Page History

...

Phase-only, continuum-only
- Amplitude attempts as future development possibility
Single pointing observations (no mosaics)
- Aggregate continuum self-calibration (gaincal combine=spw, applycal spwmap)
- Per-spw self-calibration (mapping from wide to narrow windows)
  - Need to understand conditions where per-spw will perform better
- Long and short baseline observations

...

Support for self-calibration within mosaics (interpolation over entire multiple fields/scans).

Pre-requisites:

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
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	E2E6.1.00085.S	uid://A002/Xd00f1f/Xca Selfcal Log	7	C1	1	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.S	uid://A001/X133d/X272b Selfcal Log	9	C3	1	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	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	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	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	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	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	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	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.S	uid://A001/X133d/X1b87 Selfcal Log	6	C-9	2	1	Jan 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

Test Suite:

TelescopeProject CodeMOUS/FSIDBand

Conf.

EBsTgtsVersionNotesOriginal Peak SNR

Selfcal Peak SNR

min solint

Original RMS

(mJy/bm or uJy/beam)

Final RMS

(mJy/bm or uJy/beam)

ALMA2019.1.01425

.S	uid://A001/

X1465/Xd60

X2d8/X287

Selfcal Log

7

6

C-

10

4

1

6

5

11

Novuses full MS

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 3uses full MSes, cont.dat, test case for spectral averaging

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''''''''''''Novdoes not use spectral averaging

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 3uses only continuum spw

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-

4

3

6

2

11

1

Dec 3polarization project, all data in a single combined MS, uses TDM

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

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-

311Novuses full MSes, cont.dat,

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,

point sources

DR_Tau Band_8: 126

DO_Tau Band_8: 38

DL_Tau

NGC_1068

Band_8:

61

38

FZ_Tau Band_8: 21

DR_Tau

NGC_1068_SBring

Band_8:

49

272

DO_Tau Band_8: 227

DL_Tau

NGC_1068_CH3OH

Band_8:

11

279

NGC

FZ_

1068

Tau Band_8:

77

21	DR_Tau Band_8: inf DO_Tau

NGC_1068_SBring

Band_8:

61

inf

NGC

DL_

1068_CH3OH

Tau Band_8:

11

int

NGC

FZ_

1068

Tau Band_8:

inf_EB

None

NGC

DR_

1068_SBring

Tau Band_8:

inf_EBNGC_1068_CH3OH

5.514

DO_Tau Band_8:

None

12.132

NGC

DL_

1068

Tau Band_8:

0

17.

322

709

NGC

FZ_

1068_SBring

Tau Band_8:

0

2.

301

403

NGC

DR_

1068_CH3OH

Tau Band_8:

0

2.

237

578

NGC

DO_

1068

Tau Band_8:

0

2.

266

227

NGC

DL_

1068_SBring

Tau Band_8:

0

2.

257

648

NGC

FZ_

1068_CH3OH

Tau Band_8:

0

2.

237

403

ALMA

ACA

2018

2017.1.

00510

00857.S

6C-9

uid://A001/X12c4/X21f

Selfcal Log

8

ACA

2

1

Dec 3

uses 3 TDM windows

fails due to beam, calonly would help here

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: None

NGC1333_IRAS_4A Band_6: 0.143

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

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	uid://A001/X146c/X26a	6	C-5	2	1
ALMA	2019.1.00261	uid://A001/X146c/X26f	6	C-5	2	2
ALMA	2019.1.00261

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

X263

6

C-8

ACA84Dec 3uses full MSes, cont.dat,

/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.S	uid://A001/X1465/X353f	6	C-9/10	1	1
ALMA	2018.1.01038

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

X133f/

X21f

X82

8ACA11Dec 3full MSes, cont.datAS_205A: 63AS_205A: 385AS_205A: infAS_205A: 24.770AS_205A: 4.102

6	C-5/6	8	11

VLA	13B-454	13B-454.sb29509255.eb29947371.56956.79185517361	C	C	1	1	Dec

3

6

M82, high DR, extended

SN2014J EVLA_C: 1506

SN2014J EVLA_C:

6515

6393

SN2014J EVLA_C: 17.00s

SN2014J EVLA_C: 0.

