GTAC Observation Log 1. Date : 06/2/2012 2. Observation Sr. No. : 5807 3. Observer : Giulia Macario 4. Observer's Email : giulia.macario@oca.eu,g.macario@ira.inaf.it 5. Project Name : Searching for Radio Halos in the MACS-Planck X-ray luminous clus ter sample 6. Project Code : 21_042 7. Operator(s) : Deepak, Manisha, Navanath, Rupsingh, Sachin, Santaji, 8. Command File : /odisk/gtac/cmd/21_042/feb2012/06feb12_obs.cmd, /odisk/gtac/cmd/21_042/feb2012/07feb12_obs.cmd 9. LTA File : /gsbifrdata1/06feb/21_042_06feb2012.lta, /gsbifrdata1/06feb/21_042_07feb2012.lta 10. LogFlag File : /odisk/online1/logflags/21_042.FLAGS.7 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 : 10+12 dB, 32 MHz,ON, IF-CH2 : 10+12 dB, 32 MHz,ON GSB SETTINGS : 14. GSB Mode : RealTime 15. GSB LTA : 8 16. GAIN EQ : ON 17. Stokes : Total_Intensity 18. Beam - 1 : OFF 19. Beam - 2 : OFF 20. ACQ BW : 32 MHz 21. Maximum Channels : 256 22. IFBW (MHz) : LO5 (KHz) : 32:149000-156000 23. Final Bandwidth (MHz): OFF MHz; Step # 0 24. Frequency Parameters (TPA) : 306 306 255 255 51 51. 25. Integration Time : 8.053 Sec. 26. No of Antennas Working(Fringing) :29 27. Name of Non-Working Antennas (with reason for each) : S02 : Strong RFI lines. 28. Note for Backup :-- 29. Start and End Time of Obs.(IST): 18:40 - 09:00 30. ONLINE Machine : Lenyadri 31. Comments (During Observations) : 19:40 : scan started on 3C48. 19:25 : command file started. /odisk/gtac/cmd/21_042/feb2012/06feb12_obs.cmd 01:55 : Started scan on phase cal. 02:08 : Started flux cal. 02:21 : Started cmd file. /odisk/gtac/cmd/21_042/feb2012/07feb12_obs.cmd 07:30 : S04 antenna released for painting work. 08:08 : Source set, stopped command file. 08:10 : Started scan on phase cal. 08:15 : Stopped scan on phase cal. 08:18 : Started scan on 3C286. 09:00 : Stopped scan on 3C286 and stopped observation session.