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...

  • 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:

TelescopeProject Code

MOUS/FSID &

Selfcal Log

Band

Conf.


EBsTgtsVersionNotesOriginal Peak SNR

Selfcal Peak SNR

min solint

Original RMS

(mJy/bm or uJy/beam)

Final RMS

(mJy/bm or uJy/beam)

ALMAE2E6.1.00085.S

uid://A002/Xd00f1f/Xca

Selfcal Log

7C111Feb 14

spec scan project

cont and line morphology different

flux resolved out (selfcal seems doing well)

G31.41+0.31: 189G31.41+0.31: 516G31.41+0.31: inf_EBG31.41+0.31: 0.00994G31.41+0.31: 0.00368
ALMA2018.1.00962.S

uid://A001/X133d/X272b

Selfcal Log

9C311Feb 14flux resolved out (selfcal seems doing well)NGC6334I: 58NGC6334I: 144NGC6334I: inf_EBNGC6334I: 0.052NGC6334I: 0.021
ALMA2017.A.00042.T

uid://A001/X1306/X5e

Selfcal Log

5C1/211Feb 14cont and line morphology different (different centroid)iras16293-2422: 306iras16293-2422: 1074iras16293-2422: 90.72siras16293-2422: 0.00238iras16293-2422: 0.00069
ALMA2017.1.00855.S

uid://A001/X1284/X10c9

Selfcal Log

3C621Feb 14
Uranus: 200Uranus: 833Uranus: infUranus: 0.000301Uranus: 0.000075
ALMA2017.1.00670.S

uid://A001/X1284/X20e0

Selfcal Log

7C411Feb 14
Io: 148Io: 285Io: infIo: 0.0072Io: 0.0036
ALMA2017.1.00661.S

uid://A001/X128e/X222

Selfcal Log

4ACA81Feb 14poor uv coverage (PSF sidelobe)NGC6334I: 101NGC6334I: 704NGC6334I: 90.72sNGC6334I: 0.035NGC6334I: 0.004
ALMA2016.1.00577.S

uid://A001/X87c/X10d

Selfcal Log

6ACA41Feb 14poor uv coverage (PSF sidelobe)G333.6-0.2: 47G333.6-0.2: 216G333.6-0.2: inf_EBG333.6-0.2: 0.104G333.6-0.2: 0.028
ALMA2015.1.00150.S

uid://A001/X2f6/X265

Selfcal Log

7C1/211Feb 14
NGC_6334I: 126NGC_6334I: 395NGC_6334I: infNGC_6334I: 0.0346NGC_6334I: 0.0115
ALMA2018.1.01055.L

uid://A001/X133d/X19d5

Selfcal Log

6C731Jan 12

concentric rings (protoplanetary disk) captured better by selfcal

different cont and line morphology

HD163296: 366HD163296: 801HD163296: infHD163296: 44.7HD163296: 21.3
ALMA2018.1.00659.L

uid://A001/X133d/X1284

Selfcal Log

6C5/621Jan 12Field center differ across EBs by 376 microarcsec (beyond the 200 microarcsec criteria) but maybe OK if this has large proper motionR_Hya: 196R_Hya: 1201R_Hya: intR_Hya: 167R_Hya: 42.4
ALMAE2E8.1.00062.S

uid://A001/X1587/X51b

Selfcal Log

6ACA32Jan 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

ALMA2019.1.00847.S

uid://A001/X1467/X264

Selfcal Log

7ACA35Jan 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

ALMA2019.1.01709.S

uid://A001/X1465/X435

Selfcal Log

6C-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: 0.030
ALMA2019.1.01709.S

uid://A001/X1465/X431

Selfcal Log

3C-511Jan 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
ALMA2019.1.01197.S

uid://A001/X1465/X15aa

Selfcal Log

6C-311Jan 5

All cont spw

Continuum source with lensed morphology

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

PJ011646.8: 0.1


PJ011646.8: 0.09
ALMA2019.1.00463.S

uid://A001/X146a/Xf

Selfcal Log

6C-611Jan 5

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

continuum source off phase center


BHR7: 322BHR7: 742BHR7: 42.34sBHR7: 0.072BHR7: 0.043
ALMA2019.1.01425.Suid://A001/X1465/Xd606C-1015Jan 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


