ALMA Observing Activity from 2018-04-02T17:59:00 to 2018-04-09T18:00:00
QA0 pass executions
2018-04-09
Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

11:08:15

11:36:27

2017.1.00999.S

CK_Vul_a_04_TM2

10:49:45

12:20:38

2017.1.01355.L

W51-IRS2_a_03_TP

10:46:53

11:07:40

2017.1.00999.S

CK_Vul_b_04_TM2

10:44:59

12:03:36

2017.1.01116.S

G08.670-_a_06_7M

09:55:59

10:46:46

2016.1.00314.S

RCW120_b_06_TM1

09:15:07

10:39:18

2017.1.01355.L

G333.60_a_06_TP

09:01:18

10:34:56

2017.1.01355.L

08:13:47

09:14:03

08:00:32

PI

Executive

Array

Band

Complex molecules and rare isotopes Kaminski
in Nova 1670
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

NA

12-m

4

CL EA EU NA

Total Power

3

Complex molecules and rare isotopes Kaminski
in Nova 1670
High Resolution Imaging of Inflow & Shirley
Infall in Massive Star-forming Clumps

NA

12-m

4

NA

7-m

6

Dissecting to decipher: an ALMA
Bronfmanstudy of the high-mass star formation
processes in RCW 120
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL

12-m

6

CL EA EU NA

Total Power6

G010.62_a_06_7M

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

CL EA EU NA

7-m

6

2017.1.00107.S

J162138._a_04_TM1

Probing the Grain Growth Signatures Hirano
in rho-Ophiuchi Young Stellar Objects

NA

12-m

4

08:59:27

2017.1.00180.S

6334_-_M_a_06_7M

Define the physic of high-mass starformation from the cold Hershel
sources of the NGC6334 complex

LouvetCL

7-m

6

07:50:41

09:15:00

2017.1.01355.L

G333.60_a_06_TP

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

Motte

CL EA EU NA

Total Power

6

06:58:39

08:00:26

2017.1.00180.S

6334_-_M_a_06_7M

Define the physic of high-mass starformation from the cold Hershel
sources of the NGC6334 complex

LouvetCL

7-m

6

06:24:24

07:50:34

2017.1.01355.L

G333.60_a_06_TP

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

Motte

CL EA EU NA

Total Power

605:33:56

06:58:31

2017.1.00079.S

M83_e_03_7M

NA

7-m

3

05:20:42

06:06:28

2017.1.00510.S

UR56917_a_04_TM1

EU

12-m

4

05:11:14

06:24:16

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power

3

04:47:28

05:20:37

2017.1.01318.S

SDSS_J11_a_04_TM2

EU

12-m

4

04:26:37

04:47:21

2017.1.01687.S

MP_Mus_a_04_TM2

NA

12-m

4

04:10:49

05:33:48

2017.1.00297.S

PG1229+2_a_06_7M

CL

7-m

6

03:58:08

05:11:07

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power

3

03:38:56

04:26:31

2017.1.01318.S

SDSS_J12_a_04_TM2

EU

12-m

4

02:49:12

03:38:49

2017.1.01020.S

zC-40669_a_04_TM1

Mapping Molecular ISM in the Whole Koda
Disk of M83
The ISM of the most luminous
Oteo
starbursts in the early Universe
A Wide, Deep Dense Gas Map ofGallagher
M100 to Connect Extragalactic andGalactic Dense Gas Results
Resolving molecular gas in ultraGeachcompact starburst galaxies withextreme outflows
Characterizing the solar nebula
Ribasanalog MP Mus
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
Resolving molecular gas in ultraGeachcompact starburst galaxies withextreme outflows
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

02:46:09

04:10:42

2017.1.00079.S

M83_b_03_7M

NA

7-m

3

02:45:08

03:58:00

2017.1.00815.S

NGC_4321_a_03_TP

NA

Total Power3

01:44:19

02:49:04

2017.1.01020.S

zC-40669_a_04_TM1

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
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

01:32:21

02:45:00

2017.1.00815.S

NGC_4321_a_03_TP

Gallagher

NA

Total Power3

01:19:00

02:46:01

2017.1.00771.S

NGC4038_a_03_7M

A Wide, Deep Dense Gas Map ofM100 to Connect Extragalactic andGalactic Dense Gas Results
Adjusting the Reception of The

Sliwa

EU

7-m

3

Motte

01:25:11

2017.1.01020.S

zC-40669_a_04_TM1

Antennae: A Clear Look at GMCs in a
Major Merger
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

PI

Executive

Array

Band

23:47:07

01:10:53

2017.1.01158.S

12376546_b_06_TP

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

Yamashita

EA

Total Power

6

23:37:16

00:58:55

2017.1.00527.S

G09.v10._e_06_7M

The molecular gas and resolved star- Oteo
formation law in low-redshift SMGs

EU

7-m

6

23:12:52

00:19:11

2017.1.01020.S

zC-40056_a_04_TM1

Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

22:49:00

23:45:27

2017.1.00271.S

Ridge_NW_b_03_TP

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

NA

Total Power

3

22:12:29

23:37:09

2017.1.00823.S

Cloud_4_a_03_7M

How do GMCs start to form massive Ochsendorf
stars? An ALMA survey of young,massive star forming GMCs in the
LMC