104

105	SN2014J EVLA_C: 0.

029

030

VLA

13B-454

13B-454.sb29105214.eb29105303.56758.17242523148

C

A

1

Nov

M82, high DR, extended

5932

Very long run time

SN2014J EVLA_C: 5933

SN2014J EVLA_C: 6078

SN2014J EVLA_C: 35.00s

SN2014J EVLA_C: 0.005

5

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

74

EVLA_X: 113

SN 2004gk EVLA_X: 37

SN 1990B

164

EVLA_X: 173

SN 2004cc

161

EVLA_X: 176

SN 1987K

540

EVLA_X: 661

PTF10bfz

422

EVLA_X: 421

SN 1997dq EVLA_X: 17

SN 2011bm

207

EVLA_X: 209

SN 2015bn

215

EVLA_X: 217

SN 2003dg

16

EVLA_X: 15

SN 2007I EVLA_X: 32

SN 2004gn

421

EVLA_X: 456

SN 2007rw EVLA_X: 18

SN 2000ew EVLA_X: 21

SN 2014ad

34

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 78

2002ji EVLA_X: 76

LSQ13abf EVLA_X: 9

SN 2014L

74

EVLA_X: 114

SN 2004gk EVLA_X: 37

SN 1990B

166

EVLA_X: 174

SN 2004cc

167

EVLA_X: 175

SN 1987K

603

EVLA_X: 732

PTF10bfz

431

EVLA_X: 429

SN 1997dq EVLA_X: 17

SN 2011bm

215

EVLA_X: 216

SN 2015bn

236

EVLA_X: 240

SN 2003dg

16

EVLA_X: 15

SN 2007I EVLA_X: 32

SN 2004gn

433

EVLA_X: 464

SN 2007rw

19

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

79

EVLA_X: 76

LSQ13abf EVLA_X: 9

SN 2014L

inf_EB

EVLA_X: 9.00s

SN 2004gk

None

EVLA_X: 81.00s

SN 1990B

81.00s

EVLA_X: inf_EB

SN 2004cc

int

EVLA_X: inf_EB

SN 1987K

int

EVLA_X: 18.00s

PTF10bfz EVLA_X: 39.00s

SN 1997dq

81.00s

EVLA_X: inf_EB

SN 2011bm EVLA_X: int

SN 2015bn EVLA_X: 39.00s

SN 2003dg

inf

EVLA_

EB

X: None

SN 2007I EVLA_X: inf_EB

SN 2004gn EVLA_X: inf_EB

SN 2007rw

162.00s

EVLA_X: inf_EB

SN 2000ew

162.00s

EVLA_X: inf_EB

SN 2014ad

None

EVLA_X: 81.00s

SN 2002bm EVLA_X: 39.00s

SN 2008aq EVLA_X: None

SN 2005bh EVLA_X: None

SN 2004gj

39

EVLA_X: 81.00s

SN 2002ji EVLA_X: 162.00s

LSQ13abf EVLA_X: None

SN 2014L

22

EVLA_X: 0.014

SN 2004gk

11

EVLA_X: 0.011

SN 1990B

14

EVLA_X: 0.013

SN 2004cc

14

EVLA_X: 0.013

SN 1987K

56

EVLA_X: 0.046

PTF10bfz

12

EVLA_X: 0.012

SN 1997dq

14

EVLA_X: 0.013

SN 2011bm

12

EVLA_X: 0.012

SN 2015bn

15

EVLA_X: 0.015

SN 2003dg

12

EVLA_X: 0.012

SN 2007I

12

EVLA_X: 0.012

SN 2004gn

15

EVLA_X: 0.014

SN 2007rw

12

EVLA_X: 0.012

SN 2000ew

14

EVLA_X: 0.012

SN 2014ad EVLA_X: 0.013

SN 2014ad 13

SN 2002bm

12

EVLA_X: 0.012

SN 2008aq

12

EVLA_X: 0.012

SN 2005bh

12

EVLA_X: 0.012

SN 2004gj

12

EVLA_X: 0.012

SN 2002ji

12

EVLA_X: 0.012

LSQ13abf

11

EVLA_X: 0.011

SN 2014L

22

EVLA_X: 0.014

SN 2004gk

11

EVLA_X: 0.011

SN 1990B

13

EVLA_X: 0.013

SN 2004cc

14

EVLA_X: 0.013

SN 1987K

51

EVLA_X: 0.042

PTF10bfz

12

EVLA_X: 0.012

SN 1997dq

14

EVLA_X: 0.013

SN 2011bm

12

EVLA_X: 0.012

SN 2015bn

14

EVLA_X: 0.014

SN 2003dg

12

EVLA_X: 0.012

SN 2007I

12

EVLA_X: 0.012

SN 2004gn

15

EVLA_X: 0.014

SN 2007rw

12

EVLA_X: 0.012

SN 2000ew

14

EVLA_X: 0.013

SN 2014ad

13

EVLA_X: 0.013

SN 2002bm

12

EVLA_X: 0.012

SN 2008aq

12

EVLA_X: 0.012

SN 2005bh

12

EVLA_X: 0.012

SN 2004gj

12

EVLA_X: 0.012

SN 2002ji

12

EVLA_X: 0.012

LSQ13abf

11

EVLA_X: 0.011

Space shortcuts

Page tree

Versions Compared

Old Version 40

New Version Current

Key