...
- 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):
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 | 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 | 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 | 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 | 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 | 7 | C4 | 1 | 1 | Feb 14 | Io: 148 | Io: 285 | Io: inf | Io: 0.0072 | Io: 0.0036 | |
| ALMA | 2017.1.00661.S | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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 | 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.S | 7 | C-4 | 6 | 11 | 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 | 9 | C-3 | 1 | 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 |
Test Suite:
Selfcal Peak SNR
min solint
Original RMS
(mJy/bm or uJy/beam)
Final RMS
(mJy/bm or uJy/beam)
| .S |
| 8 |
| C- |
| 2? | 3 | 2 | Jan 20 |
uses full |
L1448IRS3B: 85
L1448IRS1: 97
L1448IRS3C: 90
Per-emb-17: 100
Per-emb-22: 107
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 |
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
| .S |
| 6 | C- |
| 9 | 2 |
| 1 |
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
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
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
| 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 |
| ALMA | 2013.1.00879.S | 6 | C-3 | 2 | 1 | Jan 20 | |||||||
ALMA | 2017.1.00419.S | 6 | C-5/6 | 1 | 20 | Jan 25 | Mix of wide and narrow windows | ||||||
| ALMA | 2017.1.00449.S | 7 | C-5/6 | 1 | 1 | Jan 22 | Mostly wide windows | ||||||
| ALMA | 2017.1.00449.S | 6 | C-5/6 | 1 | 1 | Jan 22 | Mostly wide windows | ||||||
| ALMA | 2017.1.00449.S | 3 | C-8 | 1 | 1 | Jan 22 | Mostly wide windows | ||||||
| ALMA | 2018.1.01119 |
| .S |
| 6 | C- |
| 6 | 5 | 1 | Jan 22 | Mostly wide windows | |||||||||
| ALMA | 2013.1.00937.S | 6 | C-6 | 2 | 6 | Jan 22 | Mostly wide windows | ||||||
| ALMA | 2019.1.00218 |
IRAS2A: 213
IRAS2A: 959
IRAS2A: inf
IRAS2A: 0.114
IRAS2A: 0.043
| .S |
| 6 |
| C- |
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
| 2 | 1 | 100 | Jan 22 | Mostly wide windows | |||||||||
| ACA | 2017.1.00857.S | 8 | ACA | 8 | 4 | Jan 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 | |
| ACA | 2017.1.00857.S | 8 | ACA | 1 | 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 | 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.S | uid://A001/X1465/X353f | 6 | C-9/10 | 1 | 1 | |||||||
| ALMA | 2018.1.01038 |
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
NGC6334I: 46
NGC6334I: 106
NGC6334I: int
NGC6334I: 62.618
NGC6334I: 28.644
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
| .S | uid://A001/ |
| X133f/ |
| X82 |
| 6 | C-5/6 | 8 | 11 | ||||||||||
| VLA | 13B-454 | 13B-454.sb29509255.eb29947371.56956.79185517361 | C | C | 1 | 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 | 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 | 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 |
A: -
L1157 EVLA_KA: 27 L1157 EVLA_Q: |
19 | L1157 EVLA_KA |
: 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: -| 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 | 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 |
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
| 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 |
C: inf_EB
X: 72s
K: 42s
Q: int
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 |
L: 94
S: 69
C: 147
X: 27
K: 59
Q: 75
L: 99
S: 69
C: 148
X: 29
K: 47
Q: 73| 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 | 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: |
SN 2004cc int
SN 1987K int
PTF10bfz39.00s 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 |
SN 2014ad None
SN 2002bm2002bm 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 |
SN 2004gk 11
SN 1990B 14
SN 2004cc 14
SN 1987K 56
PTF10bfz 12
SN 1997dq 14
SN 2011bm 12
SN 2015bn 15
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
LSQ13abf 11
SN 2014L 22
SN 2004gk 11
SN 1990B 13
SN 2004cc 14
SN 1987K 51
PTF10bfz 12
SN 1997dq 14
SN 2011bm 12
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 |
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
LSQ13abf 11