NA

7-m

3

21:50:23

23:12:44

2017.1.01553.S

OMC-4_a_03_TM1

CL

12-m

3

21:41:17

22:38:07

2017.1.00271.S

Ridge_NW_b_03_TP

Interplay between the Orion A South Zhu(OMC-4) filament and dense cores
therein
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

20:46:59

21:40:02

2017.1.01100.S

SPT0348-_a_04_TM1

An Unprecedented Census of the
Molecular ISM in Starburst Galaxies
at the End of Cosmic Reionization

CL

12-m

4

20:44:34

21:41:10

2017.1.00271.S

Ridge_NW_b_03_TP

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

NA

Total Power

3

20:42:13

22:09:21

2017.1.00765.S

TMC1A_a_04_7M

EU

7-m

4

19:35:10

20:44:51

2017.1.01109.S

SDSS_J02_a_04_TM1

Large-scale infalling envelopes
Harsonothrough cold gas tracers
How universal are surprisingly
Bezansonsignificant molecular gas reservoirs inmassive post-starburst galaxies at
z~0.6?

NA

12-m

4

18:41:20

20:11:35

2017.1.01140.S

NGC_1316_a_06_7M

NA

7-m

6

17:47:12

19:02:25

2017.1.00161.L

ngc253_c_04_TM1

EA EU NA12-m

4

16:36:36

18:08:05

2017.1.00461.S

GMC-8_a_06_7M

Radio-Mode AGN Feedback on the Kenney
Molecular Gas in the Merger Remnant
Fornax A
ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
Revealing the roles of filamentary
Muraoka
clouds in GMC evolution of M33

EA

7-m

6

16:19:20

17:28:40

2017.1.00202.S

SMG_C_a_03_TM1

EU

12-m

3

15:41:46

15:52:122017.1.00009.S

Sun_10_a_03_TP

The extent of (by far) the mostOteo
extreme starbursts in the early
Universe
Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power3

15:31:15

15:41:40

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

15:20:44

15:31:08

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power3

15:06:15

15:16:42

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

14:55:43

15:06:08

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

14:45:07

14:55:36

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

14:39:01

15:50:172017.1.00009.S

Sun_10_a_03_INT

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

12-m

3

00:20:32

NA

12-m

4

2018-04-08

Aravena14:34:33

14:45:01

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

14:24:00

14:34:26

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

14:12:51

14:23:51

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power3

14:01:41

14:12:42

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

13:50:30

14:01:32

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

13:39:17

13:50:22

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

13:27:47

13:39:09

2017.1.00009.S

Sun_10_a_03_TP

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

Total Power

3

13:27:46

14:38:55

2017.1.00009.S

Sun_10_a_03_INT

Oscillations and waves contributing to Okamotocoronal heating on the Sun

EA

12-m

3

11:52:57

12:17:49

2017.1.00602.S

ALMAJ221_b_06_TM1

EA

12-m

6

11:41:15

12:55:16

2017.1.01355.L

G010.62_a_03_TP

Confimation of Blindly Detected
Hayatsu[CII]158um emitter candidates at z =6.0 and 6.5
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

Total Power

3

11:26:50

11:52:172017.1.00602.S

ALMAJ221_a_06_TM1

EA

12-m

6

11:23:37

12:13:34

2017.1.00595.S

AQ Sgr_a_07_7M

EU

7-m

7

10:09:55

11:41:08

2017.1.01355.L

W43-MM3_a_06_TP

Confimation of Blindly Detected
Hayatsu[CII]158um emitter candidates at z =6.0 and 6.5
DEATH STAR: DEtermining Accurate Ramstedt
mass-loss rates of THermally pulsing
AGB STARs
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

Total Power6

10:07:28

11:26:44

2017.1.00983.S

G18.89_a_06_TM1

Quantifying the Feedback Potential of Brogan
Young Massive Protoclusters

NA

12-m

6

09:53:16

10:50:22

2017.1.00180.S

6334_-_M_a_06_7M

Define the physic of high-mass starformation from the cold Hershel
sources of the NGC6334 complex

LouvetCL

7-m

6

09:44:55

10:06:29

2017.1.01205.S

Postman

NA

12-m

6

08:39:10

10:09:47

2017.1.01355.L

MACSJ193_a_06_TM1 The Role and Origin of Dust in a
Feedback-Induced BCG Starburst
W43-MM3_a_06_TP
ALMA-IMF: ALMA transforms ourview of the origin of stellar masses

Motte

CL EA EU NA

Total Power6

07:55:52

09:15:48

2017.1.00983.S

G18.89_a_06_TM1

Quantifying the Feedback Potential of Brogan
Young Massive Protoclusters

NA

12-m

6

07:23:08

08:56:31

2017.1.00716.S

G340.39_a_06_7M

A survey of prestellar, high-mass
clump candidates: constraining
models of high-mass star formation

EA

7-m

6

07:10:00

08:24:50

2017.1.00886.L

NGC5530_a_06_TP

EU NA

Total Power

606:48:54

07:55:45

2017.1.00180.S

6334_-_M_a_06_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Define the physic of high-mass star Louvet
formation from the cold Hershel
sources of the NGC6334 complex

