Page History

...

Support for self-calibration within mosaics (interpolation over entire multiple fields/scans).
switch to nterms =2 imaging for high S/N cases
Amplitude selfcal (solnorm = True) following successful phase selfcal
handling bright sources outside main primary beam (edge case?)
Per-spw calibration (defined allowed for solutions across entire EB already, may not be needed)
allowing applymode=calonly for some data to attempt to solve for those data by cleaning deeper holding solint constant

Selfcal Prototype:

Interpolation from high S/N target to low S/N target

Documentation of requirements:

https://www.overleaf.com/1674875949hqpbbpdtdzym

Selfcal Prototype:

Obtain via 'git clone https://github.com/jjtobin/auto_selfcal'

Copy scripts to working directory where _target.ms files reside
Start CASA in MPI mode (i.e., mpicasa -n 9 /path/to/casa/bin/casa); otherwise edit script to set parallel=False
run via execfile('auto_selfcal.py')
- will make use of cont.dat to flag line channels if cont.dat is present, otherwise will use all channels
- Can make use of spectral averaging by setting spectral_average=True in auto_selfcal.py
  - averaging depends on frequency for VLA, will simply average to 15.625 MHz channels for ALMA

Aggregate Test Suite plots for ALMA (includes both John and Ilsang's runs):

Image AddedImage AddedImage Added

Test Suite:

Telescope

Project Code

MOUS/FSID &

Selfcal Log

Band

Conf.

EBs

Tgts

Version

Notes

Original Peak SNR

Selfcal Peak SNR

min solint

Original RMS

(mJy/bm or uJy/beam)

Final RMS

(mJy/bm or uJy/beam)

ALMA

2019

E2E6.1.

01709

00085.S

uid://

A001

A002/

X1465/X4356C-321Jan 5

All cont spw

Strong point-like continuum source and faint radio jet separated by 3x beam size

Final selfcal image captures the faint radio jet better than the original PL image does

PKS1030-357: 109PKS1030-357: 254PKS1030-357: 10.08sPKS1030-357: 0.053PKS1030-357: 0.030ALMA

Xd00f1f/Xca

Selfcal Log

7

C1

1

Feb 14

spec scan project

cont and line morphology different

flux resolved out (selfcal seems doing well)

G31.41+0.31: 189

G31.41+0.31: 516

G31.41+0.31: inf_EB

G31.41+0.31: 0.00994

G31.41+0.31: 0.00368

ALMA

2018.1.00962

2019.1.01709

.S	uid://A001/

X1465/X4313

X133d/X272b

Selfcal Log

9

C3

C-5

1

Jan 5

All cont spw

strong point source continuum

Selfcal failed due to increased final RMS. But actual images (original PL image and selfcal image) are not very different in terms of RMS and peak SNR. This dataset needs some investigation.

4C-03.79: 5

4C-03.79: 715

Seems to be increased by erroneous estimate of the original RMS

4C-03.79: None

4C-03.79: 0.009

This reported value (9.8e-6 Jy) from pickle file seems wrong. Original PL image has RMS of 1 mJy/beam

4C-03.79: 1

Feb 14

flux resolved out (selfcal seems doing well)

NGC6334I: 58

NGC6334I: 144

NGC6334I: inf_EB

NGC6334I: 0.052

NGC6334I: 0.021

ALMA

2017.A.00042.T

uid://A001/X1306/X5e

Selfcal Log

5

C1/2

1

Feb 14

cont and line morphology different (different centroid)

iras16293-2422: 306

iras16293-2422: 1074

iras16293-2422: 90.72s

iras16293-2422: 0.00238

iras16293-2422: 0.00069

ALMA

2017.1.00855.S

uid://A001/X1284/X10c9

Selfcal Log

3

C6

2

1

Feb 14

Uranus: 200

Uranus: 833

Uranus: inf

Uranus: 0.000301

Uranus: 0.000075

ALMA

2017.1.00670.S

uid://A001/X1284/X20e0

Selfcal Log

7

C4

1

Feb 14

Io: 148

Io: 285

Io: inf

Io: 0.0072

Io: 0.0036

ALMA

2017.1.00661.S

uid://A001/X128e/X222

Selfcal Log

4

ACA

8

1

Feb 14

poor uv coverage (PSF sidelobe)

NGC6334I: 101

NGC6334I: 704

NGC6334I: 90.72s

NGC6334I: 0.035

NGC6334I: 0.004

ALMA

2016.1.00577.S

uid://A001/X87c/X10d

Selfcal Log

6

ACA

4

1

Feb 14

poor uv coverage (PSF sidelobe)

