHOCKS IN MOLECULARHYDROGEN EMITTING GALAXIES(MOHEGs)

EA

12-m

3

23:17:41

23:53:54

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

22:23:15

23:04:28

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

3

21:46:15

22:22:30

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

21:38:55

22:50:43

2015.1.00627.S

UGC9799_a_06_TE

EU12-m621:05:14

21:36:40

2015.1.00167.S

Arp220_d_03_TE

EU

12-m

3

20:57:02

21:38:33

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

3

19:18:07

19:51:51

2015.1.01140.S

ngc3628_a_03_TP

EA

Total Power

3

18:55:17

19:52:18

2015.1.01019.S

Filament_a_03_7M

EU7-m

3

18:22:10

19:11:25

2015.1.01140.S

ngc3628_a_03_TP

EA

Total Power

3

17:35:03

18:39:39

2015.1.01019.S

Filament_a_03_7M

EU7-m

3

17:29:52

18:19:192015.1.01140.S

ngc3628_a_03_TP

EA

Total Power

3

16:23:42

17:12:51

2015.1.01140.S

ngc3628_a_03_TP

G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
Driving molecular gas flows with radio Russell
bubbles in A2052's brightest cluster
galaxySpatially resolved wideband
Martinspectroscopy in ULIRG obscured
nuclei II
G351.77--0.51: ridge formation caught Leurini
in the act
Do galaxies lose molecular gas more Tsaithan expected?
Star formation efficiency in the outer Salome
filament of Centaurus A
Do galaxies lose molecular gas more Tsaithan expected?
Star formation efficiency in the outer Salome
filament of Centaurus A
Do galaxies lose molecular gas more Tsaithan expected?
Do galaxies lose molecular gas
Tsai

EA

Total Power3

2016-08-24
PI

2016-08-23
PImore than expected?
15:17:45

16:07:13

2015.1.01140.S

ngc3628_a_03_TP

Do galaxies lose molecular gas more Tsaithan expected?
Why do isolated galaxies host red
Verdespseudobulges?
Montenegro
Investigating the dyncamics of aOhashi
thermal starless core in the Orion Acloud.
Investigating the dyncamics of a
Ohashithermal starless core in the Orion Acloud.
Investigating the dyncamics of aOhashi
thermal starless core in the Orion Acloud.
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Investigating the dyncamics of a
Ohashithermal starless core in the Orion A
cloud.
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act

EA

Total Power3

14:01:30

14:34:24

2015.1.00587.S

CIG222_a_03_TE

EU12-m3

13:52:29

14:39:48

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

12:58:18

13:45:34

2015.1.01025.S

TUKH122_a_03_TPEA

Total Power

312:07:51

12:55:56

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power3

11:00:52

11:46:33

2015.1.00925.S

NGC_1300_b_06_TP

CL

Total Power

610:12:30

11:00:06

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power3

09:24:39

10:11:25

2015.1.00925.S

NGC_1300_b_06_TP

CL

Total Power

608:37:1209:23:00

2015.1.00925.S

NGC_1300_b_06_TP

CL

Total Power607:52:43

08:36:56

2015.1.00925.S

NGC_1300_a_06_TP

CL

Total Power603:12:58

03:51:41

2015.1.00601.S

mosaic1_a_03_TP

EU

Total Power

302:31:21

03:12:11

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

301:54:30

02:30:35

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

300:51:26

01:27:25

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

300:07:01

00:48:10

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:30:31

00:06:38

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

323:29:40

2015.1.00601.S

mosaic4_a_03_TP

EU

Total Power

322:42:21

2015.1.00601.S

mosaic2_a_03_TP

G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act

22:48:31
22:05:39

EUTotal Power3

2016-08-22
PI