ALMA Observing Activity from 2016-05-02T17:59:00 to 2016-05-09T18:00:00
QA0 pass executions
2016-05-08
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

18:06:12

19:14:38

2015.1.01395.S

NGC_625_a_03_TE

15:23:07

16:32:02

2015.1.01395.S

NGC_625_a_03_TE

14:11:08

15:30:24

2015.1.00059.S

TX_Psc_a_06_7M

14:02:19

15:15:08

2015.1.00782.S

NGC_7793_a_06_TE

12:33:28

13:38:47

2015.1.00463.S

HFF1C-Y5_a_06_TE

12:08:26

13:27:56

2015.1.00059.S

TX_Psc_a_06_7M

11:06:10

12:15:46

2015.1.00307.S

HD_20712_a_06_TE

10:40:16

12:07:38

2015.1.01273.S

W43-MM1_a_06_7M

10:24:24

11:11:55

2015.1.00925.S

IC_5332_a_06_TP

09:42:40

10:24:53

2015.1.00075.S

PKS1830-_h_07_TE

09:42:10

10:19:38

2015.1.00956.S

NGC6744_a_06_TP

09:04:21

10:23:20

2015.1.00850.S

6334_-_M_a_06_7M

08:55:22

09:41:14

2015.1.00749.S

08:34:22

09:38:08

08:13:11

PI

Executive

Array

Band

Resolving Molecular Clouds in a Low Imara
Metallicity Galaxy
Resolving Molecular Clouds in a Low Imara
Metallicity Galaxy
The mass loss history of the "fresh" Brunnercarbon star TX Piscium - A showcase
for stellar evolution
ALMA-LEGUS: The Impact of Spiral Johnson
Arm Structure on Molecular Cloud
Properties and Star Cluster Formation

NA

12-m

3

NA

12-m

3

EU

7-m

6

NA

12-m

6

Exploring the Earliest Epoch of the
Ouchi
Massive Dust Production
The mass loss history of the "fresh" Brunnercarbon star TX Piscium - A showcase
for stellar evolution
Debris Disk Structure around Nearby Wilner
Sun-like Stars
Investigating the origin of the IMF and Motte
constraining SFR models in the W43MM1 mini-starbust ridge
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Monitoring PKS1830-211: the submm Muller
activity of the blazar and the variabilityof the foreground absorption lines

EA

12-m

6

EU

7-m

6

NA

12-m

6

EU

7-m

6

CL

Total Power

6

EU

12-m

7

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Digging within the cold Herschel
Louvetsources of the NGC 6334 complex, todefine the initial phase of high-massstar formation

NA

Total Power

6

CL

7-m

6

G028.314_a_06_TP

Properties of the most distant starforming GMC in the Milky Way

Mottram

EU

Total Power6

2015.1.00667.S

AG22.36+_b_06_TE

Mass assembly in the pre-stellar
phase of high-mass star formation

Wang

EU

12-m

6

08:54:31

2015.1.01363.S

MC23_a_03_TP

Total Power

3

07:41:18

09:03:50

2015.1.01273.S

W43-MM1_a_06_7M

7-m

6

07:34:35

08:33:26

2015.1.00994.S

PN_Th3-1_a_06_TE

12-m

6

07:22:08

08:12:43

2015.1.00850.S

6334_-_M_d_06_TP

Large scale infall or local collapse
CsengeriEU
forms massive clusters?
Investigating the origin of the IMF and MotteEU
constraining SFR models in the W43MM1 mini-starbust ridge
Weighing the Galactic Bulge
Guzman-RamirezEU
Planetary Nebulae
Digging within the cold Herschel
LouvetCLsources of the NGC 6334 complex, todefine the initial phase of high-massstar formation

Total Power

6

06:33:16

07:33:49

2015.1.00667.S

AG22.36+_b_06_TE

Mass assembly in the pre-stellar
phase of high-mass star formation

Wang

EU

12-m

6

06:21:10

07:40:52

2015.1.00850.S

6334_-_M_a_06_7M

Digging within the cold Herschel
Louvetsources of the NGC 6334 complex, todefine the initial phase of high-massstar formation

CL

7-m

6

05:36:33

06:26:32

2015.1.01539.S

G341.03_a_06_TP

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

Total Power

605:33:01

06:32:51

2015.1.00994.S

PN_Th3-1_a_06_TE

12-m

6

04:45:14

05:35:43

2015.1.01539.S

G337_a_06_TP

Weighing the Galactic Bulge
Guzman-RamirezEU
Planetary Nebulae
A survey of prestellar, high-mass
Sanhueza
EA
cluster-forming clumps: constraining
models of high-mass star formation