G333.6-0.2: 47

G333.6-0.2: 216

G333.6-0.2: inf_EB

G333.6-0.2: 0.104

G333.6-0.2: 0.028

ALMA

2015.1.00150.S

uid://A001/X2f6/X265

Selfcal Log

7

C1/2

1

Feb 14

NGC_6334I: 126

NGC_6334I: 395

NGC_6334I: inf

NGC_6334I: 0.0346

NGC_6334I: 0.0115

ALMA

2018.1.01055.L

uid://A001/X133d/X19d5

Selfcal Log

6

C7

3

1

Jan 12

concentric rings (protoplanetary disk) captured better by selfcal

different cont and line morphology

HD163296: 366

HD163296: 801

HD163296: inf

HD163296: 44.7

HD163296: 21.3

ALMA

2018.1.00659.L

uid://A001/X133d/X1284

Selfcal Log

6

C5/6

2

1

Jan 12

Field center differ across EBs by 376 microarcsec (beyond the 200 microarcsec criteria) but maybe OK if this has large proper motion

R_Hya: 196

R_Hya: 1201

R_Hya: int

R_Hya: 167

R_Hya: 42.4

ALMA

E2E8.1.00062.S

uid://A001/X1587/X51b

Selfcal Log

6

ACA

3

2

Jan 12

For some reason, primary or backup flux was not queried when importing the data. ASDM value was used.

Poor uv-coverage (PSF sidelobe)

SDC13_MM2: Selfcal success code: False

SDC13_MM1: 20

SDC13_MM2: 14

SDC13_MM1: 39

SDC13_MM2: 14

SDC13_MM1: inf_EB

SDC13_MM2: None

SDC13_MM1: 0.0016

SDC13_MM2: 0.0015

SDC13_MM1: 0.0008

SDC13_MM2: 0.0015

ALMA

2019.1.00847.S

uid://A001/X1467/X264

Selfcal Log

7

ACA

3

5

Jan 12

For some reason, primary or backup flux was not queried when importing the data. ASDM value was used.

Poor uv-coverage (PSF sidelobe)

IRAM04191: Selfcal success code: False

04191+1523: 58

04287+1801: 86

04288+1802: 78

HH_30: 51

IRAM04191: 9.7

04191+1523: 146

04287+1801: 464

04288+1802: 560

HH_30: 61

IRAM04191: 9.7

04191+1523: 30.24s

04287+1801: inf

04288+1802: inf_EB

HH_30: inf_EB

IRAM04191: None

04191+1523: 0.0026

04287+1801: 0.027

04288+1802: 0.015

HH_30: 0.001

IRAM04191: 0.002

04191+1523: 0.0011

04287+1801: 0.005

04288+1802: 0.002

HH_30: 0.0008

IRAM04191: 0.002

ALMA

2019.1.01709.S

uid://A001/X1465/X435

Selfcal Log

6

C-3

2

1

Jan 5

All cont spw

Strong point-like continuum source and faint radio jet separated by 3x beam size

Final selfcal image captures the faint radio jet better than the original PL image does