CL

12-m

6

05:55:11

07:23:00

2017.1.00297.S

PG1310-1_a_06_7M

CL

7-m

6

05:54:22

07:09:52

2017.1.00886.L

EU NA

Total Power

605:23:50

06:48:46

2017.1.00090.S

EA

12-m

6

04:43:52

05:54:13

2017.1.00886.L

EU NA

Total Power

6

04:33:21

05:55:04

2017.1.00886.L

EU NA

7-m

6

Sanhueza

An ALMA-ACA Survey of CO(2-1) in Bauer
PG QSOs
NGC5530_a_06_TP
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
NGC_4374_a_06_TM1 Do the Accretion Environments of
Bower
Low Luminosity AGN Resemble thatof Sgr A*?
NGC4689_b_06_TP
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
NGC4826_a_06_7M
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution

04:18:42

05:23:42

2017.1.00090.S

NGC_4374_a_06_TM1 Do the Accretion Environments of
Bower
Low Luminosity AGN Resemble thatof Sgr A*?
NGC4689_b_06_TP
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
NGC4826_a_06_7M
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
NGC_4374_a_06_TM1 Do the Accretion Environments of
Bower
Low Luminosity AGN Resemble thatof Sgr A*?
PJ132217_a_06_TM1 ALMA Study of the Hyperluminous
Yun
SMGs Identified from Planck All-Sky
SurveySDSS_J12_a_06_TM1 Feedback and Star Formation in
HamannExtremely Red Quasars
SN_2015b_a_06_TM1 Searching for the Smoking Gun ofMuraseMagnetar-Powered Super-Luminous
Supernovae
GJ_273_a_06_7M
Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
12376546_b_06_TP
ACA Study on the Driving
Yamashita
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

EA

12-m

6

03:33:24

04:43:47

2017.1.00886.L

EU NA

Total Power6

03:11:33

04:33:14

2017.1.00886.L

EU NA

7-m

6

02:42:21

04:18:35

2017.1.00090.S

EA

12-m

6

02:16:31

02:37:07

2017.1.01214.S

NA

12-m

6

01:13:51

02:16:24

2017.1.00478.S

NA

12-m

6

00:47:20

01:13:44

2017.1.00975.S

NA

12-m

6

00:47:15

02:13:34

2017.1.01644.S

EU

7-m

6

00:15:45

01:43:49

2017.1.01158.S

EA

Total Power

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:08:42

00:09:26

2017.1.00271.S

Ridge_NW_b_03_TP

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

NA

Total Power

3

23:04:32

00:14:35

2017.1.00478.S

SDSS_J08_b_06_TM1

NA

12-m

6

22:46:39

00:19:13

2017.1.01644.S

EU

7-m

6

21:58:18

23:02:09

2017.1.00704.S

EU

12-m

6

14:55:36

15:43:07

2017.1.01387.S

EU

12-m

6

14:49:42

15:43:48

2017.1.00595.S

EU

7-m

7

14:23:56

15:47:172017.1.01158.S

Feedback and Star Formation in
HamannExtremely Red Quasars
GJ_273_a_06_7M
Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
HD_69830_a_06_TM1 Getting the composition of exocomets Kral
with ALMAXDCP_B6__a_06_TM1 Understanding the nature of the
Stach
ULIRG population in massive clusters
at z ~ 1-1.5
AFGL_306_a_07_7M
DEATH STAR: DEtermining Accurate Ramstedt
mass-loss rates of THermally pulsing
AGB STARs
VV642_a_06_TP
ACA Study on the Driving
Yamashita
Mechanisms of Starburst and MainSequence Star Formation in Local
Galaxies

EA

Total Power

6

13:44:31

14:54:40

2017.1.00496.S

EU

12-m

6

12:59:44

13:44:24

2017.1.01387.S

EU

12-m

6

12:45:49

14:39:53

2017.1.00828.S

CL

7-m

7

12:37:03

14:14:01

2017.1.00716.S

JW100_CO_a_06_TM1 Mapping the molecular gas in jellyfish poggianti
galaxies
XDCP_B6__a_06_TM1 Understanding the nature of the
Stach
ULIRG population in massive clusters
at z ~ 1-1.5
HD206893_a_07_7M
The reddened pale dot. Is a disk the Zurlo
responsible of the red colour ofHD206893B?
G016.97_a_06_TP
A survey of prestellar, high-mass
Sanhuezaclump candidates: constraining
models of high-mass star formation

EA

Total Power

6

11:33:01

12:28:45

2017.1.00040.S

cnd_cs43_d_05_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power5

11:09:52

12:42:54

2017.1.00040.S

cnd_cs76_b_07_TM1

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

12-m

7

10:17:59

12:10:51

2017.1.00377.S

G08.68-0_a_07_7M

EU

7-m

7

09:18:39

10:31:14

2017.1.00019.S

Lupus_3__a_06_TP

NA

Total Power6

09:17:32

10:54:37

2017.1.00040.S

cnd_cs76_c_07_TM1

Exploring the mid-IR SED of highLeurini
mass YSOs
Outflow structure of the young
Plunkett
protostar Lupus 3 MMS
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

12-m

7

08:50:18

09:17:24

2017.1.00232.S

M3-28_24_a_06_TM1

The Surprising Molecular Content of Schmidt
Planetary Nebulae: A Closer Look at
Chemistry, Dynamics, Structure andEvolution

NA

12-m

6

2018-04-07PI08:21:08

08:50:11

2017.1.00180.S

6334_-_M_b_06_TM1

Define the physic of high-mass starformation from the cold Hershel
sources of the NGC6334 complex