Total Power

6

04:41:44

06:20:40

2015.1.01539.S

G14.49_a_06_7M

A survey of prestellar, high-masscluster-forming clumps:

7-m

6SanhuezaEA04:39:35

05:32:34

2015.1.01243.S

HD_13148_a_06_TE

03:30:28

04:39:10

2015.1.01355.S

Cl_J1449_a_04_TE

03:16:59

04:31:48

2015.1.00306.S

Lupus_3__a_03_TP

03:15:46

04:40:58

2015.1.01014.S

SDC338.3_a_03_7M

02:28:01

03:16:15

2015.1.00908.S

Thakeray_a_03_TP

02:18:40

03:30:04

2015.1.01114.S

NGC_3627_c_03_TE

02:10:10

03:03:51

2015.1.01014.S

SDC338.3_a_03_7M

01:38:59

02:27:36

2015.1.00908.S

Thakeray_a_03_TP

00:55:15

02:06:22

2015.1.01114.S

NGC_3627_c_03_TE

00:49:53

01:38:15

2015.1.00908.S

Start (UT)

End (UT)

18:09:54

constraining models of high-mass starformation
Molecular gas in debris disks around Cure
young A-type stars
Cold gas in the most distant cluster Strazzullo
galaxies: completing the ALMA
picture of CL J1449+0856 at z=2

CL

12-m

6

EU

12-m

4

The earliest stages of molecular
Plunkett
outflow activity from the young
protostar Lupus 3 MMS
What can hubs tell us on massive star Peretto
formation?
Thackeray's Globules
ReipurthNA

Total Power

3

EU

7-m

3

NA

Total Power

3

Chemical Variation in a Barred Spiral Watanabe
Galaxy NGC 3627
What can hubs tell us on massive star Peretto
formation?
Thackeray's Globules
Reipurth

EA

12-m

3

EU

7-m

3

NA

Total Power

3

EA

12-m

3

Thakeray_a_03_TP

Chemical Variation in a Barred Spiral Watanabe
Galaxy NGC 3627
Thackeray's Globules
ReipurthNA

Total Power

3

Project Code

SchedBlock

Project Title

Executive

Array

Band

19:05:30

2015.1.00094.S

OrionBN-_a_03_7M

NA

7-m

3

18:02:26

18:43:33

2015.1.00196.S

LMC2N113_a_03_TP

Surveying the Seeds of Star
DunhamFormation: Starless Cores in Orion B
North
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

17:11:45

17:52:52

2015.1.00196.S

LMC2N113_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

17:07:52

18:22:22

2015.1.01395.S

NGC_625_a_03_TE

NA

12-m

3

16:41:38

18:07:08

2015.1.00894.S

SPT-CL_J_a_03_7M

Resolving Molecular Clouds in a Low Imara
Metallicity GalaxyFirst spatially-resolved imaging of a Kitayama
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effect

EA

7-m

3

16:30:01

17:11:04

2015.1.00196.S

LMC2N113_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

15:45:18

16:25:36

2015.1.00196.S

SMC0N69_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

15:43:15

16:51:38

2015.1.01395.S

NGC_625_a_03_TE

NA

12-m

3

15:07:44

16:27:56

2015.1.00894.S

SPT-CL_J_a_03_7M

Resolving Molecular Clouds in a Low Imara
Metallicity GalaxyFirst spatially-resolved imaging of a Kitayama
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effect

EA

7-m

3

15:04:19

15:44:38

2015.1.00196.S

SMC0N69_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

14:35:26

15:27:15

2015.1.00586.S

haro11_a_03_TE

EU

12-m

3

14:08:19

14:48:31

2015.1.00196.S

SMC0N69_a_03_TP

Solving the mystery of star formation Cormierwithout cold gas
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

13:40:00

14:08:10

2015.1.00587.S

CIG55_a_03_TC

EU

12-m

3

13:27:20

14:07:39

2015.1.00196.S

SMC0N69_a_03_TP

Why do isolated galaxies host red
Verdespseudobulges?
Montenegro
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

