ALMA Observing Activity from 2016-08-01T17:59:00 to 2016-08-08T18:00:00
QA0 pass executions
2016-08-07
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

09:21:24

10:20:33

2015.1.00665.S

0413_238_a_06_TP

08:46:27

10:01:16

2015.1.00834.S

08:27:57

09:19:58

08:27:30

PI

Executive

Array

Band

After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

WMH_5_a_06_TE

Resolving a main-sequence starforming galaxy merger at redshift 6

NA

12-m

6

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power3

09:49:22

2015.1.00925.S

NGC_1300_b_06_7M

CL

7-m

6

07:52:32

08:26:06

2015.1.00587.S

CIG55_a_03_TE

EU

12-m

3

06:27:56

07:42:30

2015.1.00212.S

mADF22_a_03_TE

Investigating the dyncamics of a
Ohashithermal starless core in the Orion A
cloud.
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Why do isolated galaxies host red
Verdespseudobulges?
Montenegro
Dense Molecular Gas Mapping of the Umehata
Node in the Cosmic Web at z=3.1

EA

12-m

3

05:10:45

06:25:04

2015.1.00212.S

mADF22_a_03_TE

Dense Molecular Gas Mapping of the Umehata
Node in the Cosmic Web at z=3.1

EA

12-m

3

04:21:06

04:59:41

2015.1.01452.S

1-3_b_03_TE

EA

12-m

3

04:18:39

05:10:38

2015.1.01014.S

SDC338.3_a_03_TP

EU

Total Power

3

03:49:25

04:19:45

2015.1.00734.T

Neutron__b_03_TE

CO spectral scanning of z>6.5 QSO Koptelova
candidates selected fromPanSTARRS
What can hubs tell us on massive star Peretto
formation?
Exploring the nature of relativistic jets Diaz Trigoin neutron star X-ray binaries - Part 2

EU

12-m

3

03:24:30

04:45:14

2015.1.00230.S

NGC6334-_b_03_7M

EA

7-m

3

03:24:29

04:04:41

2015.1.00601.S

mosaic2_a_03_TP

Mass accretion flows in high-mass
Liustar formation
G351.77--0.51: ridge formation caught Leurini
in the act

EUTotal Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

12:22:28

13:13:31

2015.1.01008.S

HOPS-247_a_06_TP

NA

Total Power

6

11:26:43

12:38:18

2015.1.00925.S

NGC_1433_a_06_7M

CL

7-m

6

11:25:25

12:20:18

2015.1.00665.S

0413_238_a_06_TP

Mapping Infall in Filamentary
MegeathEnvironments: A Study of three Orion
Class 0 Protostars
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power

6

11:23:48

12:42:41

2015.1.01108.S

DG_Tau_B_a_06_TE

CL

12-m

6

09:49:57

11:05:33

2015.1.00834.S

WMH_5_a_06_TE

A molecular disk wind from DG Tau B Louvet?
Resolving a main-sequence starWillott
forming galaxy merger at redshift 6

NA

12-m

6

09:35:26

10:30:03

2015.1.00665.S

0413_238_a_06_TP

After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

09:35:07

10:57:58

2015.1.00925.S

NGC_1433_b_06_7M

CL

7-m

6

08:54:39

09:09:16

2015.1.00925.S

NGC_1087_a_06_TP

CL

Total Power6

08:21:47

08:53:34

2015.1.00196.S

SMC1N42_a_06_TP

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power6

08:20:11

09:35:22

2015.1.00834.S

WMH_5_a_06_TE

Resolving a main-sequence starforming galaxy merger at redshift 6

Willott

NA

12-m

6

06:55:15

08:16:192015.1.00925.S

NGC_1300_b_06_7M

CL

7-m

6

06:52:46

08:10:22

2015.1.00762.S

WD2226-2_a_06_TE

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
The nature and origin of the Solar
Ertel
system scale disk in the Helix Nebula