Louvet

CL

12-m

6

08:12:38

09:46:19

2017.1.00716.S

G340.39_a_06_7M

A survey of prestellar, high-mass
clump candidates: constraining
models of high-mass star formation

Sanhueza

EA

7-m

6

07:32:34

08:25:01

2017.1.00886.L

NGC4689_b_06_TP

EU NA

Total Power

6

06:59:56

08:21:00

2017.1.00377.S

G08.68-0_a_07_TM1

EU

12-m

7

05:56:17

07:32:26

2017.1.01355.L

G337.92_a_06_TP

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Exploring the mid-IR SED of highLeurini
mass YSOs
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

CL EA EU NA

Total Power

605:50:13

06:58:43

2017.1.00478.S

SDSS_J13_c_06_TM1

NA

12-m

6

05:42:24

07:19:51

2017.1.00040.S

cnd_cs76_c_07_7M

Feedback and Star Formation in
HamannExtremely Red Quasars
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

7-m

7

04:40:31

05:56:10

2017.1.00886.L

NGC5530_a_06_TP

EU NA

Total Power

604:20:35

05:42:172017.1.00886.L

NGC4826_a_06_7M

EU NA

7-m

6

03:30:03

04:40:24

2017.1.00886.L

NGC4689_b_06_TP

EU NA

Total Power6

03:19:59

04:44:41

2017.1.01259.S

UDst1_pK_a_07_TM1

EA

12-m

7

02:58:42

04:20:27

2017.1.00886.L

NGC4826_a_06_7M

EU NA

7-m

6

02:17:58

03:29:54

2017.1.00886.L

NGC4689_b_06_TP

EU NA

Total Power

6

01:57:50

03:19:52

2017.1.00326.S

cl01_a_07_TM1

EA

12-m

7

00:44:48

02:39:27

2017.1.00379.S

ngc_3256_a_07_7M

EA

7-m

7

00:38:49

01:58:56

2017.1.01003.S

AM_1158-_b_03_TP

NA

Total Power

300:36:13

01:57:39

2017.1.00326.S

cl01_a_07_TM1

100,000 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
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Identifying z~6 passive galaxies: relicsMawatariof first galaxies at z~20
100,000 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 Follow-up Survey for Clumpy Murata
Galaxies at z~0.9 in the COSMOS
Field
Physical properties of dense gas in an Harada
AGN-driven outflow
Recovering Extended Structures in
Ueda
Merger Remnants
ALMA Follow-up Survey for Clumpy Murata
Galaxies at z~0.9 in the COSMOS
Field

EA

12-m

7

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:30:09

00:26:53

2017.1.00271.S

Ridge_NW_b_03_TP

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

NA

Total Power

3

23:09:48

00:15:28

2017.1.00704.S

HD_69830_a_06_TM1

EU

12-m

6

22:53:33

00:42:40

2017.1.01280.S

Orion_Ba_a_07_7M

EU

7-m

7

22:33:07

23:30:02

2017.1.00271.S

Ridge_NW_b_03_TP

Getting the composition of exocomets Kral
with ALMA
The complete ALMA view of the Orion Goicoechea
Bar: unexpected structures andprocesses
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

20:55:55

21:56:50

2017.1.00271.S

Ridge_NW_b_03_TP

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

NA

Total Power

3

20:54:09

22:17:00

2017.1.01053.S

HH_212_c_07_7M

NA

7-m

7

11:16:24

11:59:03

2017.1.01583.S

SMORES: Shocked Molecular
McGuireOutflows across a Range ofEnvironments Survey
2MASS_J2_a_07_TM1 The frontier of rocky planet formation: Kennedy
are low-mass stars super-efficient?

EU

12-m

7

10:45:36

12:04:09

2017.1.00040.S

cnd_cs76_g_07_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power

7

10:16:45

12:05:172017.1.00377.S

G08.68-0_a_07_7M

Leurini

EU

7-m

7

09:54:41

11:16:172017.1.00377.S

G08.68-0_a_07_TM1

Leurini

EU

12-m

7

09:14:13

10:45:28

2017.1.01355.L

W43-MM3_a_06_TP

Exploring the mid-IR SED of highmass YSOs
Exploring the mid-IR SED of highmass YSOs
ALMA-IMF: ALMA transforms ourMotte

CL EA EU NA

Total Power

6

2018-04-06
PIview of the origin of stellar masses
08:58:35

09:39:27

2017.1.01583.S

GSC_0739_a_07_TM1 The frontier of rocky planet formation: Kennedy
are low-mass stars super-efficient?

