On this page we summarize requested calibrator monitoring by VLBA observers per semester, starting with 21A. All collected data is publicly accessible through https://data.nrao.edu/ under project codes TCAL0009 or TPOL0003.


Observing Semester 23B

Proposal
Code
Legacy
Code
Type of Requestdate of VLBA
observation
calibrators
to observe
BandsSB iddate of VLA
observation
23B-062BR253VLBA Triggered, VLA polcal requestedNever triggered3C279, J2136+0041, J2202+4216

K (21.812-22.324 GHz on the VLBA)

44530999

BM546

Continuation of BL286 from 21B

(6 hours of EVPA calibrators every 4-6 months for 3 years)

Monthly for 3 yearssame as for BL273 (1828+487, 1803+784, 1807+698, 0212+735, 2200+420, 2351+456, 1901+319, 2201+315, 0208+106, 0234+285, 0333+321, J2355+4950, 0430+052, 3C 138, 0415+379)X - Q37501394
23B-137BL310EVPA measurements close to time of observation2023Dec05BL Lac and DA193 (both in TPOL0003)K (21512-24024 MHz)44867309


Observing Semester 23A

Proposal
Code
Legacy
Code
Type of Requestdate of VLBA
observation
calibrators
to observe
BandsSB iddate of VLA
observation
23A-198BN064AVLBA Triggered, VLA polcal requested

BN064A1, 2023Oct28

BN064A2, 2024May29

BN064A3, 2024Nov15

3C279 (J1256-0547) and 3C286 (J1331+3030)

C (4412-4668,6540-6796 MHZ)

K (23312-23824 MHz)

Q (42912-43424 MHz)

44546405

2023-11-14

2024-05-24

2024-11-21

23A-198BN064CVLBA Triggered, VLA polcal requested

BN064C1, 2024Jan30

BN064C2, 2024Jul22


J0555+3948

C (4412-4668,6540-6796 MHZ)

U (15040-15552 MHz)

K (23312-23824 MHz)

Q (42912-43424 MHz)

450409782024-09-01








Observing Semester 22B

Proposal Code

Legacy CodeType of Request

date of VLBA

observation

calibrators

to observe

BandsSB id

date of VLA

observation

22B-260BT154

within 10 days of VLBA observations.

BT154A  2022 Oct 18

BT154B  2023 Jan24

OJ287, 0528+134, and 0235+164

K,U,C

(23.5-24 GHz, 15-15.5 GHz, 4.4-6.7GHz)

42608628

2022 Oct 20

2023 Jan 17

22B-183BL299within 10 days of VLBA observationsBL299A 2022 Sep 240133+476, 0736+017, 0814+425, 1611+343, 1633+382, 1641+399, 2201+315

8176, 8304, 8432, 8560, 11974, 12104, 12232, 12360, 15176,

 15304, 15432, 15560 MHz

42764486

42768214

2022 Sep 26

2022 Sep 26

22B-120BL298Sep 25 to Oct 10

BL298A  2022 Oct 01

BL298B  2022 Oct 02

NRAO150, BLLac, 2023+335 (in theTPOL0003 monitoring list), 3C41811976,12104,12232,12360,  15176,15304,15432,15560,  23376,23504,23632,23760,  42976,43104,43232,43360 MHz

42779727






42783688

Repeat for 42779727:
42856397

43831036

43831242 / 43831546 (linked)

2022 Sep 29 (CBE error last two scans no data; only Q and K will be able to calibrate)

2022 Sep 27



2022 Oct 10


Observing Semester 21B

Proposal
Code
Legacy
Code
Type of Requestdate of VLBA
observation
calibrators
to observe
BandsSB iddate of VLA
observation
21B-011BT152VLA observation within 4 days of each VLBA observation / alternatively 2 week cadence between first and last VLBA observation

2021-10-07

2021-10-08

2021-10-31

2022-01-23

2022-05-26

2022-06-18

2-22-06-19

Complete.