EU

12-m

6

05:47:27

06:51:37

2015.1.00734.T

Neutron__b_07_TE

Exploring the nature of relativistic jets Diaz Trigoin neutron star X-

EU

12-m

7

Willott

2016-08-05
PIray binaries - Part 2

2016-08-04
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

17:54:41

18:39:37

2015.1.00956.S

NGC_3627_b_06_TP

17:11:50

17:44:16

2015.1.01271.S

RW_LMi_a_03_TE

17:04:35

17:51:44

2015.1.00956.S

NGC_3351_a_06_TP

16:39:30

17:55:21

2015.1.00956.S

NGC_3351_a_06_7M

16:14:19

17:01:41

2015.1.00956.S

NGC_3351_a_06_TP

16:11:13

17:11:072015.1.01320.S

G09.97_a_04_TE

15:21:50

16:12:34

2015.1.01008.S

HOPS-178_a_06_TP

15:15:12

16:37:192015.1.01339.S

HG2907_a_06_7M

15:06:55

16:09:46

2015.1.01452.S

11-16_b_03_TE

14:30:21

15:21:072015.1.01008.S

HOPS-178_a_06_TP

13:51:56

15:14:06

2015.1.01339.S

HG2794_a_06_7M

13:39:06

14:30:01

2015.1.01008.S

HOPS-178_a_06_TP

12:44:29

13:35:32

2015.1.01008.S

HOPS-178_a_06_TP

12:25:27

13:37:06

2015.1.00925.S

NGC_1433_b_06_7M

12:07:17

13:22:58

2015.1.00040.S

ALESS73._a_04_TE

11:49:00

12:43:46

2015.1.00665.S

10:58:24

12:24:59

09:43:56

PI

Executive

Array

Band

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Circumstellar chemistry in carbon
Kellerstars: How unique is IRC+10216?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Dissecting starbursts at z=3.6 through Omont
multi-line H2O imaging
Mapping Infall in Filamentary
MegeathEnvironments: A Study of three Orion
Class 0 Protostars
Identifying the transition phase of the Olmiclump mass function toward the IMF

NATotal Power

6

EU

12-m

3

NA

Total Power

6

NA

7-m

6

NA

Total Power

6

EU

12-m

4

NA

Total Power

6

EU

7-m

6

CO spectral scanning of z>6.5 QSO Koptelova
candidates selected fromPanSTARRS
Mapping Infall in Filamentary
MegeathEnvironments: A Study of three Orion
Class 0 Protostars
Identifying the transition phase of the Olmiclump mass function toward the IMF

EA

12-m

3

NA

Total Power

6

EU

7-m

6

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
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Using [CI]to determine the distribution De Breuckand heating mechanism of H2 in az=4.8 star-forming disk

NA

Total Power

6

NA

Total Power

6

CL

7-m

6

EU

12-m

4

0413_238_a_06_TP

After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

2015.1.00925.S

NGC_1300_a_06_7M

CL

7-m

6

10:38:33

2015.1.00665.S

0413_238_a_06_TP

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

09:35:23

10:57:39

2015.1.00925.S

NGC_1433_b_06_7M

CL

7-m

6

08:47:39

09:56:37

2015.1.00404.S

NGC_613_a_07_TE

EU

12-m

7

08:46:50

09:41:26

2015.1.00665.S

0413_238_a_06_TP

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Gas fueling and outflow around
Combesmassive black holes
After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

08:12:52

09:34:12

2015.1.00925.S

NGC_1300_a_06_7M

CL

7-m

6

08:02:14

08:45:48

2015.1.00925.S

NGC_1087_a_06_TP

CL

Total Power6

07:19:47

08:44:25

2015.1.00834.S

WMH_5_a_06_TE

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Resolving a main-sequence starWillott
forming galaxy merger at redshift 6

NA

12-m

6

07:17:59

08:01:55

2015.1.00925.S

NGC_1300_a_06_TP

CL

Total Power

6

06:53:37

08:10:31

2015.1.00925.S

NGC_1433_b_06_7M

CL

7-m

6

06:27:24

07:11:02

2015.1.00925.S

NGC_1087_a_06_TP

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

CL

Total Power

6

05:59:21

07:16:03

2015.1.00762.S

WD2226-2_a_06_TE

The nature and origin of the Solar
Ertel
system scale disk in the Helix Nebula

EU

12-m

6

05:48:20

06:26:57

2015.1.00601.S

mosaic1_a_03_TP

EU

Total Power

3

05:32:54

06:48:36

2015.1.01013.S

MagBridg_a_06_7M

G351.77--0.51: ridge formation caught Leurini
in the act
Physical Properties and Submillimeter Rubio
Exccess in low metallicity clouds in
the Magellanic Bridge

