Versions Compared

Old Version 18

changes.mady.by.user John Tobin

Saved on

compared with

New Version Current

changes.mady.by.user John Tobin

Saved on

Key

  • This line was added.
  • This line was removed.
  • Formatting was changed.

...

  • 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

Test Suite:

TelescopeProject CodeMOUS/FSIDBandConfigurationEBsTargetsNotesOriginal 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

X133d/X1e68

Selfcal Log


6C-
10
921
5uses full MS

L1448IRS3B: 85

L1448IRS1: 97

L1448IRS3C: 90

Per-emb-17: 100

Per-emb-22: 107

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: 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

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-425uses full MSes, cont.dat, test case for spectral averaging

L1527-IRS: 442

TMC1A: 389

IRAS_04302+2247: 148

L1489IRS: 107

TMC1: 209

L1527-IRS: 1717

TMC1A: 2003

IRAS_04302+2247: 163

L1489IRS: 134

TMC1: 294

L1527-IRS: 30.24s

TMC1A: 30.24s

IRAS_04302+2247: None

L1489IRS: inf

TMC1: 30.24s

L1527-IRS: 0.228

TMC1A: 0.315

IRAS_04302+2247: 0.140

L1489IRS: 0.063

TMC1: 0.074

L1527-IRS: 0.062

TMC1A: 0.065

IRAS_04302+2247: 0.140

L1489IRS: 0.054

TMC1: 0.057

ALMA''''''''''''does 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-522spectrally 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

X1465/X365e

Selfcal Log

6C-
9
21
uses only  continuum spw
100Jan 22Mostly wide windows




ACA2017.1.00857

IRAS2A: 213

IRAS2A: 959

IRAS2A: inf

IRAS2A: 0.114

IRAS2A: 0.043

ALMA2015.1.01503
.S

uid://A001/

X2d8

X12c4/

X287

X217

7C-4611polarization 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

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






ALMA2019.1.00261

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.S
uid://A001/
X133d
X146c/
X2727
X26f
9
6C-
311uses full MSes, cont.dat,

NGC6334I: 46

NGC6334I: 106

NGC6334I: int

NGC6334I: 62.618

NGC6334I: 28.644

522






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






ALMA2019.1.00261
ALMA-ACA2017.1.00857.S
uid://A001/
X12c4
X146c/
X217
X259
8
6
ACA
C-8/91(4
uses full MSes, cont.dat,
)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

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: 2.1551015443817s16846





















VLA13B-45413B-454.sb29509255.eb29947371.56956.79185517361CC11Dec 6M82, high DR, extended

SN2014J EVLA_C: 1506

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

SN2014J EVLA_C: 0.030

59325

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


VLA15A-370

15A-370.sb30976913.eb30980293.57204.36680753472

15A-370.sb30976913.eb30978455.57203.32521244213

Ka, QA21Dec 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,
C,Ku,K,Ka
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

C12compact at HF, compact+extended at LF, multiband

S: 1357

C: 966

U: 174

K: 101

A: 70

S: -

C: 1104

U: 259

K: 208

A: 115

S: None

C: inf

U: 33s

K: int

A: inf

S: 29

C: 26

U: 72

K: 86

A: 83

S: -

C: 22

U: 52

K: 51

A: 59


VLATDRW0001TDRW0001.sb35624494.eb35628826.58395.23719237269SD11Dec 3extended, high DR
3097491225s47

3C75 EVLA_S: 3815

3C75 EVLA_S: 6733

3C75 EVLA_S: 25.00s

3C75 EVLA_S: 0.038

3C75 EVLA_S: 0.022

30

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

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		KaC51Dec 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

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

2014L 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 EVLA_X: inf_EB

SN 1987K EVLA_X: 18.00s

PTF10bfz EVLA_X:

SN 2004cc int

SN 1987K int

PTF10bfz

39.00s

SN 1997dq

81.00s

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

2007I

2000ew EVLA_X: inf_EB

SN

2004gn inf_EBSN 2007rw 162

2014ad EVLA_X: 81.00s

SN

2000ew 162.00s

SN 2014ad None

SN 2002bm

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 EVLA_X: 0.011

SN 2004gk 11

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 EVLA_X: 0.012

SN 2003dg 12

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

12

EVLA_X: 0.012

SN 2005bh EVLA_X: 0.012

SN 2005bh 12

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

SN 1987K 51

PTF10bfz 12

SN 1997dq 14

SN 2011bm 12

SN 2015bn 14

SN 2003dg 12

SN 2007I 12

SN 2004gn 15

SN 2007rw 12

SN 2000ew 14

SN 2014ad 13

SN 2002bm 12

SN 2008aq 12

SN 2005bh 12

SN 2004gj 12

SN 2002ji 12

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

LSQ13abf 11