Szia Tibor!

Ha jol tudom az Omegafiltersen van T-reteg a Schuler-en
nincs. Nyilvan ez is tukorozi az arat.

Ha HEGE olvasna a listat jo lenne ha erre a kerdesre valaszolna,
mert ugy emlekszem nekik van tapasztalatuk mind ketto
termekrol.

Bar kezenfekvo lenne mindezeket Bajan megbeszelni.

Mas.
Megtalaltak a GRB040924 optikai azonositojat a SUBARU-val, adatok
es a kepek alabb lathatok (bocs Brasko Sanyi de ez az eredeti). Mileyen
jo lett volna ramozdulni hiszen K-ban 17.5 mg volt, ezt lehet, hogy
lattuk volna I-ben.

H. Terada, M. Akiyama (Subaru Telescope, NAOJ) and N. Kawai (Tokyo
Tech) report:

"We have made the second epoch observation of the afterglow candidate
(GCN 2734) of GRB 040924 (=H3564, GCN 2735) in the K´-band with IRCS
on the 8.2m Subaru Telescope at 15:07-15:41 UT on September 25 (27.5
hours after the burst) for an integration time of 1200 seconds with an
average seeing of 0.52 arcsec.

At the position of the afterglow, we detected an extended source with
magnitude K´=20.4 +/- 0.2.  It is probably the afterglow of GRB 040924
with a significant contribution from its host galaxy.  Comparison with
the earlier flux (K´=17.5 at t=2.4 hr, Terada and Akiyama, GCN 2742)
imply that the NIR afterglow decay index was steeper than -1.

The image is available at
http://www.hp.phys.titech.ac.jp/nkawai/grb/040924/."


Udv:
Kereszty Zsolt
-------------------------------
Corona Borealis Observatory
Hungary, Gyorujbarat
WEB: http://kereszty.csillagaszat.hu
E-mail: cbo@axelero.hu

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From: listserv@mcse.hu [mailto:listserv@mcse.hu]On Behalf Of
CSILLAGKEP-l: Horv