CL

7-m

6

05:10:41

05:46:38

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

04:58:06

05:58:072015.1.00250.S

BX610_a_06_TE

G351.77--0.51: ridge formation caught Leurini
in the act
Resolving the molecular ISM in a
Aravenaunique star-forming disk galaxy at z=2

CL

12-m

6

04:43:03

05:10:21

2015.1.00667.S

AG22.36+_j_06_TP

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

Wang

EU

Total Power

604:15:25

04:42:45

2015.1.00667.S

AG22.36+_i_06_TP

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

Wang

EU

Total Power

604:05:12

05:32:34

2015.1.00023.S

HD_16329_a_06_7M

EU

7-m

6

03:47:23

04:14:38

2015.1.00667.S

AG22.36+_g_06_TP

Understanding the Disk Wind from HD Klaassen
163296Mass assembly in the pre-stellar
Wangphase of high-mass star formation

EU

Total Power6

03:19:11

03:46:34

2015.1.00667.S

AG22.36+_h_06_TP

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

Wang

EU

Total Power

602:50:41

03:18:05

2015.1.00667.S

AG22.36+_j_06_TP

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

Wang

EU

Total Power602:45:21

04:29:30

2015.1.00311.S

sgra_sta_a_06_TE

ALMA probes the SagA* Accretion

Murchikova

NA

12-m

6

02:31:59

03:54:08

2015.1.00023.S

HD_16329_a_06_7M

EU

7-m

6

02:22:26

02:50:22

2015.1.00667.S

AG22.36+_g_06_TP

Understanding the Disk Wind from HD Klaassen
163296Mass assembly in the pre-stellar
Wangphase of high-mass star formation

EU

Total Power

6

01:35:09

02:22:03

2015.1.00601.S

mosaic3_a_03_TP

EU

Total Power

3

01:23:13

02:11:53

2015.1.00072.S

G31.41+0_b_06_TE

EU

12-m

6

01:10:13

02:31:38

2015.1.00601.S

mosaic2_a_03_7M

EU

7-m

3

01:03:25

01:30:59

2015.1.00667.S

AG22.36+_h_06_TP

G351.77--0.51: ridge formation caught Leurini
in the act
Does the magnetic field regulate the Beltran
collapse in the massive coreG31.41+0.31?
G351.77--0.51: ridge formation caught Leurini
in the act
Mass assembly in the pre-stellar
Wangphase of high-mass star formation

EU

Total Power

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

12:09:49

13:25:30

2015.1.00196.S

LMC0NT19_a_06_7M

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

NA

7-m

6

11:41:18

12:57:46

2015.1.00040.S

ALESS73._a_04_TE

Using [CI]to determine the distribution De Breuckand heating mechanism of H2 in az=4.8 star-forming disk

EU

12-m

4

11:05:52

12:09:25

2015.1.00331.S

L1451-we_a_06_7M

NA

7-m

6

10:09:23

11:04:11

2015.1.00665.S

0413_238_a_06_TP

A Tale of Two Cores: Stellar Birth in Storm
the Young L1451 Region
After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

09:49:06

11:05:072015.1.01013.S

MagBridg_a_06_7M

Physical Properties and Submillimeter Rubio
Exccess in low metallicity clouds in
the Magellanic Bridge

CL

7-m

6

09:14:20

10:09:04

2015.1.00665.S

0413_238_a_06_TP

After the Fall: Mapping the Molecular Smith
Fuel in Post-Starburst Galaxies

NA

Total Power6

09:06:04

10:20:58

2015.1.00834.S

WMH_5_a_06_TE

Resolving a main-sequence starforming galaxy merger at redshift 6

Willott

NA

12-m

6

08:37:33

09:48:25

2015.1.01013.S

MagBridg_a_06_7M

Physical Properties and Submillimeter Rubio
Exccess in low metallicity clouds in
the Magellanic Bridge

