sean <jaymose…@hotmail.com> writes:
> Craig Markwardt <craigm…@cow.physics.wisc.edu> wrote in message <news:mt2.0-25632-1056376051@sshserv.aei.mpg.de>…
> > Since you apparently admit that the IPN can work, your subsequent
> > statistical analysis of GCN circulars from 2000, 2002 and 2003,
> > basically addresses the question of multi-wavelength detection
> > *efficiency*, as opposed to functionality. You have then entered a
> > realm of complex interplay between many observing constraints and
> > sensitivities.
…
> >I`ll Try to cover the above points. I didnt count the fractions
…
> I have to say that to do all the above numbers properly I would need
> a research grant for about couple of months full time work …
My original point was that efficiency calculations for these sorts of
systems are extremely difficult. As you admit, you haven’t really
made a numerical case. I think even for the "insiders" who have a lot
of experience it would be a difficult task.
> Surely though it is the success rate between attempted and
> successful that is important. For instance if lets say only 10 per
> cent of IPN`s were followed up and 90 per cent of HETE etc`s. What
> difference would that make ?
The problem is the definitions of "success" and "attempt." What if
follow-up observations were made, but only covered a portion of the
error box. Is that an attempt? In your example above, if only 10% of
IPN locations were followed up, then by construction no more than 10%
could be localized by that technique. Some other biases to consider
include: HETE is only sensitive to GRBs on the night side of the
earth, so it will preferentially detect bursts which are observable,
and hence attemptable, by optical telescopes. Or, IPN single-annulus
solutions and "large error box" solutions are too big to be
successfully covered by narrow-field observers. These factors, and
others, will most certainly skew the measures of "attempt" and
"success."
> > Analyzing any real life data is complex. If you are seeking to apply
> > your "own methods," as you claimed in a previous posting, then you are
> > surely aware of this. You did not mention the data cited in either of
> > the Laros et al papers; why were they not suitable?
> I tried out the paper above and they both seem to be about sn/grb
> relationships and statistics regarding coincidences between the two.
> Its not exactly what I need . What I would need to do is create a 3-d
> model with x,y and z axis .
Neither of the Laros papers that I cited proposes a SN/GRB connection.
In fact, both of the papers provide 3D positions of the spacecraft
involved, as well as the times of arrival. These should suit your needs.
Laros, J., et al. 1997, Ap. J. Supp. Ser. 110, 157
Gamma-Ray Burst Arrival Time Localizations: Simultaneous
Observations by Mars Observer, Compton Gamma-Ray Observatory, and
Ulysses, (9 bursts, 1992-1993) – coincident GRO + IPN boxes
Laros, J., et al. 1998, Ap. J. Supp. Ser. 118, 391
Gamma-Ray Burst Arrival Time Localizations: Simultaneous
Observations by Pioneer Venus Orbiter, Compton Gamma-Ray
Observatory, and Ulysses (arrival times given) (37 bursts, 1991-1992)
> > No. X-ray and gamma-ray localizations by imaging satellites like
> > INTEGRAL/IBIS/SPI or HETE, and soon Swift, do not rely on the IPN
> > triangularization technique. Also, consider GRB 021125, which has a
> > smaller IPN localization than its associated IBIS position.
> I think you misunderstand me here. I realize that the "X-ray and
> gamma-ray localizations by imaging satellites like INTEGRAL/IBIS/SPI
> or HETE, and soon Swift" do not rely on IPN. What I was saying was
> that these localizations you mention above are the error boxes which
> IPN then uses to refine the annuli.
You are mistaken. The IPN solution is found by time of arrival
analysis alone, independent of other positions. It is also true that
if another error box is available, the authors of a GCN circular may
provide the overlap region, but this is quite distinct from the IPN
solution.
> Also regarding 021125 yes as with most IPN the refined overlap
> position is smaller then the error boxes but there were no OT`s
> observed there so we have no proof that that particular refined IPN
> localization is correct. And I believe that it isnt.
There is no need to prefer just optical and radio. As you point out,
the gamma- and X-ray imagers can provide quite precise positions. If
the IPN and imaged positions coincide, that should be considered a
"success." It is too narrowminded to say that the IPN serves only
optical and/or radio.
> AS I mentioned at the beginning of this post I believe that the annuli
> were derived not by pure time of arrival but actually by changing the
> time of arrival data to suit an annuli that does overlap the error
> boxes. I believe that the data must come in to the network with many
> unexplained inconsistencies that IPN finds impossible to compute
> without admitting c is not constant and therefore they actually make
> or alter existing data until they can come up with an annuli that does
> match the known error boxes.
Your claim is just silly. The point of the IPN is to enable follow-up
observations (at *all* wavelengths), not to prove that the speed of
light is constant. You are basically accusing the IPN contributors of
fraudulently altering the data to suit some ulterior motive. I am
personally acquainted with some of those involved, and they have an
honest interest in localizing GRBs as best as can be done. They are
using the best tools available for the data hand, which happens to be
time of arrival reconstruction, and it is extremely simple, involving
minimal assumptions.
There are plenty of cases which show that the IPN produces reliable
position constraints, as have been cited in my previous messages.
And, more importantly, you have not provided a single case where the
IPN solution was found to be incorrect. I have cited a case where an
IPN-only solution was used to localize both a radio and optical
transient, with no other gamma-ray positioning.
When multiple position GCN circulars come out, it is usually because
new data is incorporated into the solution, for example when more
telemetry becomes available, and of course this is always stated in
the circular.
I think enough has been said in this thread.
[[Mod. note -- I am inclined to agree with this last sentiment! -- jt]]
CM