ALMA Observing Activity from 2018-01-08T17:59:00 to 2018-01-15T18:00:00
QA0 pass executions
2018-01-15
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

11:28:33

11:59:51

2017.1.01158.S

VV847_a_06_7M

ACA Study on the Driving
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

Yamashita

EA

7-m

6

11:25:27

11:46:08

2017.1.01167.S

PDS_66_a_06_TM2

CL

12-m

6

10:52:37

11:25:122017.1.00236.S

ngc_5861_a_06_TM1

ALMA CHARACTERIZATION OF T Perez
TAURI DISKS
Feeding and feedback in an unbiased Malkan
and representative sample of AGN in
the local Universe

NA

12-m

6

10:09:52

11:27:21

2017.1.00886.L

NGC4951_a_06_TP

EU NA

Total Power6

10:05:54

10:52:09

2017.1.00301.S

NA

12-m

6

09:58:31

11:28:25

2017.1.00886.L

EU NA

7-m

6

09:28:37

10:05:23

2017.1.00236.S

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
NGC_5193_a_06_TM1 Measuring black hole masses inBarthearly-type galaxies with ALMA
NGC5248_b_06_7M
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
ngc_5506_a_06_TM1
Feeding and feedback in an unbiased Malkan
and representative sample of AGN in
the local Universe

NA

12-m

6

08:51:23

10:09:39

2017.1.00886.L

NGC4207_a_06_TP

EU NA

Total Power608:40:33

09:27:10

2017.1.00693.S

BHR71-IR_a_06_TM1

EU

12-m

6

07:54:50

09:01:40

2017.1.00716.S

G305.79_a_06_7M

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Tracing the water content ofJorgensen
protostars in isolated cores
A survey of prestellar, high-mass
Sanhuezaclump candidates: constraining
models of high-mass star formation

EA

7-m

6

07:43:45

08:51:16

2017.1.00886.L

NGC2566_a_06_TP

EU NA

Total Power6

07:10:37

08:22:18

2017.1.01334.S

EU

12-m

6

06:48:41

07:54:41

2017.1.01158.S

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
2MASS_J1_a_06_TM1 Non accreting proto-planetary discs: a Rosotti
new evolutionary class?
12376540_a_06_7M
ACA Study on the Driving
Yamashita
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

EA

7-m

6

06:29:27

07:43:27

2017.1.00886.L

NGC2903_a_06_TP

EU NA

Total Power

605:21:06

06:29:18

2017.1.00886.L

EU NA

Total Power

605:20:13

06:48:32

2017.1.01644.S

EU

7-m

6

05:16:15

06:06:41

2017.1.00301.S

NA

12-m

6

03:45:07

04:55:32

2017.1.01102.S

NA

12-m

6

03:42:17

05:10:14

2017.1.00984.S

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
NGC2566_a_06_TP
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
GJ_273_a_06_7M
Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
ESO_208-_a_06_TM1 Measuring black hole masses inBarthearly-type galaxies with ALMA
NGC_2024_a_06_TM1 The Initial Conditions of Planet
Mann
Formation in the Youngest Rich
Cluster
NGC1808_a_06_TP
Starburst-driven superwind in the
Salaknearby galaxy NGC 1808 traced by CI

EA

Total Power6

03:24:09

04:55:29

2017.1.00474.S

TUKH122_a_06_7M

EA

7-m

6

02:02:58

02:28:41

2017.A.00018.S

gm_aur_e_03_TM1

NA

12-m

3

01:52:44

03:24:01

2017.1.00474.S

TUKH122_a_06_7M

EA

7-m

6

00:52:26

02:03:29

2017.1.00886.L

IC1954_a_06_TP

EU NA

Total Power

600:01:04

01:32:37

2017.1.00474.S

TUKH122_a_06_7M

Multiple star formation of a starless Ohashicore in the Orion A cloud
Studying the effects of variable UV
Espaillat
heating on the outer disk
Multiple star formation of a starless Ohashicore in the Orion A cloud
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Multiple star formation of a starless Ohashicore in the Orion A cloud

EA

7-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:59:22

01:08:04

2017.1.01659.S

EIS_J033_a_04_TM1

Resolved distribution and dynamics of Cheminmolecular gas of a

CL

12-m

4

2018-01-14
PIdistant spiral galaxy
23:40:55

00:52:172017.1.00886.L

IC1954_a_06_TP

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Resolved distribution and dynamics of Cheminmolecular gas of a distant spiralgalaxyRevealing the roles of filamentary
Muraoka
clouds in GMC evolution of M33