13:25:56

14:46:29

2015.1.00894.S

SPT-CL_J_a_03_7M

First spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich

EA

7-m

3

2016-05-07
PI

Kitayamaeffect
12:51:34

13:24:36

2015.1.00196.S

SMC1N42_b_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

12:18:18

12:51:17

2015.1.00196.S

SMC1N42_b_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

12:17:22

13:39:39

2015.1.00952.S

B6_a_06_TE

What Powers the Lyman alpha Blobs?Ao

EA

12-m

6

11:48:23

13:09:00

2015.1.00894.S

SPT-CL_J_a_03_7M

First spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effect

EA

7-m

3

11:44:20

12:17:24

2015.1.00196.S

SMC1N42_b_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

10:58:20

12:06:31

2015.1.01543.T

spt2349_a_04_TE

Lacaille

NA

12-m

4

10:44:00

11:48:04

2015.1.00894.S

SPT-CL_J_a_03_7M

Unlensed HyLIRG systems from theSouth Pole Telescope 2500deg^2
surveyFirst spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effectKitayama

EA

7-m

3

09:53:57

10:34:45

2015.1.01363.S

MC23_a_03_TP

CsengeriEU

Total Power3

09:14:54

10:43:09

2015.1.00897.S

MRC2048-_a_03_7M

EmontsEU

7-m

3

09:13:51

10:31:34

2015.1.00230.S

NGC6334-_b_03_TE

Liu

EA

12-m

3

09:12:03

09:53:16

2015.1.01363.S

MC23_a_03_TP

Large scale infall or local collapse
forms massive clusters?
Cold gas halos at z~2: evolution ofmassive galaxies within a molecular
IGM
Mass accretion flows in high-massstar formation
Large scale infall or local collapse
forms massive clusters?

CsengeriEU

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

15:46:06

16:36:20

2015.1.00894.S

SPT-CL_J_a_03_7M

First spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effectKitayama

EA

7-m

3

15:40:26

16:41:38

2015.1.01379.S

GMASS_09_a_06_TE

Key laboratory for AGN feedback and Cassata
spheroid formation: a moderately
luminous AGN at z ~ 2

CL

12-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

11:05:30

12:14:46

2015.1.00307.S

HD_20712_a_06_TE

NA

12-m

6

10:53:41

11:34:072015.1.01363.S

MC23_a_03_TP

EU

Total Power

3

10:52:26

11:58:51

2015.1.01363.S

MC23_a_03_7M

EU

7-m

3

09:29:39

10:40:33

2015.1.01308.S

Serpens__a_06_TE

NA

12-m

6

09:17:00

10:26:59

2015.1.00223.S

serpens__a_06_7M

EA

7-m

6

09:07:37

09:48:13

2015.1.01363.S

MC23_a_03_TP

EU

Total Power3

08:26:31

09:07:14

2015.1.01363.S

MC23_a_03_TP

EU

Total Power3

08:18:07

09:28:58

2015.1.01308.S

Serpens__a_06_TE

NA

12-m

6

07:54:04

09:16:35

2015.1.01273.S

W43-MM1_a_06_7M

EU

7-m

6

07:11:31

08:26:072015.1.00306.S

Lupus_3__a_03_TP

NA

Total Power3

07:10:20

08:17:49

2015.1.01308.S

Serpens__a_06_TE

NA

12-m

6

06:11:12

07:09:54

2015.1.01355.S

Cl_J1449_a_04_TE

Debris Disk Structure around Nearby Wilner
Sun-like Stars
Large scale infall or local collapse
Csengeriforms massive clusters?
Large scale infall or local collapse
Csengeriforms massive clusters?
From Dark to Light: Star Clusters in Mundy
Formation
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
South
Large scale infall or local collapse
Csengeriforms massive clusters?
Large scale infall or local collapse
Csengeriforms massive clusters?
From Dark to Light: Star Clusters in Mundy
Formation
Investigating the origin of the IMF and Motte
constraining SFR models in the W43MM1 mini-starbust ridge
The earliest stages of molecular
Plunkett
outflow activity from the young
protostar Lupus 3 MMS
From Dark to Light: Star Clusters in Mundy
Formation
Cold gas in the most distant
Strazzullo

