ALMA Observing Activity from 2016-06-06T17:59:00 to 2016-06-13T18:00:00
QA0 pass executions
2016-06-13
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

10:55:27

11:21:27

2015.1.00196.S

Uranus_a_06_TP

Start (UT)

End (UT)

Project Code22:47:35

23:20:48

21:10:39

PI

Executive

Array

Band

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

NA

Total Power

6

SchedBlock

Project Title

Executive

Array

Band

2015.1.00960.S

NGC_3393_a_03_TE

NA

12-m

3

21:57:56

2015.1.00956.S

NGC_3351_a_06_TP

NA

Total Power

6

19:07:35

19:54:59

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

18:06:56

18:54:10

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

17:39:00

18:53:50

2015.1.00196.S

LMC0NT19_a_03_7M

SiO megamasers in AGN accretion Pesce
disks
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
Investigating the dyncamics of a
Ohashithermal starless core in the Orion A
cloud.
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

NA

7-m

3

17:18:56

18:06:30

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

16:30:15

17:18:30

2015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

16:09:32

17:24:06

2015.1.00196.S

LMC0NT19_a_03_7M

Investigating the dyncamics of a
Ohashithermal starless core in the Orion A
cloud.
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

NA

7-m

3

15:28:30

16:16:03

2015.1.01025.S

TUKH122_a_03_TP

Ohashi

EA

Total Power

3

15:28:06

15:52:43

2015.1.00697.S

sn_1987a_b_04_TE

Cherchneff

EU

12-m

4

15:03:06

15:27:192015.1.00697.S

sn_1987a_a_04_TE

Cherchneff

EU

12-m

4

14:42:32

16:08:49

2015.1.00196.S

LMC0NT19_a_03_7M

Investigating the dyncamics of athermal starless core in the Orion A
cloud.
Peering into the ejecta of SN1987A:
chemistry, clumpiness andnucleosynthesis
Peering into the ejecta of SN1987A:
chemistry, clumpiness andnucleosynthesis
Zooming in on the parsec-scale
structure of CO gas at low metallicity
and its relation to star formation

Roman-Duval

NA

7-m

3

14:39:58

15:28:072015.1.01025.S

TUKH122_a_03_TP

EA

Total Power

3

14:19:57

14:41:43

2015.1.00960.S

NGC_1386_a_03_TE

NA

12-m

3

13:47:06

14:08:02

2015.1.00419.S

NGC1574_a_06_TC

EU

12-m

6

13:28:54

13:46:26

2015.1.00932.S

4C_28.07_a_06_TC

NA

12-m

6

13:21:38

14:01:26

2015.1.00196.S

SMC2N66_a_03_TP

Investigating the dyncamics of a
Ohashithermal starless core in the Orion A
cloud.
SiO megamasers in AGN accretion Pesce
disks
WISDOM: Extending black holeDavisdemographics across the mass-size
plane with ALMA
Measuring the Spectral Evolution,
Meyer
Structure, and Speed of Extragalactic
Jets with ALMA
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power3

13:02:58

13:28:11

2015.1.01548.S

A3088_a_06_TC

Egami

NA

12-m

6

11:16:44

12:42:54

2015.1.00894.S

SPT-CL_J_a_03_7M

ALMA Imaging of Bright ClusterLensed SMGs Discovered by the
Herschel Lensing Survey
First spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effectKitayama

EA

7-m

3

10:40:04

12:22:42

2015.1.00752.S

HXMM20_a_03_TE

Bussmann

NA

12-m

3

09:54:44

11:16:00

2015.1.00894.S

SPT-CL_J_a_03_7M

ALMA Unveils the HierarchicalFormation of Massive Galaxies
First spatially-resolved imaging of a
massively star-forming, cooling-flow
galaxy cluster core using theSunyaev-Zel'dovich effectKitayama

