Astronomical Images
--- Kiso Observatory Image Use Policy ---
Kiso Observatory encourages the use of its images for educational and public
Information. If you wish to use images taken in Kiso Observatory,
please send the following application form to the observatory via e-mail.
If you want to use it temporarily in school classes, you do not need to submit an application.
--- Credit notation ---
When using th imege, please specify one of th following credits depending on th space.
- Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo
- Kiso Observatory, School of Science, The University of Tokyo
- Kiso Observatory, The University of Tokyo
--- Acknowledgement ---
The images of the Leonids meteor shower were digitized from film data by Yoshida, H. (Univ. of Tokyo).
The images of NGC7000, M31 and Rosette Nebula were color-synthesized by Yamanaka, Y. (astrophotographer).
The image of M101 was observed by Tomita, A. (Wakayama Univ.), Takeuchi, T. T. (NAOJ), Furukawa, S. (Wakayama Univ.), and Nishibata, K. (Wakayama Univ.) and was reduced by Nishibata, K. (Wakayama Univ.).
The images of The Comet Ikeya-Zhange and M64 were observed by Watanabe, J. (NAOJ), Suzuki, J., and Ishiguro, M. (Tokyo-U. of Sci.) at the Kiso Observatory during their allocated observing time. The data of the Comet Ikeya-Zhange were reduced by Fukushima, H. (NAOJ).
The images of The M33 (3 colors), M27, M57, and M16 were observed and reduced by Ishiguro, M. (ISAS) and Usui F. (U-Tokyo) at the Kiso Observatory during their allocated observing time.
The image of Comet C/2002 T7(LINEAR) was observed and reduced by Yoshioka, T. (Nagoya Univ.) and Nishiura, S. (Tokyo Gakugei Univ.) at the Kiso Observatory during their allocated observing time.
The image of NGC6791 was observed and reduced by Hasegawa, T. (Gunma Astronomical observatory) and Sakamoto, T. (Japan Spaceguard Association) at the Kiso Observatory during their allocated observing time.
All staff in the Kiso Observatory would like to thank all observers.