{"id":187,"date":"2018-12-24T19:23:44","date_gmt":"2018-12-24T10:23:44","guid":{"rendered":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/?page_id=187"},"modified":"2026-03-24T09:46:58","modified_gmt":"2026-03-24T00:46:58","slug":"presentaion","status":"publish","type":"page","link":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/?page_id=187","title":{"rendered":"Presentation"},"content":{"rendered":"\n

International Conference\/Seminar\uff08\u56fd\u969b\u5b66\u4f1a\/\u30bb\u30df\u30ca\u30fc\uff09\u8a0896\u4ef6<\/h2>\n\n\n\n
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  1. Y.Toba*<\/strong>, “Overview of AGN sciences with HSC-SSP and PFS-SSP”, SMBH growth viewed with large field surveys: special focus on the initial results from Subaru PFS<\/a>, ASIAA, Taiwan (March 2026) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  2. Y.Toba*<\/strong>, “Big data-based AGN study in the Subaru PFS, Euclid, and LSST Era”, Galaxy-IGM Workshop 2025<\/a>, Hotel Sun Valley Nasu (July 2025) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  3. Y.Toba*<\/strong>, “A Complete Census of Dust Properties in AGN: A Synergy with Subaru, JWST, and PRIMA”, PRIMA-J Science Workshop 2025, University of Tokyo (June 2025) <\/li>\n\n\n\n
  4. Y.Toba*<\/strong>, “The current status of PFS-SSP AGN sciences”, 2nd PFS-AGN Town Meeting<\/a>, NAOJ (March 2025) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  5. Y.Toba<\/strong>, “UV-to-FIR SED of JWST sources inferred by the SED fitting and implication for the PRIMA mission”, Evolution of Dust and Gas throughout Cosmic Time<\/a>, Hiroshima (December 2024)<\/li>\n\n\n\n
  6. Y.Toba*<\/strong>, “Countryside vs. City: which is favorable for a supermassive black hole?”, International Symposium on Advanced and Sustainable Science and Technology<\/a>, National Chung Hsing University, Taiwan (September 2024) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  7. Y.Toba*<\/strong>, “Overview of AGN sciences with HSC and PFS”, AGN across the sky: new windows opened by HSC and other wide-field surveys<\/a>, Hokkaido Information University (August 2024)<\/li>\n\n\n\n
  8. Y.Toba*<\/strong>, “Exploring the brightest: the hunt for the most luminous infrared galaxies in the Universe”, IAA Lunch Talk<\/a>, ASIAA, Taiwan (August 2024) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  9. Y.Toba<\/strong>, A.Hashiguchi, N.Ota, M.Oguri, N.Okabe, Y.Ueda, M.Imanishi, CAMIRA-AGN collaboration, “Emergence of AGN in galaxy clusters: the relationship among AGN, environment, and cluster-cluster mergers”, 10th Galaxy Evolution Workshop<\/a>, ASIAA, Taiwan (August 2024)<\/li>\n\n\n\n
  10. Y.Toba<\/strong>, \u201cAGN properties of \u223c1 million member galaxies of galaxy groups\/clusters at z < 1.4 based on the Subaru Hyper Suprime-Cam survey\u201d, AGN across Continents<\/a>, Durham University (July 2024) (I also introduced Subaru PFS as a panelist<\/strong> in the plenary discussion session at the conference)<\/li>\n\n\n\n
  11. Y.Toba*<\/strong>, “Insights into AGN activity in galaxy groups\/clusters: a statistical study with Subaru HSC survey”, Astro Colloquium<\/a>, Tohoku University (July 2024) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  12. Y.Toba*<\/strong>, “AGN sciences with PRIMA, synergy with Subaru HSC and PFS”, PRIMA Science Workshop, NAOJ (June 2024) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  13. Y.Toba*<\/strong>, and PFS-GE AGN subWG, “PFS-AGN sciences”, PFS-satellite workshop, NAOJ (March 2024)<\/li>\n\n\n\n
  14. Y.Toba*<\/strong>, “Mid-infrared view of optically dark galaxies in the AKARI NEP field”, ALMA workshop 2023A<\/a>, Nobumoto Ohama Memorial Hall, Ishigaki Island (January 2024)<\/li>\n\n\n\n