CL

7-m

6

08:30:26

09:13:53

2015.1.00925.S

NGC_1087_a_06_TP

Promoting Diversity: ISM Physics and Blanc
Star Formation acrossCL

Total Power6

2016-08-03
PIDifferent Environments
08:26:08

09:04:32

2015.1.01148.S

W0149+23_a_03_TE

Molecular gas in WISE-selected
Fan
Hyper-luminous Hot, Dust-obscured
Galaxies
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Resolving the molecular ISM in a
Aravenaunique star-forming disk galaxy at z=2

OTHER

12-m

3

07:46:48

08:29:50

2015.1.00925.S

NGC_1087_a_06_TP

CL

Total Power6

07:19:24

08:22:36

2015.1.00250.S

BX610_a_06_TE

CL

12-m

6

07:04:37

08:36:46

2015.1.00897.S

MRC0156-_a_03_7M

Cold gas halos at z~2: evolution of
Emontsmassive galaxies within a molecular
IGM
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Collisional star-formation in the SMC: Muller
NGC346Mass assembly in the pre-stellar
Wangphase of high-mass star formation

EU

7-m

3

07:02:01

07:46:08

2015.1.00925.S

NGC_1087_a_06_TP

CL

Total Power6

06:12:33

07:00:55

2015.1.01296.S

NGC345-p_a_06_TP

EA

Total Power

605:44:24

06:11:43

2015.1.00667.S

AG22.36+_k_06_TP

EU

Total Power

605:31:57

07:03:43

2015.1.00897.S

MRC0156-_a_03_7M

Cold gas halos at z~2: evolution ofmassive galaxies within a molecular
IGM
Mass assembly in the pre-stellar
phase of high-mass star formation

EmontsEU7-m

3

05:16:12

05:43:40

2015.1.00667.S

AG22.36+_k_06_TP

Wang

EU

Total Power

604:44:48

05:12:18

2015.1.00667.S

AG22.36+_l_06_TP

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

Wang

EU

Total Power6

04:16:09

04:43:51

2015.1.00667.S

AG22.36+_l_06_TP

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

Wang

EU

Total Power

6

04:06:34

05:59:52

2015.1.01018.S

B335_a_07_TE

Yen

EA

12-m

7

02:17:57

04:05:28

2015.1.01018.S

B335_a_07_TE

Yen

EA

12-m

7

01:49:16

02:16:49

2015.1.00667.S

AG22.36+_e_06_TP

Magnetic Field Structure around a
Protostar with Effective Magnetic
Braking
Magnetic Field Structure around a
Protostar with Effective Magnetic
Braking
Mass assembly in the pre-stellar
phase of high-mass star formation

Wang

EU

Total Power

6

01:45:11

03:06:35

2015.1.00601.S

mosaic2_a_03_7M

EU

7-m

3

01:39:36

02:06:51

2015.1.00734.T

Neutron__a_03_TE

G351.77--0.51: ridge formation caught Leurini
in the act
Exploring the nature of relativistic jets Diaz Trigoin neutron star X-ray binaries - Part 2

EU

12-m

3

01:20:25

01:47:53

2015.1.00667.S

AG22.36+_e_06_TP

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

Wang

EU

Total Power

600:52:08

01:19:32

2015.1.00667.S

AG22.36+_f_06_TP

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

Wang

EU

Total Power

600:35:09

01:38:48

2015.1.00734.T

Neutron__a_07_TE

Exploring the nature of relativistic jets Diaz Trigoin neutron star X-ray binaries - Part 2

EU

12-m

7

00:24:02

00:51:22

2015.1.00667.S

AG22.36+_f_06_TP

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

Wang

EU

Total Power

600:22:46

01:44:49

2015.1.00601.S

mosaic2_a_03_7M

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

EU

7-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:17:58

00:23:03

2015.A.00022.T

NGC6334I_b_07_TE

Measuring the Luminosity of an ALMA Hunter
Detected Accretion Event in the
Massive Protostellar Cluster
NGC6334I