EU

12-m

7

08:50:02

10:16:38

2017.1.01355.L

W43-MM2_a_06_7M

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

CL EA EU NA

7-m

6

06:57:14

08:20:122017.1.00040.S

cnd_cs76_g_07_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power

705:59:22

07:15:31

2017.1.01311.S

Enceladu_a_07_TM1

NA

12-m

7

04:40:10

05:40:50

2017.1.00478.S

SDSS_J13_a_06_TM1

NA

12-m

6

03:57:31

05:07:59

2017.1.00886.L

NGC4689_b_06_TP

EU NA

Total Power

6

03:36:51

05:05:09

2017.1.00297.S

PG1310-1_a_06_7M

CL

7-m

6

02:52:47

04:29:03

2017.1.00190.S

B14-6566_a_08_TM1

Remote Detection of Organics in
LoomisEnceladus' Plume
Feedback and Star Formation in
HamannExtremely Red Quasars
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
An ALMA-ACA Survey of CO(2-1) in Bauer
PG QSOs
Physics of the interstellar medium of Inouegalaxies in the reionization era: the[OIII]-to-[CII] line ratio II

EA

12-m

8

01:33:13

03:26:47

2017.1.00379.S

ngc_3256_a_07_7M

EA

7-m

7

01:00:04

02:18:25

2017.1.00326.S

cl01_a_07_TM1

Physical properties of dense gas in an Harada
AGN-driven outflow
ALMA Follow-up Survey for Clumpy Murata
Galaxies at z~0.9 in the COSMOS
Field

EA

12-m

7

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:53:19

01:11:30

2017.1.00527.S

G09.v10._b_06_7M

The molecular gas and resolved star- Oteo
formation law in low-redshift SMGs

EU

7-m

6

23:50:55

00:27:46

2017.1.00200.S

HD84870_a_06_TM1

REsolved ALMA Survey Of Nearby Matra
Stars (REASONS): a population studyof the formation location ofplanetesimal belts

NA

12-m

6

23:33:51

00:41:11

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

23:27:18

23:47:01

2017.1.01214.S

PJ084648_a_06_TM1

NA

12-m

6

22:35:01

23:31:45

2017.1.00271.S

Ridge_NW_b_03_TP

ALMA Study of the Hyperluminous
Yun
SMGs Identified from Planck All-Sky
SurveyWhy is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

22:27:33

23:26:57

2017.1.01559.S

Q0738+31_a_06_TM1

NA

12-m

6

21:32:13

22:28:58

2017.1.00271.S

Ridge_NW_b_03_TP

The Origin of z < 1 Damped Lyman- Bowenalpha Absorbers: Completing the
CensusWhy is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

21:26:24

22:48:45

2017.1.01053.S

HH_212_b_07_7M

NA

7-m

7

20:24:51

21:32:06

2017.1.00271.S

Ridge_ce_b_03_TP

SMORES: Shocked Molecular
McGuireOutflows across a Range ofEnvironments Survey
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

NA

Total Power

3

19:21:51

20:05:16

2017.1.00595.S

U_Men_a_06_7M

EU

7-m

6

19:11:12

19:27:19

2016.1.00209.S

L1551_IR_a_06_TM2

EA

12-m

6

18:38:34

20:00:15

2017.1.00129.S

FCC102_a_03_TP

DEATH STAR: DEtermining Accurate Ramstedt
mass-loss rates of THermally pulsing
AGB STARs
Multi-scale disk and envelope
Takamikinematics around the most extremely
accreting young stars
Deep CO(J=1-0) mapping survey of Morokuma
Fornax galaxies with Morita array

EA

Total Power

3

18:17:30

19:11:06

2017.1.00510.S

SGP38326_a_06_TM1

EU

12-m

6

17:20:04

17:49:30

2017.1.00508.S

J0217-02_a_06_TM1

EA

12-m

6

14:07:23

15:32:26

2017.1.00161.L

ngc253_p_07_7M

EA EU NA7-m

7

11:57:36

13:52:172017.1.00828.S

HD206893_a_07_7M

The ISM of the most luminous
Oteo
starbursts in the early Universe
Investigating ISM Physics at z~6 with Harikane
Multiple FIR Lines of NewlyDiscovered Luminous Galaxies
ALCHEMI: the ALMA Comprehensive Martin
High-resolution Extragalactic
Molecular Inventory
The reddened pale dot. Is a disk the Zurlo
responsible of the red colour

CL

7-m

7

Motte

2018-04-05
PIof HD206893B?
11:11:02

12:24:23

2017.A.00030.S

CK_Vul_a_05_TM1

First radioactive molecule observed in Kaminski
space: 26AlF in a stellar-merger
remnant
ALMA-IMF: ALMA transforms ourMotteview of the origin of stellar masses

NA

12-m

5

09:04:19

10:35:30

2017.1.01355.L

W43-MM3_a_06_TP

CL EA EU NA

Total Power6

08:59:53

10:53:25

2017.1.00717.S

NGC6334I_a_10_TM1

Astrochemical ABCs - An ALMA Band McGuire
9/10 Chemical Survey of NGC 6334I

NA

12-m

10

08:50:58

09:35:00

2016.1.00314.S

RCW120_b_07_7M

CL

7-m

7

08:50:51

2016.1.00314.S

RCW120_a_07_7M

CL

7-m

7

07:13:56

08:31:28

2017.1.00377.S

G337.92-_a_07_TM1

EU

12-m

7

07:09:22

08:37:38

2017.1.00040.S

cnd_cs76_e_07_TP

Dissecting to decipher: an ALMA
Bronfmanstudy of the high-mass star formation
processes in RCW 120
Dissecting to decipher: an ALMA
Bronfmanstudy of the high-mass star formation
processes in RCW 120
Exploring the mid-IR SED of highLeurini
mass YSOs
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