PKS1030-357: 109

PKS1030-357: 254

PKS1030-357: 10.08s

PKS1030-357: 0.053

PKS1030-357: 0.030

ALMA

2019.1.01709.S

uid://A001/X1465/X431

Selfcal Log

3

C-5

1

Jan 5

All cont spw

strong point source continuum

4C-03.79: 614

4C-03.79: 5300

4C-03.79: 151.20s

4C-03.79: 1.19

4C-03.79: 0.14

ALMA

2019.1.01197.S

uid://A001/X1465/X15aa

Selfcal Log

6

C-3

1

Jan 5

All cont spw

Continuum source with lensed morphology

PJ011646.8: 34

PJ011646.8: 38

PJ011646.8: 52.42s

PJ011646.8: 0.1

PJ011646.8: 0.09

ALMA

2019.1.00463.S

uid://A001/X146a/Xf

Selfcal Log

6

C-6

1

Jan 5

mixture of narrow(59, 234MHz)/wide (1.8GHz) band width

continuum source off phase center

BHR7: 322

BHR7: 742

BHR7: 42.34s

BHR7: 0.072

BHR7: 0.043

ALMA

2019.1.01425.S

uid://A001/X1465/Xd60

6

C-10

1

5

Jan 20

uses full MS

low-SB extended emission surrounding point-like sources

L1448IRS3B: 85

L1448IRS1: 97

L1448IRS3C: 90

Per-emb-17: 100

Per-emb-22: 107

L1448IRS3B: 93

L1448IRS1: 101

L1448IRS3C: 97

Per-emb-17: 108

Per-emb-22: 150

L1448IRS3B: inf_EB

L1448IRS1: inf_EB

L1448IRS3C: inf_EB

Per-emb-17: inf_EB

Per-emb-22: inf

L1448IRS3B: 0.033

L1448IRS1: 0.031

L1448IRS3C: 0.031

Per-emb-17: 0.031

Per-emb-22: 0.031

L1448IRS3B: 0.032

L1448IRS1: 0.031

L1448IRS3C: 0.031

Per-emb-17: 0.031

Per-emb-22: 0.031

ALMA

2017.1.01413.S

uid://A001/X1273/X7bc

Selfcal Log

6

C-4

2

5

Jan 20

uses full MSes, cont.dat, test case for spectral averaging

compact, disk sources

L1527-IRS Band_6: 471

TMC1A Band_6: 411

IRAS_04302+2247 Band_6: 158

L1489IRS Band_6: 115

TMC1 Band_6: 211

L1527-IRS Band_6: 1729

TMC1A Band_6: 2002

IRAS_04302+2247 Band_6: 157

L1489IRS Band_6: 135

TMC1 Band_6: 295

L1527-IRS Band_6: 30.24s

TMC1A Band_6: 30.24s

IRAS_04302+2247 Band_6: None

L1489IRS Band_6: inf

TMC1 Band_6: 30.24s

L1527-IRS Band_6: 0.214

TMC1A Band_6: 0.299

IRAS_04302+2247 Band_6: 0.131

L1489IRS Band_6: 0.058

TMC1 Band_6: 0.073

L1527-IRS Band_6: 0.061

TMC1A Band_6: 0.065

IRAS_04302+2247 Band_6: 0.131

L1489IRS Band_6: 0.054

TMC1 Band_6: 0.057

ALMA

''