ALMA2017.1.01413.S

uid://A001/X1273/X7bc

Selfcal Log


6C-425Jan 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


ALMA2019.1.00261.L

uid://A001/X146c/X26f

Selfcal Log


6C-522Jan 20spectrally 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.S

uid://A001/X133d/X1b87

Selfcal Log


6C-921Jan 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


ALMA2015.1.01503.S

uid://A001/X2d8/X287

Selfcal Log


7C-4611Jan 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


ALMA2018.1.00962.S

uid://A001/X133d/X2727


9C-311Jan 20

uses full MSes, cont.dat,

extended emission

NGC6334I: 46

NGC6334I: 106

NGC6334I: int

NGC6334I: 62.618

NGC6334I: 28.644

ALMA2017.1.00586.S

uid://A001/X1284/X20cf

Selfcal Log


8C-2?32Jan 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


ALMA2018.1.00510.S

uid://A001/X133d/X1e68

Selfcal Log


6C-921Jan 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: 129


NGC1333_IRAS_4A Band_6: None


NGC1333_IRAS_4A Band_6: 0.143


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


ALMA2013.1.00879.S

uid://A001/X11f/X7f

Selfcal Log


6C-321Jan 20










ALMA

2017.1.00419.S

uid://A001/X1284/X149

Selfcal Log

6C-5/6120Jan 25Mix of wide and narrow windows




ALMA2017.1.00449.S

uid://A001/X1289/Xa6

Selfcal Log

7C-5/611Jan 22Mostly wide windows




ALMA2017.1.00449.S

uid://A001/X1289/Xaa

Selfcal Log

6C-5/611Jan 22Mostly wide windows




ALMA2017.1.00449.S

uid://A001/X1296/X7a5

Selfcal Log

3C-811Jan 22Mostly wide windows




ALMA2018.1.01119.S

uid://A001/X133d/X2c5e

Selfcal Log

6C-651Jan 22Mostly wide windows




ALMA2013.1.00937.S

uid://A001/X144/X189

Selfcal Log

6C-626Jan 22Mostly wide windows




ALMA2019.1.00218.S

uid://A001/X1465/X365e

Selfcal Log

6C-21100Jan 22Mostly wide windows




ACA2017.1.00857.S

uid://A001/X12c4/X217

Selfcal Log


8ACA84Jan 20

uses full MSes, cont.dat,

point sources

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


ACA2017.1.00857.S

uid://A001/X12c4/X21f

Selfcal Log

8ACA11Jan 20

full MSes, cont.dat

point source

AS_205A: 63AS_205A: 385AS_205A: infAS_205A: 24.770AS_205A: 4.102
ALMA2019.1.00261uid://A001/X146c/X26a6C-521






ALMA2019.1.00261uid://A001/X146c/X26f6C-522






ALMA2019.1.00261uid://A001/X146c/X2636C-8/92(5)2






ALMA2019.1.00261uid://A001/X146c/X2596C-8/91(4)2






ALMA2019.1.00255.Suid://A001/X1465/X35416C-611






ALMA2019.1.00255.Suid://A001/X1465/X353f6C-9/1011






ALMA2018.1.01038.Suid://A001/X133f/X826C-5/6811

Test Suite:

TelescopeProject CodeMOUS/FSIDBandConfigurationEBsTargetsVersionNotesOriginal Peak SNR

Selfcal Peak SNR

min solint

Original RMS

(mJy/bm or uJy/beam)

Final RMS

(mJy/bm or uJy/beam)

ALMA2019.1.01425.Suid://A001/X1465/Xd606C-1015uses full MS

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

ALMA2017.1.01413.Suid://A001/X1273/X7bc6C-425Novuses full MSes, cont.dat, test case for spectral averaging

L1527-IRS: 471

TMC1A: 411

IRAS_04302+2247: 158

L1489IRS: 115

TMC1: 211

L1527-IRS: 1729

TMC1A: 2002

IRAS_04302+2247: 322

L1489IRS: 135

TMC1: 295

L1527-IRS: 30.24s

TMC1A: 30.24s

IRAS_04302+2247: inf_EB

L1489IRS: inf

TMC1: 30.24s

L1527-IRS: 0.214

TMC1A: 0.299

IRAS_04302+2247: 0.131

L1489IRS: 0.058

TMC1: 0.073

L1527-IRS: 0.061

TMC1A: 0.065

IRAS_04302+2247: 0.075

L1489IRS: 0.054

TMC1: 0.057

ALMA''''''''''''Dec 3does 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-921Novuses only  continuum spw

IRAS2A: 213

IRAS2A: 959

IRAS2A: inf

IRAS2A: 0.114

IRAS2A: 0.043

ALMA2015.1.01503.Suid://A001/X2d8/X2877C-4611Novpolarization project, all data in a single combined MS, uses TDM

