Experiment | End date |
Friend | Result | Problem |
Text |
RSG09 | 2018-02-07 | JIVE | Failure | None | No LL pol in subbands 0-1? |
N18L1 | 2018-02-22 | Jun Yang | Success | , , , , , , , , , , , , , , | None |
EG100A | 2018-02-23 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems |
EP106A | 2018-02-23 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EG100B | 2018-02-24 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EP106B | 2018-02-24 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EM128D | 2018-02-25 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EM131A | 2018-02-26 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EM131B | 2018-02-26 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
ES085A | 2018-02-28 | Jun Yang | Success | , , , , , , , , , , , , , , | Our antenna was off-source during UT 3:20 - 5:57, 6:40 - 7:39, 7:55 - 8:10
because of polar amplifier power-overload. |
EM132A | 2018-03-15 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EC057C | 2018-03-14 | Jun Yang | Success | , , , , , , , , , , , , , , | Forgot changing form=astro2 to form=astro3 in the experimental prc file. There
were some error messages due to the wrong request in the log file. Whilst, the actually
used mode was still astro3. So, the data should be fine. |
EB064B | 2018-03-14 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problem. |
EB064A | 2018-03-13 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problem. |
RP030C | 2018-03-13 | Jun Yang | Success | , , , , , , , , , , , , , , | The targets are some low-Dec sources and it was quite cloudy. So, the Onsala 20m
telescope had quite higher Tsys (>=150 K). |
N18K1 | 2018-03-12 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
GG084A | 2018-03-12 | Jun Yang | Success | , , , , , , , , , , , , , , | The target sources had quite low Elevation at Onsala. Because of the antenna
elevation limit (~7 deg), our telescope was off-source during 2:40 -- 3:50 UT. |
EK038B | 2018-03-09 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problem. |
EP106C | 2018-03-08 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problem. |
EM131C | 2018-03-07 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problem. |
EK038A | 2018-03-06 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
N18C1 | 2018-03-05 | Jun Yang | Success | , , , , , , , , , , , , , , | None |
EM117N | 2018-03-03 | Jun Yang | Success | , , , , , , , , , , , , , , | No known problems. |
EM117M | 2018-03-02 | Jun Yang | Minor failures | , , , , , , , , , , , , , , | Off-source during 9:53 -- 10:32 UT and 3:29 -- 3:56 UT due to the problem of
polar motor power overloaded. |
N18M1 | 2018-02-27 | Jun Yang | Success | , , , , , , , , , , , , , , | None |
RP030C | 2018-03-13 | Jun Yang | Success | , , , , , , , , , , , , , , | The Chopper-wheel calibration was used. Because of the slightly longer processing
time of the hot load in and out, the first 3-6 seconds data at the scan beginning were
affected and had high Tsys. So, these data should be flagged out in the post data
reduction. Note that the Tsys data were opacity-corrected. |
EB064A | 2018-03-13 | Jun Yang | Success | , , , , , , , , , , , , , , | The Chopper-wheel calibration was used. Because of the slightly longer processing
time of the hot load in and out, the first 3-6 seconds data at the scan beginning were
affected and had high Tsys (flagged out already in the antabfs file). So, these related
data should be flagged out in the post data reduction. Note that the Tsys data were
opacity-corrected (optical depth: 0.2-0.3). |
EB064B | 2018-03-14 | Jun Yang | Success | , , , , , , , , , , , , , , | The Chopper-wheel calibration was used. Because of the slightly longer processing
time of the hot load in and out, the first 3-6 seconds data at the scan beginning were
affected and had high Tsys (flagged out already in the antabfs file). So, these related
data should be flagged out in the post data reduction. Note that the Tsys data were
opacity-corrected (optical depth: 0.1-0.25). |
EC057C | 2018-03-14 | Jun Yang | Success | , , , , , , , , , , , , , , | The Chopper-wheel calibration was used. Because of the slightly longer processing
time of the hot load in and out, the first 3-6 seconds data at the scan beginning were
affected and had high Tsys (flagged out already in the antabfs file). So, these related
data should be flagged out in the post data reduction. Note that the Tsys data were
opacity-corrected (optical depth: 0.1-0.2). |
EM132A | 2018-03-15 | Jun Yang | Success | , , , , , , , , , , , , , , | The Chopper-wheel calibration was used. Because of the slightly longer processing
time of the hot load in and out, the first 3-6 seconds data at the scan beginning were
affected and had high Tsys (flagged out already in the antabfs file). So, these related
data should be flagged out in the post data reduction. Note that the Tsys data were
opacity-corrected (optical depth: 0.1-0.2). |
EG102B | 2018-01-17 | None | None | None | None |
ES085B | 2018-03-01 | None | None | None | None |
RP030B | 2018-02-05 | None | None | None | None |