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[vsnet-campaign 21] XTE J1118+480
In the light curve obtained on 8 and 9 May,
we see the change of hump profile from superhump-like (cf IAUC 7418)
to the hump characterized with the slower rise and faster decline
(vsnet-alert 4796).
Both light curves on 8 May and 9 May show this feature.
The problem whether this change is due to the growth of superhump or not,
will be solved with the next few weeks observations.
Some observers newly showed the interest to ASCA - VSNET
multiwavelength campaign on XTE J1118+480 (Drs.
G. Sostero (high-speed photometry), Zong yun Li (possibly spectroscopy?),
V. Simon (photometry), Junhui Fan, and A. Merloni).
We wish you will have successful observations.
Regards,
Makoto Uemura
on behalf of ASCA - VSNET multiwavelength campaign on XTE J1118+480
vsnet-adm@kusastro.kyoto-u.ac.jp
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