EU NA

Total Power

6

22:48:35

23:59:15

2017.1.01659.S

EIS_J033_a_04_TM1

CL

12-m

4

22:29:16

00:00:53

2017.1.00461.S

GMC-8_a_06_7M

EA

7-m

6

21:40:50

22:48:26

2017.1.01163.S

ALESS_06_a_03_TM1

ALESS CO: A CO survey ofspectroscopically-confirmed, ALMAidentified SMGs
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Wardlow

EU

12-m

3

17:23:41

18:47:11

2017.1.01355.L

W43-MM1_a_03_7M

Motte

CL EA EU NA

7-m

3

16:53:26

20:05:17

2016.1.01346.S

AGAL010._a_06_TP

Galactic Census of All Massive
Starless Cores within 5 kpc
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

PillaiEU

Total Power

6

15:58:14

16:37:09

2017.1.01355.L

W51-E_a_03_TPMotte

CL EA EU NA

Total Power

3

15:53:45

16:37:40

2017.1.01355.L

W43-MM3_a_03_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

7-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

14:51:45

16:13:24

2017.1.01355.L

W43-MM1_a_03_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

7-m

3

13:22:06

14:50:25

2017.1.01355.L

G351.77_a_03_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power

3

13:20:03

14:51:38

2017.1.00661.S

NGC6334I_a_04_7M

NA

7-m

4

11:43:08

13:07:55

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

10:17:21

11:42:50

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

08:52:43

10:16:59

2017.1.00815.S

NGC_4321_a_03_7M

NA

7-m

3

07:50:02

08:41:27

2017.1.00373.S

ID200101_a_03_TM1

Testing predictions of stellar cluster Brogan
formation in NGC6334I
Mapping Molecular ISM in the Whole Koda
Disk of M83
Mapping Molecular ISM in the Whole Koda
Disk of M83
A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Molecular gas and dust in theJinreionization epoch: massive
vigorously star forming galaxies at
z~7

EU

12-m

3

07:21:34

08:52:16

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

06:49:26

07:49:45

2017.1.00373.S

ID200101_c_03_TM1

Mapping Molecular ISM in the Whole Koda
Disk of M83
Molecular gas and dust in theJinreionization epoch: massive
vigorously star forming galaxies at
z~7

EU

12-m

3

05:48:15

07:21:09

2017.1.00379.S

ngc_3256_a_06_7M

EA

7-m

6

04:16:11

05:25:11

2017.1.01099.S

cosclust_a_03_TM1

Physical properties of dense gas in an Harada
AGN-driven outflow
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

03:06:40

04:15:54

2017.1.00270.S

ALPS.3_4_a_03_TM1

EU

12-m

3

03:04:16

04:11:172017.1.00474.S

EA

7-m

6

01:57:15

03:06:30

2017.1.00248.S

EA

12-m

3

01:10:39

01:36:31

2017.A.00018.S

NA

12-m

3

00:15:33

01:10:27

2017.1.00629.S

Dust vs. CO: Do both trace molecular Waltergas emission in high-redshift
galaxies?
TUKH122_a_06_7M
Multiple star formation of a starless Ohashicore in the Orion A cloudNGC1300__a_03_TM1 MOLECULAR CLOUDS AND STAR Maeda
FORMATION IN BAR OF NGC1300
gm_aur_c_03_TM1
Studying the effects of variable UV
Espaillat
heating on the outer disk
A496_a_03_TM1
Constraining the cold accretion onto Edge
the most massive Black Holes