  15. Y.Toba*<\/strong>, “An overview of the HSC-AGN sciences”, The HSC-AGN collaboration meeting 2023<\/a>, Ehime University (November, 2023)<\/li>\n\n\n\n
  16. Y.Toba<\/strong>, “Dust properties of extremely luminous infrared galaxies”, Illuminating the Dusty Universe: A Tribute to the Work of Bruce Draine<\/a>, Galileo Galilei Institute for Theoretical Physics, Florence, Italy (October 2023)<\/li>\n\n\n\n
  17. Y.Toba*<\/strong>, “How does the AGN number fraction in galaxy clusters depend on redshift and distance from the cluster center?”, East-Asia AGN Workshop 2023<\/a>, Kagoshima University (September 2023)<\/li>\n\n\n\n
  18. Y.Toba*<\/strong>, “A search for the most luminous galaxies in the Universe”, International Symposium on Advanced and Sustainable Science and Technology<\/a>, National Chung Hsing University, Taiwan (September 2023) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  19. Y.Toba*<\/strong>, “Dust-obscured AGN viewed with multi-wavelength data”, ASIAA Colloquium<\/a>, ASIAA (September 2023)<\/li>\n\n\n\n
  20. Y.Toba*<\/strong>, “Ionized and molecular gas outflow in dust-obscured AGN”, Mini-workshop on AGN x ALMA, Ehime University (June 2023)<\/li>\n\n\n\n
  21. Y.Toba<\/strong>, “Galaxy SED and morphological works based on Subaru Hyper Suprime-Cam towards Euclid”, Euclid Consortium meeting 2023<\/a>, CPH Conference, Copenhagen (June 2023)<\/li>\n\n\n\n
  22. Y.Toba<\/strong>, S.Yamada, K.Matsubayashi, K.Terao, A.Moriya, Y.Ueda, and GOLAS-KOOLS collaboration, “How do galaxy mergers affect the ionized gas kinematics of galaxies? ~KOOLS-IFU\/Seimei view of local U\/LIRGs~”, 9th Galaxy Evolution Workshop<\/a>, Kyoto University (February 2023)<\/li>\n\n\n\n
  23. Y.Toba<\/strong>, and PFS-GE AGN subWG, “PFS-SSP preparation: AGN sciences with cosmology and galaxy evolution surveys”, Subaru Users Meeting FY2022<\/a>, NAOJ (January 2023)<\/li>\n\n\n\n
  24. Y.Toba*<\/strong>, “An overview of the HSC-AGN sciences”, Tracing the SMBH growth: outlook beyond the HSC-SSP, and future collaborations<\/a>, Kagoshima University (November 2022)<\/li>\n\n\n\n
  25. Y.Toba*<\/strong>, “A multi-wavelength view of Active Galactic Nuclei selected with eROSITA”, ISAS Astrophysics Colloquia<\/a>, ISAS\/JAXA (November 2022) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  26. Y.Toba*<\/strong>, T.Liu, T.Urrutia, M.Salvato, J.Li, Y.Ueda, M.Brusa, N.Yutani, K.Wada, and HSC-eROSITA AGN collaboration, “eROSITA and WISE view of dust-obscured AGN at z < 4”, What drives the growth of black holes: a decade of reflection<\/a>, Reykjavik, Iceland (September, 2022)<\/li>\n\n\n\n
  27. Y.Toba*<\/strong><\/strong>, “An Introduction of Dust-Obscured AGN Viewed with Multi-Wavelength Data”, 2022 NCHU Astrophysics Symposium<\/a>, National Chung Hsing University, Online (September, 2022) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  28. Y.Toba*<\/strong><\/strong>, A.Hashiguchi, N.Ota, M.Oguri, N.Okabe, B.-Ch.Hsieh, A.Yanagawa, Y.Ueda, and HSC Projects 364 and 417 members, “Dependence of AGN fraction on cluster redshift and the distance from the cluster center viewed with Subaru Hyper Suprime-Cam”, COSPAR 2022,<\/a> Athens, Greece (July, 2022)<\/li>\n\n\n\n
  29. Y.Toba*<\/strong>, “X-ray properties of WISE selected AGN viewed with eROSITA”, KIAA-DoA seminar<\/a>, KIAA-PKU, Online (May, 2022) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  30. Y.Toba*<\/strong>, “Multi-wavelength view of dust-obscured AGN”, Astronomy Colloquium<\/a>, Seoul National University, Online (April, 2022) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  31. Y.Toba*<\/strong>, “An overview of AGN WG”, The HSC collaboration meeting 2022, Online (February, 2022) [Invited]<\/strong><\/mark> <\/li>\n\n\n\n