08:05:24

EA

Total Power

705:48:46

06:22:30

2017.1.00040.S

cnd_cs76_e_07_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power

705:40:24

07:11:01

2017.1.00775.S

A1689-zD_a_08_TM1

Mapping all phases of the ISM in anormal reionisation-epoch galaxy

EU

12-m

8

04:17:41

05:40:18

2017.1.00753.S

NGC5253_a_08_TM1

EU

12-m

8

03:56:53

05:18:32

2017.1.00886.L

EU NA

7-m

6

03:23:49

03:46:02

2017.1.01276.S

EA

12-m

7

02:28:57

03:56:46

2017.1.00297.S

CL

7-m

6

02:05:40

03:20:14

2017.1.00326.S

EA

12-m

7

01:44:59

02:55:122017.1.00886.L

EU NA

Total Power6

01:19:39

02:09:53

2017.1.01572.S

NA

7-m

6

00:34:08

01:43:47

2017.1.01618.S

EA

12-m

6

00:05:03

01:25:20

2017.1.01003.S

Revisiting the star formation efficiency De Looze
of low-metallicity starburst galaxy
NGC5253
NGC4826_a_06_7M
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
COSMOS-H_g_07_TM1 Unveiling the nature of the most HST- Wang
dark galaxies at z > 4
PG1310-1_a_06_7M
An ALMA-ACA Survey of CO(2-1) in Bauer
PG QSOs
cl01_a_07_TM1
ALMA Follow-up Survey for Clumpy Murata
Galaxies at z~0.9 in the COSMOS
Field
NGC4689_b_06_TP
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
4C20.24_a_06_7M
ALMA Observations of Resolved
Meyer
Extragalactic Jets in a Critically
Unsampled Spectral Window
4.12027_a_06_TM1
Do there exist mini-SMGs at cosmic Kusakabenoon?
AM_1158-_b_03_TP
Recovering Extended Structures in
Ueda
Merger RemnantsNA

Total Power

3

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:51:33

01:18:48

2017.1.01644.S

GJ_273_a_06_7M

EU

7-m

6

22:53:38

00:11:33

2017.1.01020.S

zC-40056_a_04_TM1

Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
Deep [CI] 1-0 observations in the
Bisbashigh-redshift Universe: studying the
distribution of Dark Matter in galaxies

NA

12-m

4

22:15:51

23:48:31

2017.1.01644.S

GJ_273_a_06_7M

EU

7-m

6

21:55:15

22:51:51

2017.1.00286.S

GW_Ori_a_06_TM2

EA

12-m

6

20:23:14

21:12:30

2017.1.00595.S

R_Dor_a_07_7M

EU

7-m

7

20:15:34

21:28:07

2017.1.01109.S

SDSS_J02_a_04_TM1

Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
Search for Possible Disk-scale
Muto
Asymmetric Structures inProtoplanetary Disks
DEATH STAR: DEtermining Accurate Ramstedt
mass-loss rates of THermally pulsing
AGB STARs
How universal are surprisingly
Bezansonsignificant molecular gas reservoirs inmassive post-starburst galaxies at
z~0.6?

NA

12-m

4

19:09:28

20:07:58

2017.1.01512.S

ALESS001_d_03_TM1

Weiss

EU

12-m

3

16:38:18

16:48:38

2016.1.00298.S

Sun_10_a_03_TP

Leenaarts

EU

Total Power

3

16:27:56

16:38:15

2016.1.00298.S

Sun_10_a_03_TP

Gas mass fractions in z>3 main
sequence galaxies from ALESS
Constraining the temperature andheating mechanisms in the solar
plage chromosphere
Constraining the temperature