EU

12-m

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

10:33:18

11:52:39

2017.1.00815.S

NGC_4321_a_03_7M

NA

7-m

3

10:30:38

11:41:32

2017.1.01232.S

Cloverle_b_03_TM1

A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar

EA

12-m

3

2018-01-13

2018-01-12
PI10:25:50

11:39:13

2017.1.00815.S

NGC_4321_a_03_TP

09:17:14

10:30:26

2017.1.01232.S

Cloverle_b_03_TM1

09:12:50

10:25:41

2017.1.00815.S

NGC_4321_a_03_TP

09:09:29

10:33:11

2017.1.00815.S

NGC_4321_a_03_7M

08:24:56

09:17:04

2017.1.01214.S

PJ113921_a_03_TM1

07:48:45

09:01:59

2017.1.00815.S

NGC_4321_a_03_TP

07:21:34

08:13:39

2017.1.01214.S

PJ113921_a_03_TM1

07:14:00

08:37:38

2017.1.00815.S

NGC_4321_a_03_7M

06:35:07

07:48:38

2017.1.00815.S

NGC_4321_a_03_TP

06:16:51

07:21:26

2017.1.00280.S

SN2015bn_a_03_TM1

05:25:33

06:33:00

2017.1.00271.S

Ridge_ce_b_03_TP

05:17:05

06:16:33

2017.1.00373.S

04:17:57

05:25:26

04:16:02

A Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
Spectral line survey in the rest-frame
350 GHz band toward the Cloverleaf
quasarA Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
A Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
ALMA Study of the Hyperluminous
SMGs Identified from Planck All-Sky
SurveyA Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
ALMA Study of the Hyperluminous
SMGs Identified from Planck All-Sky
SurveyA Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
A Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
A Direct Test of the Possible
Connection Between Fast Radio
Bursts and Superluminous
Supernovae

Gallagher

NA

Total Power

3

Nishimura

EA

12-m

3

Gallagher

NA

Total Power

3

Gallagher

NA

7-m

3

Yun

NA

12-m

3

Gallagher

NA

Total Power

3

Yun

NA

12-m

3

Gallagher

NA

7-m

3

Gallagher

NA

Total Power

3

Berger

NA

12-m

3

Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

ID200101_b_03_TM1

Molecular gas and dust in thereionization epoch: massive
vigorously star forming galaxies at
z~7

EU

12-m

3

2017.1.00271.S

Ridge_ce_b_03_TP

Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

305:15:59

2017.1.00373.S

ID200101_b_03_TM1

Molecular gas and dust in thereionization epoch: massive
vigorously star forming galaxies at
z~7

EU

12-m

3

04:04:55

05:36:01

2017.1.00474.S

TUKH122_a_06_7M

EA

7-m

6

03:10:18

04:17:49

2017.1.00271.S

Ridge_ce_b_03_TP

Multiple star formation of a starless Ohashicore in the Orion A cloud
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power3

03:05:04

04:14:19

2017.1.00270.S

ALPS.3_4_a_03_TM1

EU

12-m

3

01:50:21

02:59:35

2017.1.00270.S

ALPS.3_4_a_03_TM1

EU

12-m

3

01:26:13

02:00:58

2017.1.00271.S

Ridge_ce_b_03_TP

Dust vs. CO: Do both trace molecular Waltergas emission in high-redshift
galaxies?
Dust vs. CO: Do both trace molecular Waltergas emission in high-redshift
galaxies?
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power3

01:05:29

01:31:31

2017.A.00018.S

gm_aur_b_03_TM1

Espaillat

NA

12-m

3

00:23:10

01:05:04

2017.1.00629.S

Edge

EU

12-m

3

00:17:01

01:24:14

2017.1.00271.S

Ridge_ce_b_03_TP

Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:43:33

00:22:54

2017.1.00629.S

A3112_a_03_TM1

Constraining the cold accretion onto
the most massive Black Holes

Edge

EU

12-m

3

19:58:32

21:18:35

2015.1.01296.S

NGC346-r_a_03_7M

EA

7-m

3

19:57:57

20:51:35

2017.1.00629.S

A2390_a_03_TM1

Collisional star-formation in the SMC: Muller
NGC346
Constraining the cold accretion onto Edge
the most massive Black Holes

EU

12-m

3

14:36:55

16:04:34

2017.1.01355.L

G351.77_a_03_TP

ALMA-IMF: ALMA transforms our

CL EA EU NA

Total Power

3

Studying the effects of variable UV
heating on the outer disk
MACSJ024_a_03_TM1 Constraining the cold accretion onto
the most massive Black Holes

Jin

Jin

2018-01-11

Motteview of the origin of stellar masses
14:32:17

15:19:58

2017.1.01306.S

13:43:25

14:22:14

13:04:33

IRAS1720_a_03_TM1

EU

12-m

3

2017.1.00280.S

Tracing the Enrichment of the ISM in Sliwa
Extreme Starbursts
SN2010md_a_03_TM1 A Direct Test of the Possible
BergerConnection Between Fast Radio
Bursts and Superluminous
Supernovae