EA

7-m

3

2016-06-12
PI08:33:05

09:54:06

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

07:02:59

08:32:44

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

05:33:02

07:02:23

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

04:57:49

05:32:03

2015.1.00601.S

mosaic3_a_03_TP

EU

Total Power

3

04:20:27

05:32:13

2015.1.01584.S

M17SW_a_03_TE

EA

12-m

3

04:18:27

04:40:27

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

03:58:07

04:17:27

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

03:33:44

03:54:16

2015.1.01014.S

SDC340.9_a_03_TP

EU

Total Power

3

03:20:57

04:17:38

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

03:01:11

04:10:00

2015.1.00369.S

G11.11-0_a_03_TE

NA

12-m

3

01:40:53

02:15:38

2015.1.01014.S

SDC326.4_a_03_TP

EU

Total Power3

01:08:10

02:23:32

2015.1.00964.S

HD143006_a_06_TE

NA

12-m

6

01:01:18

02:15:38

2015.1.00306.S

Lupus_3__b_03_7M

NA

7-m

3

00:33:30

01:16:33

2015.1.00956.S

NGC_4535_a_06_TP

Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
South
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
South
G351.77--0.51: ridge formation caught Leurini
in the act
A statistical study of molecular clumps Ishii
in the triggered star-forming region
M17SW
G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
What can hubs tell us on massive star Peretto
formation?
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
SouthThe evolution of outflows from high- Rosero
mass stars
What can hubs tell us on massive star Peretto
formation?
The astrochemical evolution from disk Oberg
formation to disk dissipation
The earliest stages of molecular
Plunkett
outflow activity from the young
protostar Lupus 3 MMS
How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?

NA

Total Power

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:49:38

00:33:10

2015.1.00956.S

NGC_4535_a_06_TP

NA

Total Power

6

23:38:44

00:40:51

2015.1.00623.S

Abell_17_a_06_TE

EU

12-m

6

23:15:31

00:35:072015.1.01593.S

m83_a_03_7M

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
AGN feedback and jet triggered star Russell
formation in Abell 1795
Multi CO line imaging of the nearby Hirota
galaxy M83: Variation of cloudproperties across the g|observe gas
clouds dens alactic structures

EA

7-m

3

23:02:09

23:46:54

2015.1.00357.S

G286_5_a_06_TP

NA

Total Power6

23:00:46

23:25:23

2015.1.00598.S

NGC3169_a_06_TE

EU

12-m

6

22:34:31

22:59:06

2015.1.00598.S

NGC3607_a_06_TE

EU

12-m

6

22:16:09

23:01:02

2015.1.00357.S

G286_4_a_06_TP

NA

Total Power

6

21:47:40

23:12:39

2015.1.00908.S

Thakeray_a_03_7M

Kinematics of Massive Star Cluster in Tan
Formation
WISDOM: CO Imaging of SMBH
BureauMass Measurement Candidates
WISDOM: CO Imaging of SMBH
BureauMass Measurement Candidates
Kinematics of Massive Star Cluster in Tan
Formation
Thackeray's Globules
Reipurth

NA

7-m

3

21:46:28

22:17:54

2015.1.00483.S

Centauru_c_03_TE

Israel

EU

12-m

3

18:56:42

20:08:46

2015.1.00661.S

TXS0828+_a_03_TE

Fogasy

EU

12-m

3

17:39:41

18:54:54

2015.1.00661.S

TXS0828+_a_03_TE

Fogasy

EU

12-m

3

16:43:12

17:58:06

2015.1.00196.S

LMC0NT19_a_03_7M

The nature of the Centaurus A
circumnuclear diskStar formation outside of powerful
AGN host galaxies
Star formation outside of powerful
AGN host galaxies
Zooming in on the parsec-scale
structure of CO gas at low metallicity
and its relation to star formation

Roman-Duval

NA

7-m

3

16:15:34

17:19:32

2015.1.01222.S

SXDF-ALM_a_03_TE

Investigating the nature of a new dust Yamaguchi
obscured star forming galaxy which
can only be understood via deep
ALMA spectroscopy

EA

12-m

3

15:27:51

16:42:32

2015.1.00196.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

15:27:08

15:53:57

2015.1.00196.S

LMC1N127_b_03_TP

Zooming in on the parsec-scale
structure of CO gas at low

NA

Total Power

3

2016-06-11
PI

Roman-Duvalmetallicity and its relation to starformation
Bright End of Number Counts
HatsukadeRevealed by ALMA
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