Leenaarts

EU

Total Power

3

Watson2018-04-04
PI16:17:29

16:27:49

2016.1.00298.S

Sun_10_a_03_TP

16:07:00

16:17:21

2016.1.00298.S

Sun_10_a_03_TP

15:56:28

16:06:53

2016.1.00298.S

Sun_10_a_03_TP

15:45:59

15:56:22

2016.1.00298.S

Sun_10_a_03_TP

15:35:25

15:45:49

2016.1.00298.S

Sun_10_a_03_TP

15:24:53

15:35:16

2016.1.00298.S

Sun_10_a_03_TP

15:14:00

15:24:46

2016.1.00298.S

Sun_10_a_03_TP

14:58:53

15:13:53

2016.1.00298.S

Sun_10_a_06_TP

14:43:44

14:58:44

2016.1.00298.S

Sun_10_a_06_TP

14:28:43

14:43:37

2016.1.00298.S

Sun_10_a_06_TP

14:13:38

14:28:36

2016.1.00298.S

Sun_10_a_06_TP

13:57:53

14:13:32

2016.1.00298.S

Sun_10_a_06_TP

13:42:08

13:57:47

2016.1.00298.S

Sun_10_a_06_TP

13:26:04

13:42:01

2016.1.00298.S

Sun_10_a_06_TP

13:25:37

15:07:49

2016.1.00298.S

Sun_10_a_06_INT

12:08:55

12:57:37

2017.1.00595.S

IRC-3039_a_07_7M

12:08:49

12:31:41

2017.1.01119.S

pks_1830_a_05_TM1

11:19:12

12:03:53

2016.1.00314.S

RCW120_b_07_7M

10:55:45

12:08:01

2017.A.00030.S

CK_Vul_a_05_TM1

10:35:02

12:13:55

2017.1.00040.S

cnd_cs76_e_07_TP

09:22:37

10:37:43

2017.1.00377.S

G337.92-_a_07_TM1

09:06:22

11:09:08

2017.1.01539.S

SgrB2_M_a_09_7M

08:35:12

09:21:20

2017.1.00377.S

G30.89+0_a_07_TM1

08:32:44

10:06:47

2017.1.00040.S

cnd_cs76_e_07_TP

07:13:54

08:35:05

2017.1.00753.S

NGC5253_a_08_TM1

07:12:37

08:23:58

2017.1.00040.S

cnd_cs54_d_06_TP

07:07:29

09:03:52

2017.1.01560.S

CO-0.40-_a_07_7M

05:49:22

07:10:13

2017.1.00753.S

NGC5253_a_08_TM1

and heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
Constraining the temperature andLeenaarts
heating mechanisms in the solar
plage chromosphere
DEATH STAR: DEtermining Accurate Ramstedt
mass-loss rates of THermally pulsing
AGB STARs
Carbon fractionation at redshift z=0.89Wallström

EU

Total Power

3

EU

Total Power

3

EU

Total Power

3

EU

Total Power

3

EU

Total Power

3

EU

Total Power

3

EU

Total Power

3

EU

Total Power

6

EU

Total Power

6

EU

Total Power

6

EU

Total Power

6

EU

Total Power

6

EU

Total Power

6

EU

Total Power

6

EU

12-m

6

EU

7-m

7

NA

12-m

5

Dissecting to decipher: an ALMA
Bronfmanstudy of the high-mass star formation
processes in RCW 120
First radioactive molecule observed in Kaminski
space: 26AlF in a stellar-merger
remnant
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

CL

7-m

7

NA

12-m

5

EA

Total Power

7

Exploring the mid-IR SED of highmass YSOs
Where's the oxygen in Sgr B2?

Leurini

EU

12-m

7

ComitoEU7-m

9Exploring the mid-IR SED of highLeurini
mass YSOs
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EU

12-m

7

EA

Total Power

7

Revisiting the star formation efficiency De Looze
of low-metallicity starburst galaxy
NGC5253
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EU

12-m

8

EA

Total Power

6

Dense Gas associated with the
TanakaClaimed Intermediate-mass Blackhole
Object CO-0.40
Revisiting the star formation
De Looze

EA

7-m

7

EU

12-m

8

05:20:45

07:07:22

2017.1.01565.S

IRAS_162_a_07_7M

04:30:45

05:48:37

2017.1.00886.L

NGC4571_b_06_TP

03:48:56

05:11:22

2017.1.00377.S

G301.14-_a_07_TM1

03:10:57

04:28:55

2017.1.00886.L

NGC4571_b_06_TP

02:44:41

04:08:122017.1.00297.S

PG1211+1_a_06_7M

02:17:20

03:30:05

2017.1.00326.S

cl01_a_07_TM1

01:59:15

03:10:50

2017.1.00886.L

NGC3507_b_06_TP

00:58:34

02:02:26

2017.1.01618.S

24.38380_a_06_TM1

00:47:35

01:59:08

2017.1.00886.L

NGC3507_b_06_TP

00:44:37

01:42:06

2017.1.01023.S

HH137_HH_a_06_7M

Start (UT)

End (UT)

Project Code

SchedBlock

23:38:11

00:19:54

2017.1.01353.S

23:20:14

00:27:41

2017.1.00271.S

23:16:48

00:44:31

22:39:47

efficiency of low-metallicity starburst
galaxy NGC5253
A comprehensive inventory of
Wampfler
nitrogen isotopic ratios in a nascentsolar system
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Exploring the mid-IR SED of highLeurini
mass YSOs
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
An ALMA-ACA Survey of CO(2-1) in Bauer
PG QSOs
ALMA Follow-up Survey for Clumpy Murata
Galaxies at z~0.9 in the COSMOS
Field
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Do there exist mini-SMGs at cosmic Kusakabe
noon?
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
Resolving molecular outflows inRubio
HH137 and HH138

EU

7-m

7

EU NA

Total Power

6

EU

12-m

7

EU NA

Total Power

6

CL

7-m

6

EA

12-m

7

EU NA

Total Power

6

EA

12-m

6

EU NA

Total Power

6

CL

7-m

6

Executive

Array

Band

OMC-1_Re_e_06_TM1 Fragmentation in the Orion Integral Takahashi
Shaped Filament
Ridge_ce_b_03_TP
Why is ~ 1/4 of the LMC's molecular Indebetouw
gas not forming massive stars?

EA

12-m

6

NA

Total Power3

2017.1.01644.S

GJ_273_a_06_7M

EU

7-m

6

23:38:04

2017.1.00093.S

YSO01_a_03_TM1

Searching for Kuiper-Belt analogues Amado
around the closest M-dwarf planetarysystems
Evolution of molecular clouds
Onishiassociated with O-type YSOs in giant
molecular clouds in the LMC

EA

12-m

3

17:34:30

17:44:52

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

17:24:00

17:34:22

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

17:13:31

17:23:53

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

17:03:01

17:13:23

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

16:52:32

17:02:54

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

16:42:02

16:52:23

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

16:31:34

16:41:56

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

16:21:06

16:31:28

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

16:10:36

16:20:57

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power3

16:00:07

16:10:28

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

15:49:37

15:59:59

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

15:43:35

17:47:07

2017.1.00072.S

Sun_10_b_03_INT

How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?