NA

12-m

3

14:36:48

2017.1.01355.L

G327.29_a_03_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

CL EA EU NA

Total Power

3

12:56:11

14:20:18

2017.1.01406.S

RX_J1713_b_03_7M

A Quest for Cosmic Ray Acceleration Sano
Site: Unveiling the Shock-Cloud
Interaction toward the Young SNR RX
J1713.7-3946

EA

7-m

3

12:36:48

13:43:11

2017.1.01232.S

Cloverle_a_03_TM1

EA

12-m

3

11:31:57

12:55:55

2017.1.01406.S

RX_J1713_c_03_7M

Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar
A Quest for Cosmic Ray Acceleration Sano
Site: Unveiling the Shock-Cloud
Interaction toward the Young SNR RX
J1713.7-3946

EA

7-m

3

11:23:15

12:30:19

2017.1.01232.S

Cloverle_a_03_TM1

EA

12-m

3

11:21:12

12:53:59

2017.1.01355.L

G327.29_a_03_TP

Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

Total Power3

10:02:42

11:08:58

2017.1.01232.S

Cloverle_a_03_TM1

EA

12-m

3

10:02:15

11:20:03

2017.1.00886.L

NGC4207_a_06_TP

EU NA

Total Power

6

09:55:36

11:20:39

2017.1.00886.L

NGC4654_a_06_7M

EU NA

7-m

6

08:53:43

10:02:36

2017.1.01232.S

Cloverle_a_03_TM1

EA

12-m

3

08:44:00

10:02:06

2017.1.00886.L

NGC4207_a_06_TP

EU NA

Total Power6

08:30:16

09:55:26

2017.1.00886.L

NGC4654_a_06_7M

EU NA

7-m

6

07:47:50

08:52:57

2017.1.01214.S

PJ113805_a_03_TM1

NA

12-m

3

07:36:10

08:43:44

2017.1.00886.L

NGC2566_a_06_TP

EU NA

Total Power6

06:49:52

08:22:43

2017.1.00379.S

ngc_3256_a_06_7M

EA

7-m

6

06:45:47

07:47:39

2017.1.01081.S

RXJ0911_a_04_TM1

NA

12-m

4

06:22:05

07:35:54

2017.1.00886.L

NGC2903_a_06_TP

EU NA

Total Power

605:43:49

06:45:39

2017.1.01081.S

RXJ0911_a_04_TM1

NA

12-m

4

05:18:43

06:49:44

2017.1.00474.S

TUKH122_a_06_7M

EA

7-m

6

05:13:09

06:21:57

2017.1.00886.L

NGC2997_a_06_TP

EU NA

Total Power

6

04:41:55

05:43:42

2017.1.01081.S

RXJ0911_a_04_TM1

NA

12-m

4

04:15:55

04:41:45

2017.A.00018.S

gm_aur_a_03_TM1

NA

12-m

3

03:57:28

05:18:25

2017.1.01353.S

OMC-2_Re_b_06_7M

EA

7-m

6

03:45:03

05:12:56

2017.1.00984.S

NGC1808_a_06_TP

Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
ALMA Study of the Hyperluminous
Yun
SMGs Identified from Planck All-Sky
Survey100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Physical properties of dense gas in an Harada
AGN-driven outflow
Probing the Molecular Gas Dynamics Leungof High-z Quasar Hosts on Sub-kpc
Scales100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Probing the Molecular Gas Dynamics Leungof High-z Quasar Hosts on Sub-kpc
ScalesMultiple star formation of a starless Ohashicore in the Orion A cloud
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Probing the Molecular Gas Dynamics Leungof High-z Quasar Hosts on Sub-kpc
ScalesStudying the effects of variable UV
Espaillat
heating on the outer disk
Fragmentation in the Orion Integral Takahashi
Shaped Filament
Starburst-driven superwind in the
Salaknearby galaxy NGC 1808 traced by CI

EA

Total Power6

03:26:06

04:03:15

2017.1.00629.S

RXCJ0439_a_03_TM1

Constraining the cold accretion

EU

12-m

3

Motte

Edge

onto the most massive Black Holes
02:29:18

03:08:08

2017.1.00015.S

FUOri_a_06_TM1

What's inside the enormous cavities
of FUOr outflows?
Multiple star formation of a starlesscore in the Orion A cloud
Are Close Binaries Formed ThroughDisk Fragmentation?
Why is ~ 1/4 of the LMC's molecular
gas not forming massive stars?