Jan 20

does not use spectral averaging

compact, disk sources

L1527-IRS Band_6: 470

TMC1A Band_6: 413

IRAS_04302+2247 Band_6: 158

L1489IRS Band_6: 116

TMC1 Band_6: 230

L1527-IRS Band_6: 1710

TMC1A Band_6: 1925

IRAS_04302+2247 Band_6: 316

L1489IRS Band_6: 138

TMC1 Band_6: 322

L1527-IRS Band_6: 30.24s

TMC1A Band_6: 30.24s

IRAS_04302+2247 Band_6: inf_EB

L1489IRS Band_6: inf

TMC1 Band_6: 12.10s

L1527-IRS Band_6: 0.214

TMC1A Band_6: 0.296

IRAS_04302+2247 Band_6: 0.130

L1489IRS Band_6: 0.058

TMC1 Band_6: 0.067

L1527-IRS Band_6: 0.061

TMC1A Band_6: 0.067

IRAS_04302+2247 Band_6: 0.070

L1489IRS Band_6: 0.052

TMC1 Band_6: 0.052

ALMA

2019.1.00261.L

uid://A001/X146c/X26f

Selfcal Log

6

C-5

2

Jan 20

spectrally averaged, 2 spws, used for fast runs

IRAS32: 507

IRS5N: 588

IRAS32: 1244

IRS5N: 1039

IRAS32: 18.14s

IRS5N: int

IRAS32: 0.092

IRS5N: 0.061

IRAS32: 0.039

IRS5N: 0.036

ALMA

2018.1.00427

ALMA2019.1.01197.Suid://A001/X1465/X15aa6C-311Jan 5

All cont spw

Continuum source with lensed morphology

PJ011646.8: 34PJ011646.8: 38PJ011646.8: 52.42s

PJ011646.8: 0.1

PJ011646.8: 0.09ALMA2019.1.00463

.S	uid://A001/

X146a/Xf

X133d/X1b87

Selfcal Log

6

C-

6

9

1

2

1

Jan

5

mixture of narrow(59, 234MHz)/wide (1.8GHz) band width

continuum source off phase center

20

uses only continuum spw

compact sources

IRAS2A Band_6: 224

IRAS2A Band_6: 995

IRAS2A Band_6: inf

IRAS2A Band_6: 0.109

IRAS2A Band_6: 0.041

ALMA

2015.1.01503

BHR7: 322BHR7: 742BHR7: 42.34sBHR7: 0.072BHR7: 0.043ALMA2019.1.01425

.S	uid://A001/

X1465/Xd60

X2d8/X287

Selfcal Log

7

6

C-

10

4

1

6

5

11

Nov

uses full MS

low-SB extended emission surrounding point-like sources

L1448IRS3B: 85

L1448IRS1: 97

L1448IRS3C: 90

Per-emb-17: 100

Per-emb-22: 107

Jan 20

polarization project, all data in a single combined MS, uses TDM

sources range from very extended to somewhat extended

Per26 Band_7: 224

Per18 Band_7: 174

Per21 Band_7: 200

Per11 Band_7: 270

Per14 Band_7: 266

Per50 Band_7: 223

Per2 Band_7: 161

Per5 Band_7: 292

Per41 Band_7: 164

Per29 Band_7: 251

Per26 Band_7: 1162

Per18 Band_7: 583

Per21 Band_7: 704

Per11 Band_7: 1029

Per14 Band_7: 794

Per50 Band_7: 1157

Per2 Band_7: 390

Per5 Band_7: 1087

Per41 Band_7: 283

Per29 Band_7: 1149

Per26 Band_7: int

Per18 Band_7: int

Per21 Band_7: int

Per11 Band_7: int

Per14 Band_7: int

Per50 Band_7: int

Per2 Band_7: int

Per5 Band_7: int

Per41 Band_7: 14.11s

Per29 Band_7: int

Per26 Band_7: 0.976

Per18 Band_7: 0.493

Per21 Band_7: 0.368

Per11 Band_7: 0.601

Per14 Band_7: 0.329

Per50 Band_7: 0.553

Per2 Band_7: 0.485

Per5 Band_7: 0.759

Per41 Band_7: 0.148

Per29 Band_7: 0.643

Per26 Band_7: 0.231

Per18 Band_7: 0.170

Per21 Band_7: 0.128

Per11 Band_7: 0.180

Per14 Band_7: 0.130

Per50 Band_7: 0.135

Per2 Band_7: 0.220

Per5 Band_7: 0.233

Per41 Band_7: 0.098

Per29 Band_7: 0.163

ALMA

2018.1.00962.S

uid://A001/X133d/X2727

9

C-3

1

Jan 20

uses full MSes, cont.dat,

extended emission

NGC6334I: 46

NGC6334I: 106

NGC6334I: int

NGC6334I: 62.618

NGC6334I: 28.644

ALMA

2017.1.00586.S

uid://A001/X1284/X20cf

Selfcal Log

8

C-2?

3

2

Jan 20

uses full MSes, cont.dat,

some extended emission, collections of point sources

NGC_1068 Band_8: 61

NGC_1068_SBring Band_8: 49

NGC_1068_CH3OH Band_8: 11

NGC_1068 Band_8: 77

NGC_1068_SBring Band_8: 61

NGC_1068_CH3OH Band_8: 11

NGC_1068 Band_8: inf_EB

NGC_1068_SBring Band_8: inf_EB

NGC_1068_CH3OH Band_8: None

NGC_1068 Band_8: 0.322

NGC_1068_SBring Band_8: 0.301

NGC_1068_CH3OH Band_8: 0.237

NGC_1068 Band_8: 0.266

NGC_1068_SBring Band_8: 0.257

NGC_1068_CH3OH Band_8: 0.237

ALMA

2018.1.00510.S

uid://A001/X133d/X1e68

Selfcal Log

6

C-9

2

1

Jan 20

uses 3 TDM windows

fails due to beam, calonly would help here

well-resolved in C-10

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: None

NGC1333_IRAS_4A Band_6: 0.143

''