Per26: 214

Per18: 162

Per21: 193

Per11: 255

Per14: 253

Per50: 213

Per2: 151

Per5: 279

Per41: 160

Per29: 232

Per26: 1154

Per18: 584

Per21: 716

Per11: 1045

Per14: 799

Per50: 1144

Per2: 397

Per5: 1095

Per41: 286

Per29: 1171

Per26: int

Per18: int

Per21: int

Per11: int

Per14: int

Per50: int

Per2: int

Per5: int

Per41: int

Per29: int

Per26: 1.019

Per18: 0.529

Per21: 0.382

Per11: 0.635

Per14: 0.345

Per50: 0.579

Per2: 0.516

Per5: 0.795

Per41: 0.152

Per29: 0.695

Per26: 0.232

Per18: 0.169

Per21: 0.126

Per11: 0.177

Per14: 0.129

Per50: 0.137

Per2: 0.216

Per5: 0.231

Per41: 0.098

Per29: 0.160

ALMA2018.1.00962.Suid://A001/X133d/X27279C-311Novuses full MSes, cont.dat,

NGC6334I: 46

NGC6334I: 106

NGC6334I: int

NGC6334I: 62.618

NGC6334I: 28.644

ALMA2017.1.00586.Suid://A001/X1284/X20cf8C-2?32Dec 3uses full MSes, cont.dat,

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

ALMA2018.1.00510.S6C-921Dec 3uses 3 TDM windows

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: 129

NGC1333_IRAS_4A Band_6: None

NGC1333_IRAS_4A Band_6: 0.143

NGC1333_IRAS_4A Band_6: 0.143

ALMA-ACA2017.1.00857.Suid://A001/X12c4/X2178ACA84Novuses full MSes, cont.dat,

DR_Tau: 109

DO_Tau: 28

DL_Tau: 27

FZ_Tau: 22

DR_Tau: 285

DO_Tau: 244

DL_Tau: 285

FZ_Tau: 24

DR_Tau: inf_EB

DO_Tau: inf

DL_Tau: inf_EB

FZ_Tau: None

DR_Tau: 6.404

DO_Tau: 16.446

DL_Tau: 25.543

FZ_Tau: 2.394

DR_Tau: 2.450

DO_Tau: 2.086

DL_Tau: 2.621

FZ_Tau: 2.155

ALMA-ACA2017.1.00857.Suid://A001/X12c4/X21f8ACA11Dec 3full MSes, cont.datAS_205A: 63AS_205A: 385AS_205A: infAS_205A: 24.770AS_205A: 4.102





















VLA13B-45413B-454.sb29509255.eb29947371.56956.79185517361CC11
Nov
Dec 6M82, high DR, extended
1015443817s16846

SN2014J EVLA_C: 1506

SN2014J EVLA_C: 6393SN2014J EVLA_C: 17.00sSN2014J EVLA_C: 0.105

SN2014J EVLA_C: 0.030

VLA


13B-45413B-454.sb29105214.eb29105303.56758.17242523148CA11Nov

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


SN2014J EVLA_C: 0.005

59325


VLA15A-370

15A-370.sb30976913.eb30980293.57204.36680753472

15A-370.sb30976913.eb30978455.57203.32521244213

Ka, QA21
Nov
Dec 3compact, low DR
A

L1157 EVLA_KA:

 

28

L1157 EVLA_Q: 19

A: -

L1157 EVLA_KA: 27

L1157 EVLA_Q:

-

19

L1157 EVLA_KA

A

: None

L1157 EVLA_Q: None

A: 12

Q: 19

L1157 EVLA_KA: 0.011

L1157 EVLA_Q: 0.020

L1157 EVLA_KA: 0.011

L1157 EVLA_Q: 0.020

A: -

Q: -

VLA17B-18817B-188.sb35564398.eb35590549.58363.10481791667S,C,Ku,K,KaC12Dec 3compact 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


VLATDRW0001TDRW0001.sb35624494.eb35628826.58395.23719237269SD11
Nov
Dec 3extended, high
DR3097491225s4730
DR

3C75 EVLA_S: 3815

3C75 EVLA_S: 6733

3C75 EVLA_S: 25.00s

3C75 EVLA_S: 0.038

3C75 EVLA_S: 0.022

VLA16B-42716B-427.sb33651951.eb34041883.57963.57173581018L,S,C,X,K, QC11
Novmultiband

L: 362

S: 214

C: 104

X: 792

K: 424

Q: 222

L: 344

S: 212

C: 105

X: 737

K: 590

Q: 534

L: inf

S: inf_EB

C: inf_EB

X: 72s

K: 42s

Q: int

L: 94

S: 69

C: 147

X: 27

K: 59

Q: 75

L: 99

S: 69

C: 148

X: 29

K: 47

Q: 73

Dec 3multiband

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

VLA20A-39020A-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		KaC51
Nov
Dec 3point source, low dec
162277129s5149

TWHya EVLA_KA: 164

TWHya EVLA_KA: 278

TWHya EVLA_KA: 129.00s

TWHya EVLA_KA: 0.005

TWHya EVLA_KA: 0.005

VLA21A-17821A-178.sb39472833.eb39589695.59326.113018460645XD121Novvariety 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

2004gn 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

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:

SN 2011bm

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

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

13

EVLA_X: 0.013

SN 2002bm

12

EVLA_X: 0.012

SN 2008aq EVLA_X: 0.012

SN 2008aq 12

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 EVLA_X: 0.012

SN 2007rw 12

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