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[12:00:19\] David Smith Good afternoon.
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[12:00:23\] David Smith yes
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[12:00:37\] Eric Grove [https://confluence.slac.stanford.edu/display/SCIGRPS/Agendae+for+Galactic+Sources+Meetings+starting+April+2008]
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[12:00:43\] Eric Grove we'll start in a minute
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[12:02:08\] Eric Grove [https://confluence.slac.stanford.edu/display/SCIGRPS/Agendae+for+Galactic+Sources+Meetings+starting+April+2008]
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[12:03:19\] Eric Grove ok, not Science Express
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[12:04:00\] Massimiliano Razzano Last minute update : Geminga should be on ApJ 719 (august 20)
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[12:04:06\] Massimiliano Razzano my mic not working...sorry
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[12:04:15\] Jean Ballet W49B about to be resubmitted
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[12:06:49\] David Smith Nice list. Update it from time to time and re-link it to the agenda. Useful.
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[12:06:50\] Yasunobu Uchiyama joined
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[12:07:17\] Joshua Lande joined
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[12:07:19\] Eric Grove yep, David, that's the idea
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[12:07:57\] Terri Brandt should these papers just be on LAT data? or also on sources seen with LAT?
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[12:08:08\] Eric Grove anything that's relevant to us
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[12:08:30\] Terri Brandt sounds good\!
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[12:09:21\] Pablo Saz Parkinson yes
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[12:09:22\] David Thompson yes
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[12:09:23\] Eric Grove yes
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[12:09:23\] David Smith yes
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[12:09:24\] Damien Parent yes
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[12:14:51\] Andrew Chen patrizia, we can't hear you
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[12:14:51\] David Smith silence reigns...
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[12:14:53\] Eric Grove if you're speaking, Patrizia, I can't hear you
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[12:14:57\] Eric Grove yes
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[12:14:57\] Andrew Chen better
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[12:14:58\] David Smith yes
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[12:15:21\] David Smith wow\!
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[12:15:35\] David Thompson Congratulations to Nanni\!
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[12:15:38\] David Smith For the Green Party?
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[12:15:41\] Andrea De Luca joined
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[12:16:18\] Eric Grove you're a bit fain,t Andrew
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[12:17:47\] Eric Grove
\Grove
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[12:18:39\] Eric Grove yes
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[12:18:40\] David Smith yes
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[12:21:29\] Eric Grove yes
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[12:21:29\] David Smith yes
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[12:21:30\] Adam Hill yes
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[12:21:43\] Eric Grove [https://confluence.slac.stanford.edu/download/attachments/12222500/etacar_htakahashi_100727.pdf?version=1&modificationDate=1280245133198]
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[12:22:52\] Andrea De Luca joined
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[12:32:57\] Andrew Chen nominally E>100 MeV, photons run out at high energy
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[12:33:09\] Andrew Chen I would say that there's a lot of contamination from photons 100 MeV
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[12:34:28\] Seth Digel What does contamination from photons 100 MeV mean?
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[12:36:19\] Pablo Saz Parkinson I think the question was for Andrew
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[12:36:32\] Andrew Chen dE/E ~ 1
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[12:36:47\] Andrew Chen for steep spectra, think analogue of Eddington bias
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[12:37:00\] Seth Digel Ah, ok
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[12:37:39\] Seth Digel The color bar in that figure goes from 0 to 0.6 counts cm-2 s-1 pixel-1
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[12:40:22\] David Smith Jurgen is apparently in Tuirkey
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[12:41:16\] Rolf Buehler left
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[12:42:03\] Seth Digel Pub Board has approved resubmitting the paper on July 24, not sure if it has gone back in yet
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[12:42:07\] Eric Grove [https://confluence.slac.stanford.edu/display/SCIGRPS/UnID+Fermi+Objects+Suzaku+paper]
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[12:42:47\] Joshua Lande left
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[12:47:28\] David Smith The draft of the "Two Nancay" (PSRs J2017+0603 and J2302+4442...
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[12:48:02\] Michael Wolff Coming soon...
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[12:49:50\] David Smith Personally i don't really see that it matters... once they're in the hands of referees, all synchronisation gets lost.
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[12:49:52\] Paul Ray I don't think submission is the important thing.
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[12:50:06\] David Smith We don't post to astro-ph before acceptance anyway.
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[12:50:15\] Paul Ray Go ahead and submit any of them when ready.
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[12:50:19\] David Smith I vote: submit a.s.a.p.
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[12:50:27\] Paul Ray We'll coordinate on re-submission timescales
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[12:51:01\] David Smith Paul's remark is wise. (as usual)
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[12:51:09\] Paul Ray If you submit the Suzaku paper it will put more pressure on Scott as well.
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[12:51:18\] David Smith verily.