Jan 20

'', calonly

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: 460

NGC1333_IRAS_4A Band_6: int

NGC1333_IRAS_4A Band_6: 0.143

NGC1333_IRAS_4A Band_6: 0.054

ALMA

2013.1.00879

L1448IRS3B: 93

L1448IRS1: 101

L1448IRS3C: 97

Per-emb-17: 108

Per-emb-22: 150

L1448IRS3B: inf_EB

L1448IRS1: inf_EB

L1448IRS3C: inf_EB

Per-emb-17: inf_EB

Per-emb-22: inf

L1448IRS3B: 0.033

L1448IRS1: 0.031

L1448IRS3C: 0.031

Per-emb-17: 0.031

Per-emb-22: 0.031

L1448IRS3B: 0.032

L1448IRS1: 0.031

L1448IRS3C: 0.031

Per-emb-17: 0.031

Per-emb-22: 0.031

ALMA2017.1.01413.Suid://A001/X1273/X7bc6C-425Dec 3

uses full MSes, cont.dat, test case for spectral averaging

compact, disk sources

L1527-IRS Band_6: 471

TMC1A Band_6: 411

IRAS_04302+2247 Band_6: 158

L1489IRS Band_6: 115

TMC1 Band_6: 211

L1527-IRS Band_6: 1729

TMC1A Band_6: 2002

IRAS_04302+2247 Band_6: 157

L1489IRS Band_6: 135

TMC1 Band_6: 295

L1527-IRS Band_6: 30.24s

TMC1A Band_6: 30.24s

IRAS_04302+2247 Band_6: None

L1489IRS Band_6: inf

TMC1 Band_6: 30.24s

L1527-IRS Band_6: 0.214

TMC1A Band_6: 0.299

IRAS_04302+2247 Band_6: 0.131

L1489IRS Band_6: 0.058

TMC1 Band_6: 0.073

L1527-IRS Band_6: 0.061

TMC1A Band_6: 0.065

IRAS_04302+2247 Band_6: 0.131

L1489IRS Band_6: 0.054

TMC1 Band_6: 0.057

ALMA''''''''''''Nov

does not use spectral averaging

compact, disk sources

L1527-IRS: 451

TMC1A: 398

IRAS_04302+2247: 151

L1489IRS: 110

TMC1: 227

L1527-IRS: 1681

TMC1A: 1909

IRAS_04302+2247: 231

L1489IRS: 139

TMC1: 324

L1527-IRS: inf

TMC1A: 30.24s

IRAS_04302+2247: None

L1489IRS: inf

TMC1: 12.10s

L1527-IRS: 0.222

TMC1A: 0.307

IRAS_04302+2247: 0.137

L1489IRS: 0.061

TMC1: 0.068

L1527-IRS: 0.062

TMC1A: 0.068

IRAS_04302+2247: 0.099

L1489IRS: 0.052

TMC1: 0.051

ALMA2019.1.00261.Luid://A001/X146c/X26f6C-522Dec 3spectrally averaged, 2 spws, used for fast runs

IRAS32: 507

IRS5N: 588

IRAS32: 1244

IRS5N: 1039

IRAS32: 18.14s

IRS5N: int

IRAS32: 0.092

IRS5N: 0.061

IRAS32: 0.039

IRS5N: 0.036

ALMA2018.1.00427.Suid://A001/X133d/X1b876C-921Dec 3

uses only continuum spw

compact sources

IRAS2A Band_6: 224

IRAS2A Band_6: 995

IRAS2A Band_6: inf

IRAS2A Band_6: 0.109

IRAS2A Band_6: 0.041

ALMA2015.1.01503

.S	uid://A001/

X2d8/X287

X11f/X7f

Selfcal Log

6

7

C-

4611Dec 3

polarization project, all data in a single combined MS, uses TDM

sources range from very extended to somewhat extended

Per26 Band_7: 224

Per18 Band_7: 174

Per21 Band_7: 200

Per11 Band_7: 270

Per14 Band_7: 266

Per50 Band_7: 223

Per2 Band_7: 161

Per5 Band_7: 292

Per41 Band_7: 164

Per29 Band_7: 251

Per26 Band_7: 1162

Per18 Band_7: 583

Per21 Band_7: 704

Per11 Band_7: 1029

Per14 Band_7: 794

Per50 Band_7: 1157

Per2 Band_7: 390

Per5 Band_7: 1087

Per41 Band_7: 283

Per29 Band_7: 1149

Per26 Band_7: int

Per18 Band_7: int

Per21 Band_7: int

Per11 Band_7: int

Per14 Band_7: int

Per50 Band_7: int

Per2 Band_7: int

Per5 Band_7: int

Per41 Band_7: 14.11s

Per29 Band_7: int

Per26 Band_7: 0.976

Per18 Band_7: 0.493

Per21 Band_7: 0.368

Per11 Band_7: 0.601

Per14 Band_7: 0.329

Per50 Band_7: 0.553

Per2 Band_7: 0.485

Per5 Band_7: 0.759

Per41 Band_7: 0.148

Per29 Band_7: 0.643

Per26 Band_7: 0.231

Per18 Band_7: 0.170

Per21 Band_7: 0.128

Per11 Band_7: 0.180

Per14 Band_7: 0.130

Per50 Band_7: 0.135

Per2 Band_7: 0.220

Per5 Band_7: 0.233

Per41 Band_7: 0.098

Per29 Band_7: 0.163

ALMA

3

2

1

Jan 20

ALMA

2017.1.00419.S

uid://A001/X1284/X149

Selfcal Log

6

C-5/6

1

20

Jan 25

Mix of wide and narrow windows

ALMA

2017.1.00449.S

uid://A001/X1289/Xa6

Selfcal Log

7

C-5/6

1

Jan 22

Mostly wide windows

ALMA

2017.1.00449.S

uid://A001/X1289/Xaa

Selfcal Log

6

C-5/6

1

Jan 22

Mostly wide windows

ALMA

2017.1.00449.S

uid://A001/X1296/X7a5

Selfcal Log

3

C-8

1

Jan 22

Mostly wide windows

ALMA

2018.1.01119.S

uid://A001/X133d/X2c5e

Selfcal Log

6

C-6

5

1

Jan 22

Mostly wide windows

ALMA

2013.1.00937

2018.1.00962

.S	uid://A001/

X133d/X2727

X144/X189

Selfcal Log

6

9

C-

311Nov

uses full MSes, cont.dat,

extended emission

NGC6334I: 46

NGC6334I: 106

NGC6334I: int

NGC6334I: 62.618

NGC6334I: 28.644

6

2

6

Jan 22

Mostly wide windows

ALMA

2019.1.00218.S

uid://A001/X1465/X365e

Selfcal Log

6

C-2

1

100

Jan 22

Mostly wide windows

ACA

ALMA

2017.1.