EU

12-m

4

Kitayama

2016-05-05

2016-05-04
PI06:10:37

07:24:23

2015.1.01014.S

SDC338.3_a_03_7M

05:54:10

07:11:12

2015.1.00306.S

Lupus_3__a_03_TP

05:35:52

06:10:43

2015.1.00939.S

GRB06081_a_04_TE

05:03:16

05:30:25

2015.1.00320.S

2MASXJ13_a_03_TE

04:44:18

06:09:53

2015.1.01014.S

SDC338.3_a_03_7M

04:37:16

05:53:20

2015.1.00306.S

Lupus_3__a_03_TP

03:52:39

05:00:10

2015.1.01161.S

VV_219_a_03_TE

03:47:39

04:36:31

2015.1.00908.S

Thakeray_a_03_TP

01:17:16

01:47:072015.1.00320.S

2MASXJ13_b_03_TE

00:11:59

00:56:33

2015.1.00477.S

Start (UT)

End (UT)

23:43:55

cluster galaxies: completing the
ALMA picture of CL J1449+0856 at
z=2
What can hubs tell us on massive star Peretto
formation?
The earliest stages of molecular
Plunkett
outflow activity from the young
protostar Lupus 3 MMS
CO Survey toward the Host Galaxies Hatsukade
of Gamma-ray Bursts
Star formation suppression in recent van de Voortminor mergers
What can hubs tell us on massive star Peretto
formation?
The earliest stages of molecular
Plunkett
outflow activity from the young
protostar Lupus 3 MMS
How Is Molecular Gas Affected by the Kaneko
Collision of Galaxies at the Collision
Front
Thackeray's Globules
Reipurth

EU

7-m

3

NA

Total Power

3

EA

12-m

4

EA

12-m

3

EU

7-m

3

NA

Total Power

3

EA

12-m

3

NA

Total Power

3

EA

12-m

3

GAMA2729_a_06_TE

Star formation suppression in recent van de Voortminor mergers
Mapping the extent and durability of Sansom
dust in early-type galaxies detectedwith Herschel

EU

12-m

6

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

00:11:32

2015.1.00477.S

GAMA1771_a_06_TE

Sansom

EU

12-m

6

23:29:17

00:17:23

2015.1.00908.S

Thakeray_a_03_TP

Mapping the extent and durability of
dust in early-type galaxies detectedwith HerschelThackeray's Globules

ReipurthNA

Total Power

3

22:53:52

23:41:30

2015.1.00086.S

ngc3393_a_06_TE

Understanding Nuclear Streaming:
stellar, atomic, and molecular gas
kinematics in the inner 100pc:
Continuation

Nagar

CL

12-m

6

22:40:30

23:28:55

2015.1.00908.S

Thakeray_a_03_TP

Thackeray's Globules

ReipurthNA

Total Power

3

22:27:14

00:00:25

2015.1.01339.S

HG2907_a_06_7M

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

EU

7-m

6

22:04:07

22:53:30

2015.1.00477.S

GAMA6223_a_06_TE

EU

12-m

6

21:53:27

22:38:52

2015.1.00925.S

NGC_2835_a_06_TP

CL

Total Power6

21:05:06

22:26:47

2015.1.01339.S

HG2752_a_06_7M

Mapping the extent and durability of Sansom
dust in early-type galaxies detectedwith HerschelPromoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Identifying the transition phase of the Olmiclump mass function toward the IMF

EU

7-m

6

20:58:45

21:50:24

2015.1.01572.S

pks0718-_a_06_TE

AGN Feedback and its Role in Galaxy Prandoni
Evolution: gas and stellar kinematics
of radio-loud early-type galaxies

EU

12-m

6

20:48:48

21:39:31

2015.1.01008.S

HOPS-178_a_06_TP

NA

Total Power

6

19:56:50

20:48:00

2015.1.01008.S

HOPS-247_a_06_TP

NA

Total Power

6

19:55:03

20:51:01

2015.1.00094.S

OrionBN-_a_03_7M

NA

7-m

3

19:43:11

20:35:58

2015.1.00989.S

ngc_1370_a_03_TE

NA

12-m

3

19:14:28

19:55:14

2015.1.00196.S

LMC1N127_a_03_TP

Mapping Infall in Filamentary
MegeathEnvironments: A Study of three Orion
Class 0 Protostars
Mapping Infall in Filamentary
MegeathEnvironments: A Study of three Orion
Class 0 Protostars
Surveying the Seeds of Star
DunhamFormation: Starless Cores in Orion B
North
Does Cold Gas Fuel Almost All
Hodges-Kluck
AGNs?
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