Williams

NA

12-m

6

02:25:58

03:57:19

2017.1.00474.S

TUKH122_a_06_7M

OhashiEA

7-m

601:18:05

02:27:44

2017.1.00053.S

Per12_NG_a_06_TM1

Tobin

EU

12-m

6

00:58:26

02:05:52

2017.1.00271.S

Ridge_ce_b_03_TP

Indebetouw

NA

Total Power

300:34:31

02:06:06

2017.1.00474.S

TUKH122_a_06_7M

Multiple star formation of a starlesscore in the Orion A cloud

OhashiEA

7-m

6Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:51:30

01:00:32

2017.1.00270.S

ALPS.2_a_03_TM1

EU

12-m

3

23:50:30

00:58:19

2017.1.00271.S

Ridge_ce_b_03_TP

Dust vs. CO: Do both trace molecular Waltergas emission in high-redshift
galaxies?
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

22:29:27

23:49:12

2015.1.01296.S

NGC346-r_a_03_7M

EA

7-m

3

14:05:45

14:32:18

2017.1.00441.S

W1814+34_a_04_TM1

OTHER

12-m

4

13:34:56

14:59:37

2017.1.00079.S

M83_e_03_7M

NA

7-m

3

13:13:24

14:05:38

2017.1.01214.S

PJ144958_a_03_TM1

NA

12-m

3

12:42:04

13:13:15

2017.1.01355.L

G328.25_a_03_TM1

Collisional star-formation in the SMC: Muller
NGC346
Exploring gas-rich major mergers in Fan
WISE-selected, hot dust-obscured
galaxies
Mapping Molecular ISM in the Whole Koda
Disk of M83
ALMA Study of the Hyperluminous
Yun
SMGs Identified from Planck All-Sky
SurveyALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

12-m

3

12:10:08

13:34:44

2017.1.00079.S

M83_d_03_7M

NA

7-m

3

11:50:03

12:41:50

2017.1.01390.S

EA

12-m

3

10:29:38

11:31:36

2017.A.00021.T

Mapping Molecular ISM in the Whole Koda
Disk of M83
OphA_N6_b_03_TM1
Testing Ambipolar Diffusion Models Lai
Down to 100 AU scale
GRB17120_a_03_TM1 Radio Polarlimetry of GRB Afterglows Urata

EA

12-m

3

10:15:00

11:59:43

2017.A.00021.T

GRB17120_a_07_7M

Radio Polarlimetry of GRB Afterglows Urata

EA

7-m

7

09:33:14

10:29:30

2017.A.00021.T

GRB17120_a_03_TM1 Radio Polarlimetry of GRB Afterglows Urata

EA

12-m

3

08:34:24

10:14:52

2017.A.00021.T

GRB17120_a_07_7M

Radio Polarlimetry of GRB Afterglows Urata

EA

7-m

7

08:17:29

09:33:06

2017.A.00021.T

GRB17120_a_03_TM1 Radio Polarlimetry of GRB Afterglows Urata

EA

12-m

3

07:41:58

08:55:15

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power3

07:08:25

08:17:20

2017.1.01099.S

cosclust_a_03_TM1

A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

06:53:41

08:16:50

2017.1.00297.S

PG1119+1_a_06_7M

CL

7-m

6

06:28:03

07:41:50

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power

3

05:59:29

07:08:16

2017.1.01099.S

cosclust_a_03_TM1

An ALMA-ACA Survey of CO(2-1) in Bauer
PG QSOsA Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

05:25:36

06:53:30

2017.1.01644.S

GJ_273_a_06_7M

EU

7-m

6

05:20:09

06:27:45

2017.1.00271.S

Ridge_ce_b_03_TP

Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

04:50:16

05:59:20

2017.1.01099.S

cosclust_a_03_TM1

Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

04:04:40

05:18:59

2017.1.01363.S

30_Dor_C_b_03_TP

Revealing the Shock-interacting
YamaneMolecular Gas toward the Magellanic
Superbubble 30

EA

Total Power

3

2018-01-10

Doradus C
04:04:06

05:25:29

2017.1.01353.S

03:35:11

04:45:06

2017.1.01102.S

02:56:56

04:04:33

2017.1.00271.S

02:42:02

04:03:54

02:17:29

OMC-2_Re_b_06_7M

Fragmentation in the Orion Integral Takahashi
Shaped Filament
NGC_2024_a_06_TM1 The Initial Conditions of Planet
Mann
Formation in the Youngest Rich
Cluster
Ridge_ce_b_03_TP
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