14:49:06

16:05:56

2015.1.00442.S

SXDS-AzT_a_06_TE

EA

12-m

6

14:44:59

15:11:46

2015.1.00196.S

LMC1N127_b_03_TP

NA

Total Power

3

14:17:23

15:13:35

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

14:03:14

14:44:12

2015.1.00196.S

LMC0NT19_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

13:25:39

14:11:02

2015.1.01222.S

SXDF-ALM_b_03_TE

Investigating the nature of a new dust Yamaguchi
obscured star forming galaxy which
can only be understood via deep
ALMA spectroscopy

EA

12-m

3

13:21:12

14:02:24

2015.1.00196.S

LMC0NT19_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

12:51:27

14:16:30

2015.1.00196.S

SMC0N69_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

12:48:47

13:20:49

2015.1.00196.S

SMC2N66_a_06_TP

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

NA

Total Power

6

12:39:59

13:25:20

2015.1.01222.S

SXDF-ALM_b_03_TE

Investigating the nature of a new dust Yamaguchi
obscured star forming galaxy which
can only be understood via deep
ALMA spectroscopy

EA

12-m

3

11:55:50

12:27:28

2015.1.00196.S

SMC2N66_a_06_TP

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

NA

Total Power

6

11:34:15

12:29:09

2015.1.01222.S

SXDF-ALM_b_03_TE

Investigating the nature of a new dust Yamaguchi
obscured star forming galaxy which
can only be understood via deep
ALMA spectroscopy

EA

12-m

3

11:05:42

12:30:57

2015.1.00196.S

SMC0N69_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

10:54:02

11:34:05

2015.1.00196.S

SMC2N66_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

10:13:34

10:53:43

2015.1.00196.S

SMC2N66_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 Power3

09:40:20

11:04:57

2015.1.00196.S

SMC0N69_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

09:32:48

10:13:11

2015.1.00196.S

SMC2N66_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 Power3

08:32:39

09:08:30

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

07:56:24

08:32:192015.1.00601.S

mosaic2_a_03_TP

EU

Total Power

3

07:21:38

08:52:58

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

06:59:35

07:36:00

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power3

06:39:43

07:54:28

2015.1.01332.S

TC2_a_03_TE

G351.77--0.51: ridge formation caught Leurini
in the act
G351.77--0.51: ridge formation caught Leurini
in the act
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
South
G351.77--0.51: ridge formation caught Leurini
in the act
Radiatively-Driven Implosion in the
LeflochTrifid Nebula

CL

12-m

3

Kitayama

06:13:41

06:58:53

2015.1.01014.S

SDC326.4_a_03_TP

What can hubs tell us on massive star Peretto
formation?
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
SouthHCO as a precursor of astrobiological Rivillamolecules
What can hubs tell us on massive star Peretto
formation?
HCO as a precursor of astrobiological Rivillamolecules
What can hubs tell us on massive star Peretto
formation?
What can hubs tell us on massive star Peretto
formation?
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
South
Radiatively-Driven Implosion in the
LeflochTrifid Nebula
What can hubs tell us on massive star Peretto
formation?
ALMA Survey of Gas Evolution in
Panic
Herbig Ae Population
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
AGN Feedback and its Role in Galaxy Prandoni
Evolution: gas and stellar kinematics
of radio-loud early-type galaxies