  32. Y.Toba*<\/strong>, T.Liu, T.Urrutia, M.Salvato, J.Li, Y.Ueda, M.Brusa, N.Yutani, K.Wada, and HSC-eROSITA AGN collaboration, “eROSITA view of WISE-selected AGN at z \u2264 4”, GALAXY EVOLUTION WORKSHOP 2021<\/a>, Hybrid (online or NAOJ) (February, 2022)<\/li>\n\n\n\n
  33. Y.Toba*<\/strong>, “eROSITA view of WISE-selected AGN”, East-Asia AGN Workshop 2021<\/a>, Online (October, 2021)<\/li>\n\n\n\n
  34. Y.Toba*<\/strong>, “SOFIA\/HAWC+ view of an extremely luminous infrared galaxy at z = 3.7”, The Future of Airborne Infrared\/Submm Astronomy: Prospects and Opportunities<\/a>, Online (July, 2021)<\/li>\n\n\n\n
  35. Y.Toba*<\/strong>, “HSC AGN overview”, Joint XXL-HSC meeting, Online (July, 2021) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  36. Y.Toba*<\/strong>, M.Brusa, T.Liu, T.Urrutia, J.Buchner, J.Li, A.Merloni, T.Nagao, A.Nishizawa, M.Salvato, Y.Terashima,.Ueda, K.Wada, N.Yutani, and HSC-eROSITA AGN collaboration, “eROSITA view of WISE mid-IR galaxies\/AGN”, 17th German eROSITA Virtual Consortium meeting (online) (June, 2021) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  37. Y.Toba*<\/strong>, HSC-eROSITA AGN collaboration, “Initial results from Subaru\/HSC-eROSITA AGN collaboration”, Subaru Users Meeting FY2020<\/a> (online) (March, 2021)<\/li>\n\n\n\n
  38. Y.Toba*<\/strong>, M.Brusa, T.Liu, J.Buchner, Y.Terashima, T.Urrutia, M.Salvato, and eROSITA-HSC AGN collaboration, “eROSITA view of an extremely luminous infrared galaxy at z = 1.87”, Galaxy Evolution Workshop 2020 <\/a>(online) (January, 2021)<\/li>\n\n\n\n
  39. Y.Toba*<\/strong>, Y.Ueda, P.Gandhi, C.Ricci, D.Burgarella, V.Buat, T.Nagao, S.Oyabu, H.Matsuhara, B.-C.Hsieh, “How does the polar dust affect the dust covering factor of AGNs? “, Probing the Extragalactic Universe with High Energy and Very High Energy Sources,<\/a> NECO online workshop (December, 2020)<\/li>\n\n\n\n
  40. Y.Toba*<\/strong>, Y.Ueda, P.Gandhi, C.Ricci, D.Burgarella, V.Buat, T.Nagao, S.Oyabu, H.Matsuhara, B.-C.Hsieh, “How does the polar dust affect the dust covering factor of AGNs? ~Application of X-CIGALE to SDSS quasars~”, NEP Conference 2020<\/a>, ASIAA\/Online, Taiwan (November, 2020)<\/li>\n\n\n\n
  41. Y.Toba*<\/strong>, T.Goto, N.Oi, T.-W.Wang, S.J.Kim, S.C.-C.Ho, D.Burgarella, T.Hashimoto, B.-C.Hsieh, T.-C.Huang, H.S.Hwang, H.Ikeda, H.K.Kim, S.Kim, D.Lee, M.A.Malkan, H.Matsuhara, T.Miyaji, R.Momose, Y.Ohyama, S.Oyabu, C.Pearson, D.J.D.Santos, H.Shim, T.Takagi, Y.Ueda, Y.Utsumi, T.Wada, “Dust properties of optically dark IR galaxies without counterparts of Subaru HSC in the AKARI NEP field”, DUST2020 in Marseille<\/a>, Online (October, 2020)<\/li>\n\n\n\n
  42. Y.Toba*<\/strong>, “Search for optically `invisible’ galaxies in the AKARI North Ecliptic Pole Field”, ISAS Astrophysics Colloquia<\/a>, Online (October, 2020) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  43. Y.Toba*<\/strong>, “Report on AGN joint HSC-eROSITA science programs”, German eROSITA Virtual Consortium meeting, Online (July, 2020) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  44. Y.Toba*<\/strong>, “HSC AGN WG update”, Joint XXL-HSC meeting, Online (July, 2020) [Invited]<\/li>\n\n\n\n
  45. Y.Toba*<\/strong>, “eROSITA view of dust-obscured AGNs”, The HSC-AGN face-to-face meeting, Kyoto University, Japan (January, 2020)<\/li>\n\n\n\n
  46. Y.Toba*<\/strong>, W-H.Wang, T.Nagao, Y.Ueda, J.Ueda, C-F.Lim, Y-Y.Chang, T.Saito, R.Kawabe, “Far-infrared View of an Extremely Luminous Infrared Galaxy at z = 3.7”, Galaxy Formation and Evolution Across Cosmic Time<\/a>, ASIAA, Taiwan (December, 2019)<\/li>\n\n\n\n