EA

7-m

6

NA

12-m

6

NA

Total Power3

2017.1.01353.S

OMC-1_Re_e_06_7M

EA

7-m

6

03:28:34

2017.1.01659.S

EIS_J033_a_04_TM1

CL

12-m

4

01:49:12

02:56:27

2017.1.00271.S

Ridge_ce_b_03_TP

NA

Total Power3

01:16:21

02:17:15

2017.1.01010.S

SMMJ0443_a_03_TM1 Spatially Resolved Gas-Star
Hung
Formation-Dynamics in z~2.5 SMGs

NA

12-m

3

01:15:21

02:41:51

2017.1.00093.S

YSO01_a_03_7M

Evolution of molecular clouds
Onishiassociated with O-type YSOs in giant
molecular clouds in the LMC

EA

7-m

3

00:31:36

00:55:44

2017.1.00441.S

W0248+27_a_04_TM1

OTHER

12-m

4

00:14:16

01:29:18

2017.1.01363.S

30_Dor_C_b_03_TP

Exploring gas-rich major mergers in Fan
WISE-selected, hot dust-obscured
galaxies
Revealing the Shock-interacting
YamaneMolecular Gas toward the Magellanic
Superbubble 30 Doradus C

EA

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:19:30

00:30:49

2017.1.00270.S

ALPS.2_a_03_TM1

EU

12-m

3

22:59:08

00:14:07

2017.1.01363.S

30_Dor_C_b_03_TP

Dust vs. CO: Do both trace molecular Waltergas emission in high-redshift
galaxies?
Revealing the Shock-interacting
YamaneMolecular Gas toward the Magellanic
Superbubble 30 Doradus C

EA

Total Power

3

22:56:19

00:27:03

2017.1.00093.S

YSO01_a_03_7M

Evolution of molecular clouds
Onishiassociated with O-type YSOs in giant
molecular clouds in the LMC

EA

7-m

3

21:05:06

22:37:25

2017.1.00931.S

B1-2_SE_a_06_7M

From Beginning to End -- Star
Formation and Molecular Cloud
Evolution in the Small Magellanic
Cloud

Johnson

NA

7-m

6

19:04:13

20:28:48

2017.1.00108.S

R_CrA_IR_a_06_7M

Drozdovskaya

EU

7-m

6

19:03:25

20:17:24

2017.1.01355.L

W51-IRS2_a_03_TP

In Search of Cometary H2S in LowMass Protostars
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power

3

17:44:09

19:03:01

2017.1.00040.S

cnd_cs32_b_04_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power

4

17:44:08

19:03:56

2017.1.01355.L

G008.67_a_06_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

7-m

6

16:36:46

17:01:14

2017.1.01235.S

IRAS1954_a_03_TM2

High Resolution Survey of the Gas
and Dust Distribution in Nearby
Luminous Infrared Galaxies

Barcos-Munoz

NA

12-m

3

16:11:12

17:30:03

2017.1.00040.S

cnd_cs32_b_04_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power

4

16:10:32

17:29:57

2017.1.01355.L

W43-MM1_a_03_7M

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

7-m

3

15:45:11

16:36:34

2017.1.01390.S

OphA_N6_b_03_TM1

Lai

EA

12-m

3

14:52:36

15:44:01

2017.1.01390.S

OphA_N6_b_03_TM1

Lai

EA

12-m

3

14:41:00

16:10:24

2017.1.01355.L

G333.60_a_06_7M

Testing Ambipolar Diffusion Models
Down to 100 AU scale
Testing Ambipolar Diffusion Models
Down to 100 AU scale
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

7-m

6

14:40:00

16:11:05

2017.1.01355.L

W51-E_a_03_TP

ALMA-IMF: ALMA transforms ourview of the origin of stellar

Motte

CL EA EU NA

Total Power

3

Fragmentation in the Orion Integral Takahashi
Shaped Filament
Resolved distribution and dynamics of Cheminmolecular gas of a distant spiralgalaxyWhy is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

