SUMMARY OF PROPOSAL 41155
DR. TADAYUKI TAKAHASHI
INSTITUTE OF SPACE AND ASTRONAUTICAL SCIENCE
KANAGAWA JAPAN 229
SAGAMIHARA
3-1-3 YOSHINODAI

  E-mail: TAKAHASI@ASTRO.ISAS.AC.JP	Tel: 0427-51-3911	Fax: 0427-59-4240
  Medium: 2.5GB8MM

Subject: AGN                                                         
  Title: IDENTIFICATION OF THE GALACTIC UNIDENTIFIED EGRET SOURCE --- 2EG J2020+4026     


Abstract:
 EGRET has found almost 30 Gamma-ray sources near the galactic plane (gb <+-10 deg).
 Among them five sources are identified as pulsars, such as Geminga. However, most of
 them have not been identified with any known sources. A few hundred MeV to GeV
 emission from galactic source is particulary interesting. Pulsar could be one
 possibility and galactic objects with jets directed toward the solar system could be
 another possibility. Because of the high galactic absorption, hard X-ray observation
 with ASCA is crucial to reveal the nature of the source. We propose to observe the
 brightest, thus with the smallest error circle, unidentified EGRET source, near Cygnus Complex.

 Co-Is:
   1  KEIICHI MATSUZAKI   	UNIV. OF TOKYO                JAPAN     
      (No Co-I contact data)
   2  YOSHITAKA SAITO     	UNIV. OF TOKYO                JAPAN     
   3  YUTARO SEKIMOTO     	UNIV. OF TOKYO                JAPAN     
   4  MASAHARU HIRAYAMA   	UNIV. OF TOKYO                JAPAN     
   5  KAZUO MAKISHIMA     	UNIV. OF TOKYO                JAPAN     
   6  NORIKO YAMASAKI     	TOKYO METRO. UNIV.            JAPAN     


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
2EG J2020+4026         1  305.1400   40.4400    40   N   N   P  0.10000   1