NA

12-m

7

22:15:06

23:16:12

2015.A.00022.T

NGC6334I_a_07_TE

Measuring the Luminosity of an ALMA Hunter
Detected Accretion Event in the
Massive Protostellar Cluster
NGC6334I

NA

12-m

7

21:40:11

22:27:22

2015.1.00956.S

NGC4303_a_06_TP

NA

Total Power

6

21:39:15

22:59:36

2015.1.00956.S

NGC_4321_a_06_7M

NA

7-m

6

19:31:06

20:18:31

2015.1.00956.S

NGC_3351_a_06_TP

NA

Total Power

6

19:25:02

20:03:13

2015.1.00199.S

WISE_J12_a_04_TE

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Proving the AGN feedback in the
Toba

EA

12-m

4

2016-08-02
PI18:55:53

20:11:11

2015.1.00956.S

NGC_3351_a_06_7M

18:46:52

19:30:14

2015.1.00925.S

NGC_5068_a_06_TP

18:08:09

19:07:12

2015.1.01569.S

He_2-10_a_03_TE

17:38:36

18:26:03

2015.1.00956.S

NGC_3351_a_06_TP

16:56:13

18:29:30

2015.1.01339.S

HG2794_a_06_7M

16:48:41

17:40:11

2015.1.00026.S

NIFS-HiZ_b_06_TE

15:51:58

16:37:44

2015.1.00262.S

OrionBul_a_03_TE

15:31:47

16:54:54

2015.1.01339.S

HG2794_a_06_7M

14:49:27

15:33:03

2015.1.00262.S

OrionBul_a_03_TE

14:33:30

15:33:11

2015.1.01082.S

Orion_Ba_a_07_TP

13:32:23

14:55:18

2015.1.01339.S

HG2907_a_06_7M

13:19:09

14:30:42

2015.1.00543.S

12:07:30

13:22:17

11:24:45

extremely IR-bright Dust Obscured
Galaxies
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
CO vs. CI in Henize 2-10
Imara

NA

7-m

6

CL

Total Power

6

NA

12-m

3

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Identifying the transition phase of the Olmiclump mass function toward the IMF

NATotal Power

6

EU

7-m

6

A resolved view to the dust content in Ibar
star-forming Halpha galaxies at z =1.47-2.23
Digging for rusty bullets at an
Ginsburg
explosion site
Identifying the transition phase of the Olmiclump mass function toward the IMF

CL

12-m

6

EU

12-m

3

EU

7-m

6

Digging for rusty bullets at an
Ginsburg
explosion site
ALMA imaging of the Orion Bar:
Goicoechea
Density structures and chemical
stratification in PDRs
Identifying the transition phase of the Olmiclump mass function toward the IMF

EU

12-m

3

EU

Total Power

7

EU

7-m

6

GOODS-S_f_06_TE

Towards a census of star-formation
since z~6 with ALMA-1.1mm

EU

12-m

6

2015.1.00196.S

LMC0NT19_a_06_7M

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

NA

7-m

6

12:36:21

2015.1.00543.S

GOODS-S_f_06_TE

Towards a census of star-formation
since z~6 with ALMA-1.1mm

Elbaz

EU

12-m

6

10:25:53

11:53:27

2015.1.00925.S

NGC_1300_a_06_7M

CL

7-m

6

10:14:14

11:16:02

2015.1.00274.S

NGC253_a_07_TP

Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

Total Power7

09:38:36

10:50:39

2015.1.00543.S

GOODS-S_f_06_TE

Towards a census of star-formation
since z~6 with ALMA-1.1mm

Elbaz

EU

12-m

6

09:11:21

10:13:55

2015.1.00274.S

NGC253_a_07_TP

A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

Total Power

708:59:13

10:10:13

2015.1.01013.S

MagBridg_a_06_7M

Physical Properties and Submillimeter Rubio
Exccess in low metallicity clouds in
the Magellanic Bridge