2018-01-09
PImasses
13:30:35

14:43:02

2017.1.01355.L

G333.60_a_03_TM1

ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

12:23:49

13:30:14

2017.1.01232.S

Cloverle_a_03_TM1

12:22:58

13:38:55

2017.1.01355.L

G333.60_a_06_7M

11:16:49

12:23:35

2017.1.01232.S

Cloverle_a_03_TM1

10:53:37

12:22:43

2017.1.00886.L

NGC5248_b_06_7M

09:48:27

11:00:30

2017.1.00979.S

HD_10690_a_06_TM1

09:46:08

10:43:10

2017.1.01158.S

08:37:02

09:48:56

08:21:40

Motte

CL EA EU NA

12-m

3

Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

EA

12-m

3

CL EA EU NA

7-m

6Spectral line survey in the rest-frame Nishimura
350 GHz band toward the Cloverleaf
quasar100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Disk eccentricity and circumplanetary Hughes
dust in the HD 106906 system

EA

12-m

3

EU NA

7-m

6

NA

12-m

6

VV75_a_06_7M

ACA Study on the Driving
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

EA

7-m

6

2017.1.00886.L

NGC4293_a_06_TP

EU NA

Total Power6

09:45:14

2017.1.00815.S

NGC_4321_a_03_7M

NA

7-m

3

08:13:39

09:22:33

2017.1.01099.S

cosclust_a_03_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

07:27:44

08:36:51

2017.1.00886.L

NGC2997_a_06_TP

EU NA

Total Power6

07:04:34

08:13:20

2017.1.01099.S

cosclust_a_03_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

06:57:41

08:20:51

2017.1.01644.S

GJ_273_a_06_7M

EU

7-m

6

06:19:41

07:27:24

2017.1.00886.L

NGC2566_a_06_TP

EU NA

Total Power

605:55:28

07:04:13

2017.1.01099.S

cosclust_a_03_TM1

Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

05:05:55

06:14:27

2017.1.00886.L

NGC2997_a_06_TP

EU NA

Total Power

604:46:15

05:55:18

2017.1.01099.S

cosclust_a_03_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Witnessing the onset of environmental Wang
quenching in the most distant X-ray
cluster at z = 2.51

EA

12-m

3

04:17:05

04:38:10

2017.1.01658.S

MACSJ060_a_06_TM1 Complete Census of Bright Lensed Egami
Submillimeter Galaxies Discovered by
the Herschel Lensing Survey

NA

12-m

6

03:56:50

05:04:33

2017.1.00886.L

NGC2566_a_06_TP

EU NA

Total Power

6

03:05:09

04:36:37

2017.1.00474.S

EA

7-m

6

02:52:03

04:01:50

2017.1.01102.S

NA

12-m

6

01:35:05

02:46:04

2017.1.01659.S

CL

12-m

4

01:28:07

02:35:24

2017.1.00271.S

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
TUKH122_a_06_7M
Multiple star formation of a starless Ohashicore in the Orion A cloud
NGC_2024_a_06_TM1 The Initial Conditions of Planet
Mann
Formation in the Youngest Rich
Cluster
EIS_J033_a_04_TM1
Resolved distribution and dynamics of Cheminmolecular gas of a distant spiralgalaxyRidge_ce_b_03_TP
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power3

01:17:29

02:43:55

2017.1.00093.S

YSO01_a_03_7M

EA

7-m

3

Yamashita

Evolution of molecular clouds
Onishiassociated with O-type YSOs in giant
molecular clouds in the LMC

2018-01-08
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

22:12:30

23:00:19

2017.1.01163.S

ALESS_06_a_03_TM1

21:11:55

22:12:10

2017.1.01527.S

4c05.84_a_04_TM1

20:54:09

21:11:36

2017.1.01235.S

20:32:13

21:56:13

20:19:22

20:36:56

PI

Executive

Array

Band

ALESS CO: A CO survey ofWardlow
spectroscopically-confirmed, ALMAidentified SMGs
Searching for feedback with 3D multi- Vayner
phase interstellar medium study inz~2 quasar host galaxies

EU

12-m

3

NA

12-m

4

IIIZw035_a_03_TM2

High Resolution Survey of the Gas
and Dust Distribution in Nearby
Luminous Infrared Galaxies

Barcos-Munoz

NA

12-m

3

2017.1.01158.S

VV492_b_06_TP

ACA Study on the Driving
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

Yamashita

EA

Total Power6

2017.1.01235.S

CGCG436-_a_03_TM2 High Resolution Survey of the Gas
and Dust Distribution in Nearby
Luminous Infrared Galaxies

Barcos-Munoz

NA

12-m

3