00586

00857.S

uid://A001/

X1284/X20cf

X12c4/X217

Selfcal Log

8

C-2?32

ACA

8

4

Jan 20

Dec 3

uses full MSes, cont.dat,

some extended emission, collections of

point sources

NGC

DR_

1068

Tau Band_8:

61

126

NGC

DO_

1068_SBring

Tau Band_8:

49

38

NGC

DL_

1068_CH3OH

Tau Band_8:

11

38

NGC

FZ_

1068

Tau Band_8:

77

21

NGC

DR_

1068_SBring

Tau Band_8:

61

272

NGC

DO_

1068_CH3OH

Tau Band_8:

11

227

NGC

DL_

1068

Tau Band_8:

inf_EB

279

NGC

FZ_

1068_SBring

Tau Band_8:

inf_EB

21

NGC

DR_

1068_CH3OH

Tau Band_8:

None

inf

NGC

DO_

1068

Tau Band_8:

0.322

inf

NGC

DL_

1068_SBring

Tau Band_8:

0.301

int

NGC

FZ_

1068_CH3OH

Tau Band_8:

0.237

None

NGC

DR_

1068

Tau Band_8:

0

5.

266

514

NGC

DO_

1068_SBring

Tau Band_8:

0

12.

257

132

NGC

DL_

1068_CH3OH

Tau Band_8:

0

17.

237ALMA2018.1.00510.S6C-921Dec 3

uses 3 TDM windows

fails due to beam, calonly would help here

well-resolved in C-10

709

FZ_Tau Band_8: 2.403

DR_Tau Band_8: 2.578

DO_Tau Band_8: 2.227

DL_Tau Band_8: 2.648

FZ_Tau Band_8: 2.403

ACA

2017.1.00857.S

uid://A001/X12c4/X21f

Selfcal Log

8

ACA

1

Jan 20

full MSes, cont.dat

point source

AS_205A: 63

AS_205A: 385

AS_205A: inf

AS_205A: 24.770

AS_205A: 4.102

ALMA

2019.1.00261

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: None

NGC1333_IRAS_4A Band_6: 0.143

''''''''''''''Dec 3'', calonly

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: 460

NGC1333_IRAS_4A Band_6: int

NGC1333_IRAS_4A Band_6: 0.143

NGC1333_IRAS_4A Band_6: 0.054

ALMA-ACA2017.1.00857.S

uid://A001/

X12c4

X146c/

X217

X26a

8

6

ACA

C-5

8

2

4

1

Dec 3

uses full MSes, cont.dat,

point sources


ALMA	2019.1.00261	uid://A001/X146c/X26f	6	C-5	2	2
ALMA	2019.1.00261	uid://A001/X146c/X263	6	C-8/9	2(5)	2
ALMA	2019.1.00261	uid://A001/X146c/X259	6	C-8/9	1(4)	2
ALMA	2019.1.00255.S	uid://A001/X1465/X3541	6	C-6	1	1
ALMA	2019.1.00255