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[12:51:27\] Teddy Cheung thanks
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[12:51:32\] David Smith yes
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[12:51:46\] Eric Grove [https://confluence.slac.stanford.edu/download/attachments/12222500/J1103-53-100727-GlctEVO.pdf?version=1&modificationDate=1280246396148]
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[12:52:02\] Paul Ray joined
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[12:52:36\] Paul Ray Scott Ransom just wrote back to me that he is working on it now and expects to have a draft for me today.
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[12:53:29\] Eric Grove thanks Paul. Good news, that.
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[13:05:47\] Roger Romani So... we are to conclude that the gamma-ray source is the Blazar and the MSP is just seredipitous?
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[13:06:09\] Eric Grove yes
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[13:06:35\] Damien Parent what is the Edot of this MSP ?
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[13:06:38\] Pablo Saz Parkinson I don't think it had been associated with an AGN when it was selected
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[13:06:59\] Peter den Hartog do you detect a source adding all the data after nov, and if so what spectrum does that give?
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[13:07:08\] Michael Wolff left
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[13:07:56\] Paul Ray The best test will be to look for pulsed emission once we have a good timing ephemeris from the radio
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[13:08:01\] Peter den Hartog ok, thanks\!
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[13:08:36\] Damien Parent do you have an idea about the distance / Edot ?
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[13:08:59\] Paul Ray Not off the top of my head.
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[13:09:01\] Ozlem Celik Paul?
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[13:09:04\] Paul Ray It is in the paper draft
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[13:09:07\] Damien Parent ok
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[13:09:13\] Paul Ray we have a DM and the distance is quite large I recall
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[13:09:17\] Paul Ray maybe 5-6 kpc?
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[13:09:36\] Paul Ray I think it would be one of the most distant Fermi MSPs if we detect it
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[13:09:36\] Aous Abdo left
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[13:09:58\] Paul Ray Oh, so my memory was totally wrong\!
\!
[13:10:02\] Paul Ray Not too surprising...
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[13:10:08\] Peter den Hartog cool stuff
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[12:00:19\] David Smith Good afternoon.
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[12:00:23\] David Smith yes
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[12:00:37\] Eric Grove [https://confluence.slac.stanford.edu/display/SCIGRPS/Agendae+for+Galactic+Sources+Meetings+starting+April+2008]
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[12:00:43\] Eric Grove we'll start in a minute
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[12:00:46\] Another Uchiyama joined
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[12:01:04\] Patrizia Caraveo joined
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[12:01:15\] Massimiliano Razzano joined
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[12:02:08\] Eric Grove [https://confluence.slac.stanford.edu/display/SCIGRPS/Agendae+for+Galactic+Sources+Meetings+starting+April+2008]
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[12:03:19\] Eric Grove ok, not Science Express
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[12:03:20\] Seth Digel joined
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[12:03:33\] Denis Dumora joined
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[12:03:52\] Daniela Hadasch joined
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[12:04:00\] Massimiliano Razzano Last minute update : Geminga should be on ApJ 719 (august 20)
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[12:04:06\] Massimiliano Razzano my mic not working...sorry
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[12:04:15\] Jean Ballet W49B about to be resubmitted
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[12:04:47\] Teresa Mineo joined
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[12:04:55\] David Thompson joined
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[12:05:36\] Another Uchiyama left
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[12:06:23\] Michael Wolff joined
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[12:06:49\] David Smith Nice list. Update it from time to time and re-link it to the agenda. Useful.
\
[12:06:50\] Yasunobu Uchiyama joined
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[12:07:17\] Joshua Lande joined
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[12:07:19\] Eric Grove yep, David, that's the idea
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[12:07:22\] Robin Corbet joined
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[12:07:57\] Terri Brandt should these papers just be on LAT data? or also on sources seen with LAT?
\
[12:08:08\] Eric Grove anything that's relevant to us
\
[12:08:30\] Terri Brandt sounds good\!
\
[12:09:21\] Pablo Saz Parkinson yes
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[12:09:22\] David Thompson yes
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[12:09:23\] Eric Grove yes
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[12:09:23\] David Smith yes
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[12:09:24\] Damien Parent yes
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[12:10:03\] Marcus Ziegler joined
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[12:12:28\] Andrea De Luca left
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[12:14:51\] Andrew Chen patrizia, we can't hear you
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[12:14:51\] David Smith silence reigns...
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[12:14:53\] Eric Grove if you're speaking, Patrizia, I can't hear you
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[12:14:57\] Eric Grove yes
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[12:14:57\] Andrew Chen better
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[12:14:58\] David Smith yes
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[12:15:21\] David Smith wow\!
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[12:15:35\] David Thompson Congratulations to Nanni\!
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[12:15:38\] David Smith For the Green Party?
