GTAC Observation Log 1. Date : 01/06/2014 2. Observation Sr. No. : 7138 3. Observer : Huib Intema,Reinout Johannes vanWeeren,Abhirup Datta,Surajit Paul 4. Observer's Email : hintema@nrao.edu,rvanweeren@cfa.harvard.edu,Abhirup.Datta@colorado.edu,surajit@physics.unipune.ac.in 5. Project Name : A first low-frequency study of violent mergers in the Chandra -- South-Pole Telescope galaxy cluster sample 6. Project Code : 26_024 7. Operator(s) : Nilesh,Pramod,Surender 8. Command File : 9. LTA File : /gsbifrdata/01jun/26_024_01jun2014.lta, 10. LogFlag File : /odisk/online1/logflags/26_024.FLAGS.2, ANTENNA SETTINGS : 11. RF Band(MHz) & Solar Attn(dB)- RF1 : 306 MHz ,RF2 : 306 MHz, SA1 : 0 dB, SA2 : 0 dB 12. Ist LO (MHz) & IVth LO (MHz): ILO1 : 255 MHz, ILO2 : 255 MHz , IVLO1 : 51 MHz, IVLO2 : 51 MHz 13. IF Attn(dB) , IF BW(MHz) & IF ALC : IF-CH1 : 4+12 dB, 32 MHz,ON, IF-CH2 : 4+12 dB, 32 MHz,ON GSB SETTINGS : 14. GSB Mode : Realtime 15. GSB LTA : 8 16. GSB CTRL : ONLINE 17. GSB Fstop : ON 18. GAIN EQ : ON 19. Stokes : TotIntensity 20. Beam - 1 : OFF 21. Beam - 2 : OFF 22. ACQ BW : 33.33 MHz 23. Final BW : 33.333333 MHz; Step # 0 24. Maximum Channels : 256 25. Channel Numbers : 0:255:1 26. LO5 -1 : 149.00 27. LO5 -2 : 156.00 28. Frequency Parameters (TPA) : 306 306 255 255 51 51. 29. Integration Time : 8.053056 Sec. 30. No of Antennas Working(Fringing) at the begining :29 31. Name of Non-Working Antennas (with reason for each) : S06 : Intermediately apply brakes duo to wind meter problem. 32. Note for Backup : 33. Start and End Time of Obs.(IST): 01:00 - 13:00 34. ONLINE Machine : Shivneri 35. No of Antennas Working(Fringing) at the end :28 36. Comments (During Observations) : 01:04:25 : Started scan on 3C286 for ~ 12.2138 min. 01:28:46 : Started scan on J2031-4037 for ~ 292 min. 06:23:55 : Started scan on J0014-4952 for ~ 181.06 min. 07:59 : E03 taken for painting. 09:27:09 : Started scan on J0307-5042 for ~ 192.736 min. 12:47:34 : Started scan on 3C147 for ~ 12.8849 min. 13:00 : Stopped scan and observation session is over.