DR_Tau Band_8: 126

DO_Tau Band_8: 38

DL_Tau Band_8: 38

FZ_Tau Band_8: 21

DR_Tau Band_8: 272

DO_Tau Band_8: 227

DL_Tau Band_8: 279

FZ_Tau Band_8: 21

DR_Tau Band_8: inf

DO_Tau Band_8: inf

DL_Tau Band_8: int

FZ_Tau Band_8: None

DR_Tau Band_8: 5.514

DO_Tau Band_8: 12.132

DL_Tau Band_8: 17.709

FZ_Tau Band_8: 2.403

DR_Tau Band_8: 2.578

DO_Tau Band_8: 2.227

DL_Tau Band_8: 2.648

FZ_Tau Band_8: 2.403

ALMA-ACA2017.1.00857

.S	uid://A001/

X12c4

X1465/

X21f

X353f

8

6

C-9/10

ACA

1

Dec 3

full MSes, cont.dat

point source

AS_205A: 63AS_205A: 385AS_205A: infAS_205A: 24.770


ALMA	2018.1.01038.S	uid://A001/X133f/X82	6	C-5/6	8	11

AS_205A: 4.102

VLA

13B-454

13B-454.sb29509255.eb29947371.56956.79185517361

C

1

Dec 6

M82, high DR, extended

SN2014J EVLA_C: 1506

SN2014J EVLA_C: 6393

SN2014J EVLA_C: 17.00s

SN2014J EVLA_C: 0.105

SN2014J EVLA_C: 0.030

VLA

13B-454

13B-454.sb29105214.eb29105303.56758.17242523148

C

A

1

Nov

M82, high DR, extended

Very long run time

SN2014J EVLA_C: 5933

SN2014J EVLA_C: 6078

SN2014J EVLA_C: 35.00s

SN2014J EVLA_C: 0.005

VLA

15A-370

15A-370.sb30976913.eb30980293.57204.36680753472

15A-370.sb30976913.eb30978455.57203.32521244213

Ka, Q

A

2

1

Dec 3

compact, low DR

L1157 EVLA_KA: 28

L1157 EVLA_Q: 19

L1157 EVLA_KA: 27

L1157 EVLA_Q: 19

L1157 EVLA_KA: None

L1157 EVLA_Q: None

L1157 EVLA_KA: 0.011

L1157 EVLA_Q: 0.020

L1157 EVLA_KA: 0.011

L1157 EVLA_Q: 0.020

VLA

17B-188

17B-188.sb35564398.eb35590549.58363.10481791667

S,C,Ku,K,Ka

C

1

2

Dec 3

compact at HF, compact+extended at LF, multiband

14C_KuQ_C EVLA_K: 110

14C_KuQ_C EVLA_KA: 73

14C_KuQ_C EVLA_KU: 185

14C_SC_C EVLA_C: 1196

14C_SC_C EVLA_S: 1558

14C_KuQ_C EVLA_K: 212

14C_KuQ_C EVLA_KA: 116

14C_KuQ_C EVLA_KU: 257

14C_SC_C EVLA_C: 1384

14C_SC_C EVLA_S: 1635

14C_KuQ_C EVLA_K: int

14C_KuQ_C EVLA_KA: inf

14C_KuQ_C EVLA_KU: 33.00s

14C_SC_C EVLA_C: inf

14C_SC_C EVLA_S: int

14C_KuQ_C EVLA_K: 0.079

14C_KuQ_C EVLA_KA: 0.080

14C_KuQ_C EVLA_KU: 0.068

14C_SC_C EVLA_C: 0.021

14C_SC_C EVLA_S: 0.025

14C_KuQ_C EVLA_K: 0.050

14C_KuQ_C EVLA_KA: 0.058

14C_KuQ_C EVLA_KU: 0.052

14C_SC_C EVLA_C: 0.018

14C_SC_C EVLA_S: 0.024

VLA

TDRW0001

TDRW0001.sb35624494.eb35628826.58395.23719237269

S

D

1

Dec 3

extended, high DR

3C75 EVLA_S: 3815

3C75 EVLA_S: 6733

3C75 EVLA_S: 25.00s

3C75 EVLA_S: 0.038

3C75 EVLA_S: 0.022

VLA

16B-427

16B-427.sb33651951.eb34041883.57963.57173581018

L,S,C,X,K, Q

C

1

Dec 3

multiband

S255 NIRS3 EVLA_C: 1107

S255 NIRS3 EVLA_K: 473

S255 NIRS3 EVLA_L: 570

S255 NIRS3 EVLA_Q: 250

S255 NIRS3 EVLA_S: 596

S255 NIRS3 EVLA_X: 1849

S255 NIRS3 EVLA_C: 1173

S255 NIRS3 EVLA_K: 681

S255 NIRS3 EVLA_L: 550

S255 NIRS3 EVLA_Q: 564

S255 NIRS3 EVLA_S: 622

S255 NIRS3 EVLA_X: 2267

S255 NIRS3 EVLA_C: 80.00s

S255 NIRS3 EVLA_K: 21.00s

S255 NIRS3 EVLA_L: inf

S255 NIRS3 EVLA_Q: 36.00s

S255 NIRS3 EVLA_S: inf_EB

S255 NIRS3 EVLA_X: 9.00s

S255 NIRS3 EVLA_C: 0.014

S255 NIRS3 EVLA_K: 0.053

S255 NIRS3 EVLA_L: 0.059

S255 NIRS3 EVLA_Q: 0.109

S255 NIRS3 EVLA_S: 0.025

S255 NIRS3 EVLA_X: 0.011

S255 NIRS3 EVLA_C: 0.013

S255 NIRS3 EVLA_K: 0.041

S255 NIRS3 EVLA_L: 0.061

S255 NIRS3 EVLA_Q: 0.069

S255 NIRS3 EVLA_S: 0.024

S255 NIRS3 EVLA_X: 0.010

VLA

20A-390

20A-390.sb37850360.eb37919292.58894.32864972222
20A-390.sb37850360.eb37920910.58895.323193819444
20A-390.sb37850360.eb37926293.58898.356132071756
20A-390.sb37850360.eb37933285.58900.24178115741
20A-390.sb37850360.eb37933287.58900.32599280092