OQ208, 1144+402, 1308+326, 1331+305=3C286C, Ku40033000

2021-08-22

2021-08-24

2021-10-09

2021-10-24

2021-11-12

2021-11-27

2021-12-28

2022-01-12

2022-01-27

2022-02-13

2022-04-20

2022-05-05

2022-05-22

21B-053BL2866 hours of EVPA calibrators every 4-6 months for 3 years.Monthly for 3 years.same as for BL273 (1828+487, 1803+784, 1807+698, 0212+735, 2200+420, 2351+456, 1901+319, 2201+315, 0208+106, 0234+285, 0333+321, J2355+4950, 0430+052, 3C 138, 0415+379)X - Q37501394

2022-02-27

2022-06-02

2022-09-02

2022-12-17

21B-086BH233
EVPA calibrators OJ287 (and 0235+164) at both K and Q bands within 20 days of VLBA observations.

BH233A 2022Jan20

BH233B 2022Apr15

BH233C (Interval 75 days)

OJ287 and 0235+164;

Note OJ287 at Q-band shows two polarization components beating against each other.

OJ287: K: ~-50 deg. (~3%)
              Q: ~-35 deg. (~6%)

0235+164: K: ~29 deg (~2%)
                    Q: ~36 deg. (~24%)

K, Q41029961

2022-01-22

2022-01-22

2022-05-05

21B-366BR247Observed: 3C286 against J1159+2914, J1310+3220, J0927+3902, J1642+3948, J1602+3326 (weakly pol.), J1415+1320 (unpol.; 0.7-0.6 Jy)

Ku, Q41145606

2022-01-22

Observing Semester 21A

Proposal
Code
Legacy
Code
Type of Requestdate of VLBA
observation
calibrators
to observe
SB iddate of VLA
observation
21A-195BM509Joint VLA proposal will handle EVPA - Triggered



21A-095BA142VLA EVPA requested if target is bright enough for VLBA polarimetry within 10d of VLBA obs. - Triggered



21A-289BR236VLA observations within 10d of VLBA observations



Observing Semester 20B

Proposal
Code
Legacy
Code
Type of Requestdate of VLBA
observation
calibrators
to observe
BandsSB iddate of VLA
observation

SC030needed close in time (2-3 weeks) 15 GHz observations with JVLA2020-07-30J1310+3220
374074272020-08-29

SC030
2020-12-15J1310+3220
374074272020-11-16

SC030
2021-01-03J1310+3220
392149622021-01-06

SC030

J1310+3220L - Q374074272021-02-17

BH227

J0713+4349, J0854+2006, J1310+3220, J1331+3030X, Ku, K391856542020-12-19

BH227

J0713+4349, J0854+2006, J1310+3220, J1331+3030X, Ku, K391856542021-01-18

BH227

J0713+4349, J0854+2006, J1310+3220, J1331+3030X, Ku, K391856542021-02-25

BH227

J0713+4349, J0854+2006, J1310+3220, J1331+3030X, Ku, K391856542021-03-30

BH227

J0713+4349, J0854+2006, J1310+3220, J1331+3030X, Ku, K391856542021-05-02
20B-274BM506

Two VLA observations per year for three years.


Monthly





SB provided by PI, target date 2021/03/01 - 2021/04/30
J0854+2006, J1058+0133, J1159+2914, J1256-0547, J1512-0905Q

39347876

(released 2021/03/30)

2021-04-25


SB provided by PI, target date 2021/09/15 - 2021/11/15
J0854+2006, J1058+0133, J1159+2914, J1256-0547, J1512-0905Q

39359007

(released 2022/01/20)

2022-01-21


Copy of previous SB. Count 3, interval 135.
J0854+2006, J1058+0133, J1159+2914, J1256-0547, J1512-0905Q42790130

2022-10-22



Observing Semester 17B

Proposal Code

Legacy CodeType of Request

date of VLBA

observation

calibrators

to observe

BandsSB id

date of VLA

observation

17B-228BI043

One observation within a month of the VLBA observations.

A typical full-polarization continuum observation setup, with rms~3-5mJy/beam,

which should allow a 10-sigma detection of polarized flux of 3C48

(with Fpol ~ 0.046 Jy/beam in Q-band).

BI043A  ?

BI043B  2022/02/14

BI043C  2022/02/13

J0359+5057,

J0137+331 (AKA 3C48)

43 GHz41246468Whenever ready.
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