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W,3 ῎ "#$% &' AGN ()*+ ,-.-/0123 456789 xM B(-= yz= {|2}~ :;<-=>? @=/ 2MASS :;< 7 AGN / (GW, ] ( cross-identification A,B( C [ ! AGN / ([ DEF;/GH23 H=@2DEI/J# ,B(^-r23 456/KLM5NO2+ L 3 P,3 Q 2 7 ῏C I ( II @R@. 5. AGN ST&'U#, -/VWMXU#,3 4 }~7 P[+/ 56VY#+P, ῏C II &'A ?AP ῌ /?, ,+ 7Z[U+ 3 \].P,B(^-,3 ^7#3 B }~W = _= `a bc9#U+ &'. d, -/0123 BB7 efbc - /AB(d _= # /?AB(,3 ghO610)/῍#U ijkd, 2.1 +12d AGN 7 a¡¢# l/mnopO2 L 4%3 ijk 1 b £¤C¥¦_@,3 § AGN 7 X + c^q-῏C II --rU#,+ s a¨,[ X © ](ª.7 AGN P,( ¼ 104 f ¼6½ 289 X ! "#$% AGN &'()*+ ,- ./012 345 X 36 7489- X 30 X :;< ROSAT =>?@ABC DE - = X 319-FGHI J- ROSAT =FGHI0 X 3 K D 2 LMNOP! QRS X 30 Bright Source Catalog (BSC) T X 30 Faint Source Catalog (FSC) U1 9 V5 ROSAT FGHI 2MASS FGHI U WXYZ[\]^ _` aX ()*- K b*K-cd AGN &' (- ef E-&'g0 15,974 (BSC: 5,273, FSC: 10,701) 6 h ῍giῌ5 AGN FGHIJ E 5 SDSS FGHIJ-V j AGN &' ¡ j¢< £¤ j¥@¦§¨© BSC ª«0 ª ¬~&'j¢<0tN ®¯ FSC ª«0 °± j¢<0N²Kp BSC Q~iqj¢<³´µ¶ N -jD FSC D E-&'U0 ·¸0 AGN tppQRSiq¹1º$ j6 -&'j AGN k 4l4mn-o 3,061 (BSC: 2,053, the Radio Sky at Twenty-centimeters (FIRST) P FSC: 1,008) j AGN k 1.4 GHz National radio astronomy observatory p6D- Very large array Sky Survey (NVSS) 6 6. ῍ῒῑῐῌ῏῎ &'iqjrs AGN 6tu 0 AGN Mv-$wp5026 E-^ Wyz KJ &'{|St$w}~o q54$wj4D- x Kq54FGHIJ aT AGN ji E-&'iyzPO aVcNjk AGN {|St$w}~- 1289 yz^}~ - 0 yFGH I cross-identification ! ^_` tP J-FGHI0 0 Mvayzpjq54 6Da y X k AGN Mv-Zj6D- SDSS 0 DEep Near-Infrared Survey of 0 AGN mn&'j southern sky (DENIS) y0 Faint Images of k AGN Mv-$w- 290 :»¼ 2011 ½ 6 » FSC BSC ! " # $ u u !12), 13)O kkg@r" ! (SDSS) %&!'()*+, !h #! ¡ ! -./01 SDSS 234 ¤N$O¥%) ¦§¨© 5 "#$6789: (u῍: 0.36 mm, ῎῍: 0.48 ©^ ª&k«¬® " mm, r῍: 0.62 mm, i῍: 0.76 mm, z῍: 0.91 mm) !;< !¯°`±)²³9H>Esl !+ 1= u῍, ῎῍, C´>µ ¦§¶·h r῍ 3 89:>?%&! AGN @AB +C@+DE11) C ! 3 89:> >"#$!%&F4GHI J& 5K & 5 L MD AGN +ABL EC@+NL )O C P QRSOT AGN UVWXYX@Z[ \! AGN @] 7E Z@^_+MD AGN @ \1E CC@L `+ AGN !"+aE C@+bc 7. ¢P£ ` 1) 2) 3) 4) 5) 6) 7) 8) 9) 10) 11) 12) 13) ¸¹' , 2002, !º( 95, 253 Sandage A., 1965, ApJ 141, 1560 Lacy M., et al., 2004, ApJS 154, 166 Stern D., et al., 2005, ApJ 631, 163 Warren S. J., Hewett P. C., Foltz C. B., 2000, MNRAS 312, 827 Glikman E., et al., 2004, ApJ 607, 60 Rieke G. H., Lebofsky M. J., 1985, ApJ 288, 618 Bessell M. S., Brett J. M., 1988, PASP 100, 1134 Meyer M. R., Calvet N., Hillenbrand L. A., 1997, AJ 114, 288 Polletta M., et al., 2007, ApJ 663, 81 Anderson S. F., et al., 2007, AJ 133, 313 Kouzuma S., Yamaoka H., 2010, A&A 509, A64 Kouzuma S., Yamaoka H., 2010, MNRAS 405, 2062 VWXYX1)defgh AGN ij+kl)7"#$! mino!) + 1) AGN >pqhr "# $sT!)ino!;<> pth C@@) u!/0vino! %wx 1"#$!mino! )1)y z{ !l @|} CC!/01 vino!%wx~}>hC@ ! aElq+!l ! 1 C>E vino!kYX;<)_ h ` AGN Y9F>rC @!l » 104 ¼ »6½ Search for AGNs in Near-Infrared ῌMethod and Search Using the Methodῌ Shinjirou KOUZUMA School of International Liberal Studies, Chukyo University, Toyota 470ῌ0393, Japan Abstract : We have proposed near-infrared color selection criteria to extract Active Galactic Nuclei (AGNs). By examining the validity of our color selection, it was found that most of AGNs can be di#erentiated from stars and several types of objects using the color selection. In addition, we extracted new AGN candidates using the color selection. Statistical properties of the extracted candidates are consistent with properties of known AGNs. Accordingly, most of the candidates are expected to be real AGNs. It should be noted that astronomical catalogues have played a crucial role in this study. 291