EU

Total Power3

05:49:38

07:20:47

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

05:25:31

06:39:21

2015.1.01193.S

IRAS1629_a_03_TE

EU

12-m

3

05:21:56

05:49:18

2015.1.01014.S

SDC326.4_a_03_TP

EU

Total Power

3

04:17:48

05:25:12

2015.1.01193.S

IRAS1629_a_03_TE

EU

12-m

3

04:15:39

04:54:32

2015.1.01014.S

SDC326.4_a_03_TP

EU

Total Power

3

03:29:40

04:14:50

2015.1.01014.S

SDC326.4_a_03_TP

EU

Total Power

3

03:15:15

04:28:14

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

02:44:43

04:06:37

2015.1.01332.S

TC2_b_03_TE

CL

12-m

3

02:16:17

02:53:56

2015.1.01014.S

SDC340.9_a_03_TP

EU

Total Power3

02:08:44

02:34:26

2015.1.01600.S

HD144668_a_06_TE

EU

12-m

6

01:18:53

02:02:18

2015.1.00925.S

NGC_5068_a_06_TP

CL

Total Power6

01:14:50

02:08:00

2015.1.01572.S

ic4296_a_06_TE

EU

12-m

6

01:12:52

02:32:38

2015.1.01593.S

m83_a_03_7M

Multi CO line imaging of the nearby
galaxy M83: Variation of cloudproperties across the g|observe gas
clouds dens alactic structures

HirotaEA

7-m

3

00:35:15

01:18:10

2015.1.00956.S

NGC_4535_a_06_TP

NA

Total Power

600:56:14

2015.1.00598.S

NGC4061_a_06_TE

How Does Cloud-Scale Physics Drive Leroy
Galaxy Evolution?
WISDOM: CO Imaging of SMBH
BureauMass Measurement Candidates

00:21:27

EU

12-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:55:24

00:19:55

2015.1.00598.S

NGC3862_a_06_TE

Bureau

EU

12-m

6

23:27:26

00:47:10

2015.1.01593.S

m83_a_03_7M

WISDOM: CO Imaging of SMBH
Mass Measurement Candidates
Multi CO line imaging of the nearby
galaxy M83: Variation of cloudproperties across the g|observe gas
clouds dens alactic structures

HirotaEA

7-m

3

22:55:17

23:17:42

2015.1.00856.S

J1357+19_a_03_TE

NA

12-m

3

12:22:07

13:02:14

2015.1.00196.S

SMC2N66_a_03_TP

Searching for Molecular Gas in High- Murray
Velocity Clouds
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power

3

11:49:51

12:51:22

2015.1.01487.S

n613_a_03_TC

EA

12-m

3

11:41:44

12:21:48

2015.1.00196.S

SMC2N66_a_03_TP

Investigation of Molecular Clouds
Miyamoto
Traced by CI
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power3

11:02:03

12:23:34

2015.1.00196.S

SMC0N69_b_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

11:01:06

11:41:24

2015.1.00196.S

SMC2N66_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

10:43:07

11:49:32

2015.1.01487.S

n613_a_03_TC

EA

12-m

3

09:53:16

10:33:28

2015.1.00196.S

SMC2N66_a_03_TP

Investigation of Molecular Clouds
Miyamoto
Traced by CI
Zooming in on the parsec-scale
Roman-Duvalstructure of CO gas at low metallicity
and its relation to star formation