Ka

C

5

1

Dec 3

point source, low dec

TWHya EVLA_KA: 164

TWHya EVLA_KA: 278

TWHya EVLA_KA: 129.00s

TWHya EVLA_KA: 0.005

VLA

21A-178

21A-178.sb39472833.eb39589695.59326.113018460645

X

D

1

21

Nov

variety of S/N

SN 2014L EVLA_X: 113

SN 2004gk EVLA_X: 37

SN 1990B EVLA_X: 173

SN 2004cc EVLA_X: 176

SN 1987K EVLA_X: 661

PTF10bfz EVLA_X: 421

SN 1997dq EVLA_X: 17

SN 2011bm EVLA_X: 209

SN 2015bn EVLA_X: 217

SN 2003dg EVLA_X: 15

SN 2007I EVLA_X: 32

SN 2004gn EVLA_X: 456

SN 2007rw EVLA_X: 18

SN 2000ew EVLA_X: 21

SN 2014ad EVLA_X: 33

SN 2002bm EVLA_X: 60

SN 2008aq EVLA_X: 14

SN 2005bh EVLA_X: 6

SN 2004gj EVLA_X: 34

SN 2002ji EVLA_X: 76

LSQ13abf EVLA_X: 9

SN 2014L EVLA_X: 114

SN 2004gk EVLA_X: 37

SN 1990B EVLA_X: 174

SN 2004cc EVLA_X: 175

SN 1987K EVLA_X: 732

PTF10bfz EVLA_X: 429

SN 1997dq EVLA_X: 17

SN 2011bm EVLA_X: 216

SN 2015bn EVLA_X: 240

SN 2003dg EVLA_X: 15

SN 2007I EVLA_X: 32

SN 2004gn EVLA_X: 464

SN 2007rw EVLA_X: 18

SN 2000ew EVLA_X: 21

SN 2014ad EVLA_X: 34

SN 2002bm EVLA_X: 61

SN 2008aq EVLA_X: 14

SN 2005bh EVLA_X: 6

SN 2004gj EVLA_X: 35

SN 2002ji EVLA_X: 76

LSQ13abf EVLA_X: 9

SN 2014L EVLA_X: 9.00s

SN 2004gk EVLA_X: 81.00s

SN 1990B EVLA_X: inf_EB

SN 2004cc EVLA_X: inf_EB

SN 1987K EVLA_X: 18.00s

PTF10bfz EVLA_X: 39.00s

SN 1997dq EVLA_X: inf_EB

SN 2011bm EVLA_X: int

SN 2015bn EVLA_X: 39.00s

SN 2003dg EVLA_X: None

SN 2007I EVLA_X: inf_EB

SN 2004gn EVLA_X: inf_EB

SN 2007rw EVLA_X: inf_EB

SN 2000ew EVLA_X: inf_EB

SN 2014ad EVLA_X: 81.00s

SN 2002bm EVLA_X: 39.00s

SN 2008aq EVLA_X: None

SN 2005bh EVLA_X: None

SN 2004gj EVLA_X: 81.00s

SN 2002ji EVLA_X: 162.00s

LSQ13abf EVLA_X: None

SN 2014L EVLA_X: 0.014

SN 2004gk EVLA_X: 0.011

SN 1990B EVLA_X: 0.013

SN 2004cc EVLA_X: 0.013

SN 1987K EVLA_X: 0.046

PTF10bfz EVLA_X: 0.012

SN 1997dq EVLA_X: 0.013

SN 2011bm EVLA_X: 0.012

SN 2015bn EVLA_X: 0.015

SN 2003dg EVLA_X: 0.012

SN 2007I EVLA_X: 0.012

SN 2004gn EVLA_X: 0.014

SN 2007rw EVLA_X: 0.012

SN 2000ew EVLA_X: 0.012

SN 2014ad EVLA_X: 0.013

SN 2002bm EVLA_X: 0.012

SN 2008aq EVLA_X: 0.012

SN 2005bh EVLA_X: 0.012

SN 2004gj EVLA_X: 0.012

SN 2002ji EVLA_X: 0.012

LSQ13abf EVLA_X: 0.011

SN 2014L EVLA_X: 0.014

SN 2004gk EVLA_X: 0.011

SN 1990B EVLA_X: 0.013

SN 2004cc EVLA_X: 0.013

SN 1987K EVLA_X: 0.042

PTF10bfz EVLA_X: 0.012

SN 1997dq EVLA_X: 0.013

SN 2011bm EVLA_X: 0.012

SN 2015bn EVLA_X: 0.014

SN 2003dg EVLA_X: 0.012

SN 2007I EVLA_X: 0.012

SN 2004gn EVLA_X: 0.014

SN 2007rw EVLA_X: 0.012

SN 2000ew EVLA_X: 0.013

SN 2014ad EVLA_X: 0.013

SN 2002bm EVLA_X: 0.012

SN 2008aq EVLA_X: 0.012

SN 2005bh EVLA_X: 0.012

SN 2004gj EVLA_X: 0.012

SN 2002ji EVLA_X: 0.012

LSQ13abf EVLA_X: 0.011

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