CL

7-m

6

08:23:45

09:38:13

2015.1.00543.S

GOODS-S_e_06_TE

Towards a census of star-formation
since z~6 with ALMA-1.1mm

Elbaz

EU

12-m

6

08:05:52

09:10:38

2015.1.00274.S

NGC253_a_07_TP

A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

Total Power

7

07:48:13

08:58:55

2015.1.01013.S

MagBridg_a_06_7M

Physical Properties and Submillimeter Rubio
Exccess in low metallicity clouds in
the Magellanic Bridge

CL

7-m

6

07:09:02

08:23:03

2015.1.00723.S

HXMM01_a_06_TE

EU

12-m

6

07:03:11

08:05:34

2015.1.00274.S

NGC253_a_07_TP

Dissecting the colossi: confronting
Oteo
recent theory with two multi-merging
HyLIRGs
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

Total Power7

06:13:58

07:02:05

2015.1.01296.S

NGC345-p_a_06_TP

EA

Total Power6

06:11:16

07:47:53

2015.1.00274.S

NGC253_a_07_7M

Collisional star-formation in the SMC: Muller
NGC346
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253

NA

7-m

7

Elbaz

Starburst at One Parsec Resolution
05:48:17

07:08:21

2015.1.00212.S

mADF22_a_03_TE

Dense Molecular Gas Mapping of the Umehata
Node in the Cosmic Web at z=3.1

EA

12-m

3

05:35:51

06:13:12

2015.1.00956.S

NGC_6744_a_06_TP

NA

Total Power

604:57:55

05:35:34

2015.1.00956.S

NGC_6744_a_06_TP

NA

Total Power

6

04:41:33

05:47:48

2015.1.01099.S

Serpens__a_06_TE

EU

12-m

6

03:48:10

04:04:52

2015.1.00956.S

NGC_6744_a_06_TP

NA

Total Power6

03:12:35

04:40:48

2015.1.01058.S

CrA-1_a_06_TE

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Imaging the circumstellar matter
Dionatosaround the Class 0 protostellar binary
SMM1/FIRS1 in Serpens
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Corona Australis Disk Zoo
Liu

EA

12-m

6

03:10:13

03:47:33

2015.1.00956.S

NGC_6744_a_06_TP

NA

Total Power6

02:32:10

03:09:51

2015.1.00956.S

NGC_6744_a_06_TP

NA

Total Power6

02:09:02

03:11:46

2015.1.00888.S

2MASS_J1_a_07_TE

EA

12-m

7

02:02:05

03:23:39

2015.1.00601.S

mosaic2_a_03_7M

EU

7-m

3

01:24:59

02:02:35

2015.1.00956.S

NGC_6744_a_06_TP

NA

Total Power

600:56:19

02:07:51

2015.1.00934.S

rho_Oph__a_07_TE

NA

12-m

7

00:42:24

02:01:14

2015.1.00749.S

G028.314_a_03_7M

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Probing disk structure in a cavity of Akiyama
pre-transitional disks around Sun-likeyoung stars
G351.77--0.51: ridge formation caught Leurini
in the act
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Investigating molecular gas in disks Ricciaround young Brown Dwarfs with
ALMA
Properties of the most distant starMottram
forming GMC in the Milky Way

EU

7-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:26:20

00:35:56

2015.1.01406.S

A1689-zD_a_06_TE

EU

12-m

6

23:24:43

00:02:06

2015.1.00121.S

M83_c_06_TP

EA

Total Power

6

22:47:20

00:15:21

2015.1.00023.S

HD_16329_a_06_7M

EU

7-m

6

22:46:02

23:23:38

2015.1.00121.S

M83_c_06_TP

EA

Total Power

6

22:42:14

23:23:40

2015.1.00449.S

13039-61_a_07_TE

Anomalously faint [CII]from a merger Watson
at z=7.60
Molecular Clouds and Star Formation: Sakamoto
Inner Disk of M83
Understanding the Disk Wind from HD Klaassen
163296
Molecular Clouds and Star Formation: Sakamoto
Inner Disk of M83
Fragmentation of massive dense
Fontaniclumps: unveiling the initial conditionsof high-mass star formation

EU

12-m

7

2016-08-01
PI