NA

Total Power3

09:42:24

10:42:32

2015.1.01487.S

n613_a_03_TC

Investigation of Molecular Clouds
Traced by CI

EA

12-m

3

2016-06-10

Miyamoto

09:12:29

09:52:36

2015.1.00196.S

SMC2N66_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 Power3

08:13:31

09:00:30

2015.1.00989.S

ngc_7465_a_03_TE

NA

12-m

3

08:07:13

08:43:12

2015.1.00601.S

mosaic2_a_03_TP

EU

Total Power3

07:45:04

09:16:192015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

07:19:05

07:50:48

2015.1.01014.S

SDC340.9_a_03_TP

EU

Total Power3

07:04:17

08:12:51

2015.1.00369.S

G11.11-0_a_03_TE

NA

12-m

3

06:29:53

07:18:26

2015.1.01014.S

SDC340.9_a_03_TP

EU

Total Power3

06:07:05

07:19:50

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

05:54:16

07:03:40

2015.1.00369.S

G11.11-0_a_03_TE

NA

12-m

3

05:24:38

06:04:29

2015.1.01014.S

SDC340.9_a_03_TP

EU

Total Power304:45:23

05:33:23

2015.1.01193.S

G31.41+0_a_03_TE

EU

12-m

3

04:35:51

05:24:03

2015.1.01014.S

SDC340.9_a_03_TP

EU

Total Power

3

04:35:31

06:06:47

2015.1.00223.S

Serpens__a_03_7M

EA

7-m

3

03:22:37

04:39:26

2015.1.01584.S

M17SW_a_03_TE

EA

12-m

3

01:44:56

02:38:01

2015.1.01014.S

SDC339.6_a_03_TP

EU

Total Power3

01:44:44

02:40:13

2015.1.00530.S

TN_J1338_a_03_7M

EU

7-m

3

00:58:28

02:10:14

2015.1.01599.S

Enceladus_a_06_TE

Does Cold Gas Fuel Almost All
Hodges-Kluck
AGNs?
G351.77--0.51: ridge formation caught Leurini
in the act
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
South
What can hubs tell us on massive star Peretto
formation?
The evolution of outflows from high- Rosero
mass stars
What can hubs tell us on massive star Peretto
formation?
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
SouthThe evolution of outflows from high- Rosero
mass stars
What can hubs tell us on massive star Peretto
formation?
HCO as a precursor of astrobiological Rivillamolecules
What can hubs tell us on massive star Peretto
formation?
Revealing Fragmentation of the
Nakamura
Nearest Precluster Clump in Serpens
SouthA statistical study of molecular clumps Ishii
in the triggered star-forming region
M17SW
What can hubs tell us on massive star Peretto
formation?
An ALMA-MUSE Survey of Extended De Breuck
Radio Galaxy Haloes
Remote Detection of Organics in
LoomisEnceladus' Plume

NA

12-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:43:44

00:55:48

2015.1.01599.S

Enceladus_a_06_TE

NA

12-m

6

22:39:30

22:57:31

2015.1.01590.S

Gal3_a_04_TE

CL

12-m

4

22:37:40

23:22:30

2015.1.00357.S

G286_4_a_06_TP

NA

Total Power

6

21:54:44

22:33:34

2015.1.00190.S

HR_3126_a_03_TP

NA

Total Power

3

14:50:36

15:41:51

2015.1.00340.S

MC27_a_06_TP

EA

Total Power

6

13:58:39

15:15:48

2015.1.00442.S

SXDS-AzT_a_06_TE

EA

12-m

6

13:53:26

14:50:14

2015.1.01125.S

SMCB1clo_a_06_7M

NA

7-m

6

13:23:32

14:25:21

2015.1.00274.S

NGC253_a_07_TP

Remote Detection of Organics in
LoomisEnceladus' Plume
Constraining the molecular gas
Cassatacontent of normal star-forming
galaxies at 3<z<3.5
Kinematics of Massive Star Cluster in Tan
Formation
Getting to the bottom of the Toby Jug Rawlings- Mapping the bipolar reflection
nebula IC2220
Investigating the dynamical interaction Tokuda
at the formation of a multiple starsystemBright End of Number Counts
HatsukadeRevealed by ALMA
SMC B1 #1 is the New Perseus: The Sandstrom
Relationship Between Av and CO at
Low Metallicity
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

Total Power7

13:06:05

13:55:192015.1.00869.S

SN_1978K_a_06_TE

NA

12-m

6

12:34:16

13:52:45

2015.1.01125.S

SMCB1clo_a_06_7M

NA

7-m

6

12:20:57

13:22:53

2015.1.00274.S

NGC253_a_07_TP

Studying the Late-Time Evolution of Smith
SN 1978K
SMC B1 #1 is the New Perseus: The Sandstrom
Relationship Between Av and CO at
Low Metallicity
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