18:39:37

19:54:192015.1.00196.S

LMC0NT19_a_03_7M

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

7-m

3

18:32:38

19:13:42

2015.1.00196.S

LMC1N127_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

18:02:52

19:22:23

2015.1.00870.S

12383_a_06_TE

Evolution of the interstellar gas

NA

12-m

6

2016-05-03

Wiklindfraction over cosmic time
17:37:51

18:19:02

2015.1.00196.S

LMC2N113_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

16:59:47

18:01:49

2015.1.01379.S

GMASS_09_a_06_TE

Key laboratory for AGN feedback and Cassata
spheroid formation: a moderately
luminous AGN at z ~ 2

CL

12-m

6

16:56:54

18:03:00

2015.1.00530.S

4C04.11_a_03_7M

EU

7-m

3

16:54:04

17:35:072015.1.00196.S

LMC2N113_a_03_TP

An ALMA-MUSE Survey of Extended De Breuck
Radio Galaxy Haloes
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

16:12:27

16:53:44

2015.1.00196.S

LMC2N113_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

16:08:25

16:41:24

2015.1.00989.S

ngc_1052_a_03_TE

Hodges-Kluck

NA

12-m

3

15:33:39

16:54:55

2015.1.00258.S

NGC300_b_03_7M

Does Cold Gas Fuel Almost All
AGNs?
The failure of galactic star formation
relations on sub-galactic scales: A
direct probe of the physics of starformation

Schruba

EU

7-m

3

15:18:09

15:58:16

2015.1.00196.S

SMC1N42_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

14:49:50

16:07:59

2015.1.01395.S

NGC_625_a_03_TE

NA

12-m

3

14:37:23

15:17:44

2015.1.00196.S

SMC0N69_a_03_TP

Resolving Molecular Clouds in a Low Imara
Metallicity Galaxy
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

14:11:03

15:33:14

2015.1.01187.S

El_Gordo_a_03_7M

EU

7-m

3

13:56:50

14:36:56

2015.1.00196.S

SMC1N42_a_03_TP

ALMA observation of a galaxy cluster Basumerger shock at half the age of theuniverse
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

13:41:00

14:18:20

2015.1.00587.S

CIG64_a_03_TC

EU

12-m

3

13:15:56

13:56:05

2015.1.00196.S

SMC1N42_a_03_TP

Why do isolated galaxies host red
Verdespseudobulges?
Montenegro
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

12:49:24

14:10:40

2015.1.00258.S

NGC300_b_03_7M

The failure of galactic star formation
relations on sub-galactic scales: A
direct probe of the physics of starformation

EU

7-m

3

12:32:53

13:12:55

2015.1.00196.S

SMC1N42_a_03_TP

Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

12:25:45

13:06:13

2015.1.00587.S

CIG1044_a_03_TC

EU

12-m

3

11:49:34

12:29:55

2015.1.00196.S

SMC1N42_a_03_TP

Why do isolated galaxies host red
Verdespseudobulges?
Montenegro
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

11:28:29

12:49:02

2015.1.00894.S

SPT-CL_J_a_03_7M

First spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effectKitayama

EA

7-m

3

11:04:02

11:56:24

2015.1.01572.S

ngc7075_a_06_TE

AGN Feedback and its Role in Galaxy Prandoni
Evolution: gas and stellar kinematics
of radio-loud early-type galaxies

EU

12-m

6

10:57:12

11:37:39

2015.1.01363.S

MC23_a_03_TP

EU

Total Power

3

10:16:00

10:56:35

2015.1.01363.S

MC23_a_03_TP

EU

Total Power3

09:47:20

11:09:20

2015.1.01273.S

W43-MM1_a_06_7M

EU

7-m

6

09:32:44

10:13:21

2015.1.01363.S

MC23_a_03_TP

Large scale infall or local collapse
Csengeriforms massive clusters?
Large scale infall or local collapse
Csengeriforms massive clusters?
Investigating the origin of the IMF and Motte
constraining SFR models in the W43MM1 mini-starbust ridge
Large scale infall or local collapse
CsengeriEU

Total Power

3

Schrubaforms massive clusters?
09:19:09

10:30:10

2015.1.01308.S

Serpens__a_06_TE

08:45:45

09:31:58

2015.1.00749.S

G028.314_a_06_TP

08:24:10

09:46:34

2015.1.01273.S

W43-MM1_a_06_7M

07:54:55

08:45:23

2015.1.01539.S

G340.23_a_06_TP

07:12:11

08:23:27

2015.1.01539.S

07:10:41

09:18:20

07:03:25

From Dark to Light: Star Clusters inFormation
Properties of the most distant starforming GMC in the Milky Way

