ABCDEFGHIJKLMNOPQRSTUVWXYZ
1
Date:Wednesday, March 02, 2022Weather:
2
Observers:
Stefania, Sree, Sam, Julia and Madusha
Program:
Hector Commissioning
3
4
5
FieldRun rangeLocal timeReadOffset (arcsec)NotesDR Notes
6
Obs. Type
Exp. TimeSpeedZDSeeingN-SE-W
Rel or Abs.
7
8
Keeping the AAOmega and Spector spectograpgh focus settings from the previous night
9
10
150_m22_GAE_hexas_NS_EW_v3_OptMod_positive121:45Arc70Normal/Normal0.0FeAr1, FeAr2, CuAr1, CuAr2, He / ccd2=48k
11
2Arc60Normal/Normalccd2=40k
12
321:57Dome Flat50Normal/Normal0.0old dome screen. B=2000, R=1500, HB=3000 why signal is 10time lower than before:???? -Could the fact that the old dome screen is currently been painted cause this? or maybe the dome screen missed the telescope?
13
Telescope not focussed
14
422:30Object900Normal/Normal26.27cloudy, rotation -300,
15
522:50Object900Normal/Normal22.48cloudy, rotation -300, we lost guiding several times half way through
16
623:10Object900Normal/Normalcloudy, rotation -300, we lost guiding several times half way through
17
723:28Dome Flat50Normal/Normal14.8old dome screen. B=17k, R=20k, HB=20k
18
812:51BiasNormal/Normal33.09Bias to check after turning off fibres corresponding to hexabundle 'M'
19
901:02BiasNormal/NormalBias to check after turning off fibres corresponding to hexabundle 'M'
20
Hexabundle "M" is broken and excluded from the fibre_IFU table in observations for the rest of the commissioning run (from this point on)
21
1001:12Object1800Normal/Normalrotation -300Hexabundle "M" is broken and excluded from the fibre_IFU table in observations for the rest of the commissioning run (from this point on)
22
1101:45Dome Flat50Normal/Normal20.89new screen. B=20k, R=20k, HB=30k
23
1201:51Dome Flat90Normal/Normal22.704new screen. B=35k, R=35k, HB=saturated
24
1301:56Arc60Normal/Normal23.14
25
1402:07Object1800Normal/Normal25.19rotation -300. Not re-set to 0. Check drift of the rotator.
26
27
Telescope focus: 39.46
28
All sky fibers activated
29
150_m22_GC_hexas_NS_EW_v3_OptMod_negative1504:00Object1800Normal/Normal49.26rotation -300. Re-set to 0 first.All the sky fibres set to be active (type=S). This can be used as reference tlm
30
1604:37Object1800Normal/Normal56.9rotation -300. Re-set to 0 first.
31
1705:11Dome Flat50Normal/Normal64.42new screen. B=25k, R=25k, HB=saturated towards the blue endCount for CCD3 is changing for the same exposure. Test started. Screen was misaligned.
32
1805:19Dome Flat90Normal/Normalnew screen. B=40k, R=40k, HB=purposely saturated improve blue
33
1905:25Dome Flat50Normal/Normalnew screen. B=20k, R=25k, HB=saturated towards the blue end
34
2005:30Dome Flat30Normal/Normal64.1new screen. B=15k, R=15k, HB=30k
35
2105:40Dome Flat50Normal/Normal46.3new screen. B=20k, R=20k, HB=40k
36
2205:54Arc60Normal/Normal
37
23Flap Flat20Normal/Normal
38
2406:04Flap Flat40Normal/Normal51.0
39
40
2506:30Offset Sky200Normal/Normal16.50Twilight flat, 1Hr E. B=15k R=10k HB=20k
41
2606:37Offset Sky100Normal/Normal
Twilight flat, Offset 60E. E. B= 30k R=30k HB=49k
42
2706:42Offset Sky25Normal/Normal19.13
Twilight flat, Offset 60E. E. B=22 k R=22k HB=32k
43
2806:45Offset Sky12Normal/Normal19.6
Twilight flat, Offset 60E. E. B=22k R=22k HB=32k
44
2906:48Offset Sky6Normal/Normal
Twilight flat, Offset 60E. E. B=20 k R=18k HB=30k
45
46
30-3106:56Dark1800Normal/NormalLast dark (run 31) will finish at 08:02. So there might be some light contamination -- check
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122