Total Power

7

12:16:14

13:04:44

2015.1.00633.S

HD_15115_a_06_TE

Debris Disk Structure Disentangled

Weinberger

NA

12-m

6

11:35:06

12:06:53

2015.1.00196.S

SMC0N69_a_06_TP

Zooming in on the parsec-scale
structure of CO gas at low

Roman-Duval

NA

Total Power6

2016-06-09
PI11:01:58

11:33:59

2015.1.00196.S

SMC0N69_a_06_TP

11:01:02

12:20:03

2015.1.01125.S

SMCB1clo_a_06_7M

10:38:11

12:05:11

2015.1.00442.S

SXDS-AzT_a_06_TE

09:58:58

11:01:08

2015.1.00274.S

NGC253_a_07_TP

09:40:17

10:37:23

2015.1.00326.S

IRAS_191_a_03_TE

09:36:40

11:00:10

2015.1.00997.S

SDSS_J23_a_06_7M

08:56:16

09:58:21

2015.1.00274.S

NGC253_a_07_TP

08:42:27

09:39:40

2015.1.00326.S

IRAS_191_a_03_TE

08:21:07

09:36:18

2015.1.00959.S

G028.539_a_06_7M

07:44:22

08:41:51

2015.1.00326.S

IRAS_191_a_03_TE

06:53:24

08:20:24

2015.1.00959.S

G028.539_a_06_7M

06:22:38

07:30:12

2015.1.00678.S

AS_209_a_07_TE

05:14:00

06:22:21

2015.1.00678.S

AS_209_a_07_TE

04:13:22

05:13:17

2015.1.00678.S

IM_Lup_a_07_TE

03:41:13

04:12:21

2015.1.00102.S

IRAS_131_b_07_TE

03:24:05

04:37:10

2015.1.00121.S

M83_a_06_7M

03:11:05

03:40:32

2015.1.00102.S

IRAS_131_a_07_TE

02:48:56

03:32:14

2015.1.00925.S

NGC_5068_a_06_TP

02:04:54

02:48:17

2015.1.00925.S

NGC_5068_b_06_TP

02:03:46

03:23:28

2015.1.00121.S

M83_a_06_7M

01:03:43

01:41:44

2015.1.00925.S

NGC_5068_b_06_TP

00:27:33

00:43:26

2015.1.00872.S

PG_1149-_a_06_TE

00:18:02

01:03:23

2015.1.00357.S

G286_4_a_06_TP

00:18:01

01:35:54

2015.1.00121.S

M83_a_06_7M

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

NA

Total Power

6

SMC B1 #1 is the New Perseus: The Sandstrom
Relationship Between Av and CO at
Low Metallicity
Bright End of Number Counts
HatsukadeRevealed by ALMA
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

NA

7-m

6

EA

12-m

6

NA

Total Power

7

A detailed view of the Bird's anatomy: RomeroSF/AGN feedback
Canizales
Extreme quasar feedback in the early Maiolino
Universe
A Close Look into the Blast Furnace: Bolatto
the Core of the NGC253 Starburst at
One Parsec Resolution

CL

12-m

3

EU

7-m

6

NA

Total Power

7

A detailed view of the Bird's anatomy: RomeroSF/AGN feedback
Canizales
A Systematic ALMA Survey of the
Shirley
Most Massive Starless Clumps within
5kpc
A detailed view of the Bird's anatomy: RomeroSF/AGN feedback
Canizales
A Systematic ALMA Survey of the
Shirley
Most Massive Starless Clumps within
5kpc
Survey of CO Snow Lines in Solar
Qi
Nebula Analogues
Survey of CO Snow Lines in Solar
Qi
Nebula Analogues
Survey of CO Snow Lines in Solar
Qi
Nebula Analogues
Warm and Dense Molecular Gas in Iono
Local Merging ULIRGs
Molecular Clouds and Star Formation: Sakamoto
Inner Disk of M83
Warm and Dense Molecular Gas in Iono
Local Merging ULIRGs
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Molecular Clouds and Star Formation: Sakamoto
Inner Disk of M83
Promoting Diversity: ISM Physics and Blanc
Star Formation across Different
Environments
Is the central sub-kiloparsec gas
Schulzesurface-density the decisive
parameter for fueling supermassive
black holes?

CL

12-m

3

NA

7-m

6

CL

12-m

3

NA

7-m

6

NA

12-m

7

NA

12-m

7

NA

12-m

7

EA

12-m

7

EA

7-m

6

EA

12-m

7

CL

Total Power

6

CL

Total Power

6

EA

7-m

6

CL

Total Power

6

EA

12-m

6

Kinematics of Massive Star Cluster in Tan
Formation
Molecular Clouds and Star Formation: Sakamoto
Inner Disk of M83

NA

Total Power

6

EA

7-m

6