observing with the 10m 2005 - 2006
DESCRIPTION
Observing with the 10m 2005 - 2006. Observed from 25 Sep. 2005 - 21 Jun. 2006 We did mostly AGN Monitoring New! Webpage with realtime results/timetable We had no major technical problems Weather was great! 634 hours of A/B. [Monsoon began]. Trevor Weekes (for Deirdre Horan). - PowerPoint PPT PresentationTRANSCRIPT
Observed from 25 Sep. 2005 - 21 Jun. 2006
We did mostly AGN Monitoring
New! Webpage with realtime results/timetable
We had no major technical problems
Weather was great! 634 hours of A/B
Observing with the 10m2005 - 2006
Trevor Weekes (for Deirdre Horan)
… that we did not overcome
[Monsoon began]
Available Dark Time: 167 nights
Bad weather
We had 128.5 nights of data and in total got 634 hours of data in A/B
weather
Took Data
Tech.Probs.
128.5 nights
31 nights
7.5 nights
Crab: 108 hr
Mrk421: 150 hr
LSI+61: 85 hr
H1426: 57 hr
Mrk501: 29 hr
1es1959: 51 hr
1es2344: 94 hr
Misc: 60 hr
634 Hours of A/B DataConcentrated mostly on the Crab, 5 Whipple-detected AGN and Microquasar
LSI+61303
Total: 634 hours
Object: Hours
Crab
M421
LSIH1426M501
1es1959
1es2344
Misc.
Results of 10m Observing
• Several people will describe results from the 10m campaigns this year:• Andy Smith
•AGN•LSI+61303
• John Toner•1es2344 & 1es1959
• John Kildea•The 5 Whipple Blazars
Example of Lightcurve
Sept.-Nov. 1es1959+650: Optical data
from A. Sadun, X-ray from ASM and gamma-ray data from
10m.
We will have a lot more data from other telescopes to include here.
60 Hours of A/B “Misc.” Observations
• Data on other targets:• GRBs (4 hours)• Soft Gamma Repeater 1900+14 (10 hours)• ToOs on 10 other Blazars (23 hours)
• Calibration Data:• Zenith runs (22 hours)
• at El. 80º this year
• Pointing runs (12 hours)• Took a lot of 2-min. pointing runs to telescope characterize pointing (see next slide)
• Nitrogen runs
Included in this 60 hours were:
Two-Minute Pointing Runs
• For every target observed each night, a 2-minute “pointing star run” was taken
• In order to do this, the pedestal trigger was increased from the normal 1 Hz to ~30 Hz while tracking the pointing star
• In this way, the pedvars can be used to determine how good the telescope pointing is
• A “normal” pointing check was also done after each target
12 hours of pointing runs were taken this season
We should be able to apply accurate pointing corrections to all data
taken
10m Problems and Fixes
• Tracking … Fixed (see next slide) :-)• HV … Not Fixed :-(
– BUT, not a major problem :-) … yet? :-(
• VME Software Licenses Expired on Taurus :-(– Could not re-compile GRANITE to include new CFD calibration at start of season
• Mirror Alignment looks good :-)Overall, the 10m performed very well this observing
season :-)
Fixing the Tracking Problems
• The Problem: Telescope would occasionally report incorrect El and (more recently) Az values– Intermittent -> hard to fix/debug– Software fix … to minimise impact of problem
• Oct. 2005: problem became persistent– Were able to trace it to a flakey ribbon cable in the mount
– Cable replaced … problem has not returned in El
• May 2006: same problem with Az– Equivalent ribbon cable in mount for Az replaced
Whipple Webpage
• Webpage was updated ~daily• Timetable updated each darkrun and if MWL campaign changed/started• Email sent to collaborators to keep them posted
• Preliminary AGN results posted after each night of observing• Crab rate or upper limit
Whipple Webpagehttp://veritas.sao.arizona.edu/
VERITAS_whipple.html
Links to timetable, lightcurves
and participants
There is a direct link to this page from the VERITAS webpage
Participants: 14 + ASM
Contact TelescopeRadio
I.R.
Optical
All targets on our monitoring list are also been monitored on a daily basis in
X-rays by the ASM