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[12:15:41\] Andrea De Luca joined
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[12:16:18\] Eric Grove you're a bit fain,t Andrew
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[12:17:47\] Eric Grove
\Grove
[12:18:36\] Adam Hill joined
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[12:18:39\] Eric Grove yes
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[12:18:40\] David Smith yes
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[12:19:47\] Andrea De Luca left
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[12:21:29\] Eric Grove yes
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[12:21:29\] David Smith yes
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[12:21:30\] Adam Hill yes
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[12:21:43\] Eric Grove [https://confluence.slac.stanford.edu/download/attachments/12222500/etacar_htakahashi_100727.pdf?version=1&modificationDate=1280245133198]
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[12:22:52\] Andrea De Luca joined
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[12:32:57\] Andrew Chen nominally E>100 MeV, photons run out at high energy
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[12:33:09\] Andrew Chen I would say that there's a lot of contamination from photons 100 MeV
\
[12:33:50\] Roger Romani joined
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[12:34:28\] Seth Digel What does contamination from photons 100 MeV mean?
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[12:36:12\] Paul Ray joined
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[12:36:19\] Pablo Saz Parkinson I think the question was for Andrew
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[12:36:32\] Andrew Chen dE/E ~ 1
\
[12:36:47\] Andrew Chen for steep spectra, think analogue of Eddington bias
\
[12:37:00\] Seth Digel Ah, ok
\
[12:37:39\] Seth Digel The color bar in that figure goes from 0 to 0.6 counts cm-2 s-1 pixel-1
\
[12:39:13\] Tyrel Johnson joined
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[12:39:26\] Joshua Lande joined
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[12:39:44\] Rolf Buehler joined
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[12:40:22\] David Smith Jurgen is apparently in Tuirkey
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[12:41:16\] Rolf Buehler left
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[12:42:03\] Seth Digel Pub Board has approved resubmitting the paper on July 24, not sure if it has gone back in yet
\
[12:42:07\] Eric Grove [https://confluence.slac.stanford.edu/display/SCIGRPS/UnID+Fermi+Objects+Suzaku+paper]
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[12:42:47\] Joshua Lande left
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[12:43:00\] Joshua Lande joined
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[12:47:28\] David Smith The draft of the "Two Nancay" (PSRs J2017+0603 and J2302+4442...
\
[12:48:02\] Michael Wolff Coming soon...
\
[12:49:50\] David Smith Personally i don't really see that it matters... once they're in the hands of referees, all synchronisation gets lost.
\
[12:49:52\] Paul Ray I don't think submission is the important thing.
\
[12:50:06\] David Smith We don't post to astro-ph before acceptance anyway.
\
[12:50:15\] Paul Ray Go ahead and submit any of them when ready.
\
[12:50:19\] David Smith I vote: submit a.s.a.p.
\
[12:50:27\] Paul Ray We'll coordinate on re-submission timescales
\
[12:51:01\] David Smith Paul's remark is wise. (as usual)
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[12:51:09\] Paul Ray If you submit the Suzaku paper it will put more pressure on Scott as well.
\[12
[12:51:18\] David Smith verily.
\
[12:51:27\] Teddy Cheung thanks
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[12:51:32\] David Smith yes
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[12:51:42\] Paul Ray left
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[12:51:46\] Eric Grove [https://confluence.slac.stanford.edu/download/attachments/12222500/J1103-53-100727-GlctEVO.pdf?version=1&modificationDate=1280246396148]
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[12:52:02\] Paul Ray joined
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[12:52:36\] Paul Ray Scott Ransom just wrote back to me that he is working on it now and expects to have a draft for me today.
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[12:53:29\] Eric Grove thanks Paul. Good news, that.
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[13:05:47\] Roger Romani So... we are to conclude that the gamma-ray source is the Blazar and the MSP is just seredipitous?
\
[13:06:09\] Eric Grove yes
\
[13:06:35\] Damien Parent what is the Edot of this MSP ?
\
[13:06:38\] Pablo Saz Parkinson I don't think it had been associated with an AGN when it was selected
\
[13:06:59\] Peter den Hartog do you detect a source adding all the data after nov, and if so what spectrum does that give?
\
[13:07:08\] Michael Wolff left
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[13:07:56\] Paul Ray The best test will be to look for pulsed emission once we have a good timing ephemeris from the radio
\
[13:08:01\] Peter den Hartog ok, thanks\!
\
[13:08:36\] Damien Parent do you have an idea about the distance / Edot ?
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[13:08:54\] Robin Corbet left
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[13:08:59\] Paul Ray Not off the top of my head.
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[13:09:01\] Ozlem Celik Paul?
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[13:09:04\] Paul Ray It is in the paper draft
\
[13:09:07\] Damien Parent ok
\
[13:09:13\] Paul Ray we have a DM and the distance is quite large I recall
\
[13:09:17\] Paul Ray maybe 5-6 kpc?
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[13:09:36\] Paul Ray I think it would be one of the most distant Fermi MSPs if we detect it
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[13:09:36\] Aous Abdo left
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[13:09:58\] Paul Ray Oh, so my memory was totally wrong\!
\!
[13:10:02\] Paul Ray Not too surprising...
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[13:10:08\] Peter den Hartog cool stuff
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