EA

12-m

3

2018-04-03
Project Title

PI15:39:07

15:49:29

2017.1.00072.S

Sun_10_a_03_TP

How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
How much do the cool components of Shimojo
solar X-ray jets contribute to the fastsolar wind?
Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power

3

15:28:37

15:38:59

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

15:18:05

15:28:27

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power3

15:07:33

15:17:57

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

14:57:00

15:07:25

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

14:46:30

14:56:54

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

14:35:57

14:46:22

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

14:25:18

14:35:50

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

14:14:48

14:25:122017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

14:03:35

14:14:38

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

13:52:23

14:03:27

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

13:40:56

13:52:15

2017.1.00072.S

Sun_10_a_03_TP

EA

Total Power

3

13:40:04

15:43:27

2017.1.00072.S

Sun_10_b_03_INT

EA

12-m

3

10:53:07

12:15:42

2017.1.00040.S

cnd_cs76_g_07_TP

EA

Total Power

7

10:43:51

11:47:20

2017.1.00820.S

Sgr_A_st_c_06_TM1

ALMA Monitoring of Sgr A*
coordinated with Spitzer & Chandra
Space Observatories in July 2018

Yusef-Zadeh

NA

12-m

6

09:19:32

10:43:46

2017.1.00820.S

Sgr_A_st_c_06_TM1

ALMA Monitoring of Sgr A*
coordinated with Spitzer & Chandra
Space Observatories in July 2018

Yusef-Zadeh

NA

12-m

6

09:12:02

11:09:40

2017.1.00377.S

G08.68-0_a_07_7M

Leurini

EU

7-m

7

08:15:30

09:19:27

2017.1.00820.S

Sgr_A_st_c_06_TM1

Exploring the mid-IR SED of highmass YSOs
ALMA Monitoring of Sgr A*
coordinated with Spitzer & Chandra
Space Observatories in July 2018

Yusef-Zadeh

NA

12-m

6

07:31:22

08:54:00

2017.1.00040.S

cnd_cs76_g_07_TP

Replenishing Molecular Gas Near the Hsieh
Supermassive Black Hole SgrA*

EA

Total Power7

07:13:25

09:11:51

2017.1.00377.S

G08.68-0_a_07_7M

Leurini

EU

7-m

7

06:40:17

08:15:25

2017.1.00820.S

Sgr_A_st_c_06_TM1

Exploring the mid-IR SED of highmass YSOs
ALMA Monitoring of Sgr A*
coordinated with Spitzer & Chandra
Space Observatories in July 2018

Yusef-Zadeh

NA

12-m

6

05:07:55

06:11:50

2017.1.00886.L

NGC4689_b_06_TP

EU NA

Total Power

604:44:23

06:25:45

2017.1.00820.S

Sgr_A_st_a_06_TM1

100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution
ALMA Monitoring of Sgr A*
Yusef-Zadeh
coordinated with Spitzer & Chandra
Space Observatories in July 2018

NA

12-m

6

03:50:31

04:39:57

2016.1.00285.S

H-ATLAS__a_07_TM1

NA

12-m

7

01:59:40

02:21:09

2017.1.00508.S

J1211-01_a_06_TM1

EA

12-m

6

01:55:50

03:15:41

2017.1.00886.L

NGC4569_a_06_7M

The Ionizing Flux in Lensed Galaxies Indrioloat z~2
Investigating ISM Physics at z~6 with Harikane
Multiple FIR Lines of NewlyDiscovered Luminous Galaxies
100,000 Molecular Clouds Across the Schinnerer
Main Sequence: GMCs as the Driversof Galaxy Evolution

EU NA

7-m

6

01:13:27

01:38:05

2017.1.00255.S

IRASF104_a_06_TM2

Revealing the internal structure of
Pereira Santaella EU
molecular outflows: spatially resolved
observations in local LIRGs

12-m

6

00:18:38

01:13:20

2017.1.00478.S

SDSS_J08_c_06_TM1

NA

12-m

6

00:05:50

01:20:42

2017.1.00527.S

G09.v10._c_06_7M

Feedback and Star Formation in
HamannExtremely Red Quasars
The molecular gas and resolved star- Oteo
formation law in low-redshift SMGs

EU

7-m

6

Start (UT)

End (UT)

Project Code

SchedBlock

Project Title

Executive

Array

Band

23:52:36

00:18:31

2017.1.00255.S

ESO_557-_a_06_TM2

Revealing the internal structure of
Pereira Santaella EU
molecular outflows: spatially resolved
observations in local LIRGs

12-m

6

22:15:20

23:17:01

2017.1.00093.S

YSO01_a_03_TM1

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

EA

12-m

3

22:06:18

23:27:40

2017.1.00823.S

Cloud_4_a_03_7M

How do GMCs start to form massive Ochsendorf
stars? An ALMA survey of young,massive star forming GMCs in the
LMC

NA

7-m

3

21:16:30

22:13:50

2017.1.01512.S

ALESS001_d_03_TM1

EU

12-m

3

20:20:04

21:41:30

2017.1.00823.S

Cloud_4_a_03_7M

Gas mass fractions in z>3 main
Weisssequence galaxies from ALESS
How do GMCs start to form massive Ochsendorf
stars? An ALMA survey of young,massive star forming GMCs in the
LMC

NA

7-m

3

2018-04-02
PI