Mundy

NA

12-m

6

Mottram

EU

Total Power

6

Investigating the origin of the IMF and Motte
constraining SFR models in the W43MM1 mini-starbust ridge
A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EU

7-m

6

EA

Total Power

6

G340.17_a_06_7M

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

7-m

6

2013.1.00764.S

Sgr_A_st_e_06_TE

Probing Accretion Flow Dynamics of Bower
Sgr A* on Scales from 1 to 1000
Schwarzschild Radii with ALMA
Polarimetry

NA

12-m

6

07:54:15

2015.1.01539.S

G340.23_a_06_TP

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

Total Power6

06:12:01

07:02:41

2015.1.01539.S

G340.23_a_06_TP

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

Total Power

605:48:56

07:11:31

2015.1.01539.S

G340.17_a_06_7M

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

7-m

6

05:32:26

07:10:20

2013.1.00764.S

Sgr_A_st_e_06_TE

Probing Accretion Flow Dynamics of Bower
Sgr A* on Scales from 1 to 1000
Schwarzschild Radii with ALMA
Polarimetry

NA

12-m

6

05:21:07

06:11:192015.1.01539.S

G341.03_a_06_TP

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

Total Power6

04:16:49

05:07:12

2015.1.01539.S

G341.03_a_06_TP

A survey of prestellar, high-mass
Sanhuezacluster-forming clumps: constraining
models of high-mass star formation

EA

Total Power604:13:53

05:35:20

2015.1.00925.S

NGC_5068_a_06_7M

CL

7-m

6

04:05:02

05:20:56

2015.1.00644.S

IC_4374_a_06_TE

EA

12-m

6

03:20:09

04:03:38

2015.1.00956.S

NGC_4535_a_06_TP

NA

Total Power6

03:08:09

04:13:30

2015.1.00925.S

NGC_5068_a_06_7M

CL

7-m

6

02:45:53

03:34:42

2015.1.00860.S

n4636_a_06_TE

NA

12-m

6

02:31:48

03:19:49

2015.1.00908.S

Thakeray_a_03_TP

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Nuclear outflow and inflow in the
Fujitastrongest X-ray cool core of nearby
galaxy groups
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
CO and AGN feedback in massive
Temigalaxies
Thackeray's Globules
ReipurthNA

Total Power3

01:50:59

03:05:59

2015.1.00956.S

NGC4303_a_06_7M

NA

7-m

6

01:47:05

02:45:11

2015.1.01489.S

BRI_1202_a_06_TE

EU

12-m

6

01:42:38

02:31:072015.1.00908.S

Thakeray_a_03_TP

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Outflows and Dissipation in a distant Lehnert
QSO and SMG pair: Where does theenergy go?
Thackeray's Globules
ReipurthNA

Total Power

300:48:41

01:46:26

2015.1.01489.S

BRI_1202_a_06_TE

EU

12-m

6

00:29:47

01:18:00

2015.1.00908.S

Thakeray_a_03_TP

Outflows and Dissipation in a distant Lehnert
QSO and SMG pair: Where does theenergy go?
Thackeray's Globules
ReipurthNA

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:41:02

00:29:21

2015.1.00908.S

Thakeray_a_03_TP

Thackeray's Globules

ReipurthNA

Total Power

3

23:28:57

00:29:45

2015.1.01572.S

pks0718-_a_06_TE

AGN Feedback and its Role in Galaxy Prandoni
Evolution: gas and stellar kinematics
of radio-loud early-type galaxies

EU

12-m

6

23:12:16

23:28:33

2015.1.00932.S

QSO_B082_a_06_TC

Measuring the Spectral Evolution,

NA

12-m

6

2016-05-02

Meyer22:52:57

23:40:21

2015.1.01025.S

TUKH122_a_03_TP

22:31:47

23:57:29

2015.1.00196.S

LMC0NT19_a_03_7M

22:25:13

22:52:31

2015.1.00196.S

LMC0NT19_b_03_TP

Structure, and Speed of Extragalactic
Jets with ALMA
Investigating the dyncamics of a
Ohashithermal starless core in the Orion A
cloud.
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

EA

Total Power

3

NA

7-m

3

NA

Total Power

3