GTAC Observation Log

1. Date : 21/05/2023
2. Observation Sr. No. : 15430
3. Observer : harish k vedantham, Sanne Bloot
4. Observer\'s Email : vedantham@astron.nl, bloot@astron.nl
5. Project Name : A volume limited survey of the coldest brown dwarfs- a bridge to exoplanet magnetism
6. Project Code : 44_108
7. Operator(s) : Navnath, Sachin, Surender
8. Command File : /data1/gtac/cmd/44_108/44_108_21May2023_1200_cmd.py
9. LTA File : /gsbifrdata1/21may/44_108_21may2023_b4_gsb.lta, /gwbifrdata2/21may/44_108_21may2023_b4_gwb.lta
10. LogFlag File :  

ANTENNA SETTINGS :

11. RF Band(MHz) & Solar Attn(dB)- RF1 : 591 MHz ,RF2 : 591 MHz, SA1 : 0 dB, SA2 : 0 dB
12. Ist LO (MHz) & IVth LO (MHz): ILO1 : 540 MHz, ILO2 : 540MHz , IVLO1 : 51 MHz, IVLO2 : 51 MHz 
13. IF Attn(dB) , IF BW(MHz) & IF ALC : IF-CH1 : 4+14 dB, 32 MHz,ON, IF-CH2 : 4+14 dB, 32 MHz,ON

GSB SETTINGS :

14. GSB Host : gsbm1_shivneri
15. GSB Mode : Realtime
16. GSB LTA : 8
17. GSB CTRL : ONLINE/TGC
18. GSB Fstop : ON
19. GAIN EQ : ON
20. Stokes : Full_Stokes
21. Beam - 1 : OFF
22. Beam - 2 : OFF
23. ACQ BW : 33.333333 MHz
24. Final BW : 0 MHz; Step # 0
25. Maximum Channels : 256
26. Channel Numbers : 0:255:1
27. LO5 -1  : 149
28. LO5 -2  : 156

29. Frequency Parameters (TPA) : 591 591 540 540 51 51
30. Integration Time : 16.1061 Sec
31. No of Antennas Working(Fringing) at the beginning :29

32. Name of Non-Working Antennas (with reason for each) :
W02 : Mesh Refurbishment Work
33. Note for Backup :

34. Start and End Time of Obs.(IST): 21 May 2023 12:00:00 - 21 May 2023 18:00:00

35. ONLINE Machine : TGC

36. No of Antennas Working(Fringing) at the end :29

37. RFI Status :

38. Comments (During Observations) :
******************************************************************* 
Important Note for Observer:
The refurbishment work of the W02 antenna reflector surface is 
currently in progress. The refurbishment of the inner sectors 
will commence from 16th May 2023 onwards. Please note that this 
ongoing work may affect the sensitivity of the antenna and could 
also alter the primary beam pattern depending on the size of the
holes present on the surface. We advise exercising caution in 
using the antenna, particularly if your targets are extended or 
if you\'re using a wide field. 
******************************************************************* 
Note : GSB BB Lo problem.
********************************************************************
12:00:00 : Started setup
12:15:00 : Started cmd file
            /data1/gtac/cmd/44_108/44_108_21May2023_1200_cmd.py
18:00:00 : Stopped cmd file and observing session over.
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