  47. Y.Toba*<\/strong>, “Multi-wavelength view of hyper\/extremely-luminous infrared galaxies”, Kindai Cosmology Seminar, Kindai University, Japan (November, 2019) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  48. Y.Toba*<\/strong>, \u201cMulti-wavelength view of dust-obscured galaxies”, SUBARU TELESCOPE 20TH ANNIVERSARY<\/a>, Kona, Hawai (November, 2019)<\/li>\n\n\n\n
  49. Y.Toba<\/strong>, \u201cPossible collaboration between AGN and galaxy cluster sciences with HSC” , The 3rd HSC-X Cluster Workshop, Nagoya University, Japan (September, 2019)<\/li>\n\n\n\n
  50. Y.Toba<\/strong>*, \u201cAKARI sources without HSC counterparts “, NEP MEETING 2019 ~Future Science with Multi-Wavelength data~<\/a>, NTHU, Taiwan (June, 2019) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  51. Y.Toba*<\/strong>, \u201cPhysical properties of luminous radio galaxies at 0 < z < 1.7 selected with Subaru Hyper Suprime-Cam and VLA FIRST survey”, Supermassive Black Holes: Environment and Evolution<\/a>, Corfu, Greece (June, 2019)<\/li>\n\n\n\n
  52. Y.Toba<\/strong>, \u201cDusty radio galaxies with high SFR, AGN luminosity, and Eddington ratio discovered by Subaru\/HSC and VLA\/FIRST”, 6th Galaxy Evolution Workshop<\/a>, Kavli IPMU, Japan (June, 2019)<\/li>\n\n\n\n
  53. Y.Toba*<\/strong>, \u201cDust-obscured AGNs viewed with eROSITA and HSC”, First HSC-eROSITA-DE joint collaboration meeting, MPE, Germany (May, 2019) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  54. Y.Toba*<\/strong>, \u201cPhysical properties of optically-faint radio galaxies discovered by HSC and FIRST\u201d, Subaru Users Meeting FY2018<\/a>, NAOJ, Japan (January, 2019)<\/li>\n\n\n\n
  55. Y.Toba*<\/strong>, T.Yamashita, T.Nagao, W-H.Wang, Y.Ueda, K.Ichikawa, T.Kawaguchi, and WERGS team, \u201cPhysical properties of radio galaxies selected with Subaru Hyper Suprime-Cam and VLA FIRST surveys\u201d, East-Asia AGN Workshop 2019<\/a>, ASIAA, Taiwan (January, 2019)<\/li>\n\n\n\n
  56. Y.Toba*<\/strong>, “Multi-Wavelength properties of the HSC-FIRST radio galaxies\/quasars”, Formation and evolution of SMBHs ~revealed by ‘Wide field’, ‘Multi-wavelength’, and ‘Transient’ surveys with HSC~, Tohoku University., Japan (November, 2018)<\/li>\n\n\n\n
  57. Y.Toba,<\/strong> \u201cInfrared properties of optically-faint radio galaxies\/quasars discovered by Subaru\/HSC and FIRST\u201d, IAU Focus Meeting FM3: Radio Galaxies<\/a>: Resolving the AGN phenomenon, Austria Center Vienna, Austria (August, 2018)<\/li>\n\n\n\n
  58. Y.Toba*,<\/strong> \u201cRevisiting the relationship between mid-infrared and X-ray luminosities of AGNs\u201d, NEP meeting 2018: Since with AKARI NEP infrared data<\/a>, NTHU, Taiwan (June, 2018) <\/li>\n\n\n\n
  59. Y.Toba*,<\/strong> \u201cDiscovery of an Extremely Luminous Dust-obscured Galaxy Observed with SDSS, WISE, JCMT, and SMA\u201d, 5th Galaxy Evolution Workshop<\/a>, Ehime University, Japan (June, 2018)<\/li>\n\n\n\n
  60. Y.Toba*<\/strong>, S,Komugi, T.Nagao, T.Yamashita, W-H.Wang, M.Imanishi, A-L.Sun, \u201cNo Sign of Strong Molecular Gas Outflow in an Infrared-bright Dust-obscured Galaxy with Strong Ionized-gas Outflow\u201d, 2018 ASROC Annual Meeting<\/a>, National Quemoy University, Taiwan (May, 2018)<\/li>\n\n\n\n
  61. Y.Toba,<\/strong>, S,Komugi, T.Nagao, T.Yamashita, W-H.Wang, M.Imanishi, A-L.Sun, \u201cALMA Observation of an IR-bright Dust Obscured Galaxy with Strong Ionized Gas Outflow\u201d, ALMA\/45m\/ASTE Users Meeting 2017<\/a>, National observatory of Japan, Japan (December, 2017)<\/li>\n\n\n\n
  62. Y.Toba*<\/strong>, \u201cAn extremely luminous Dust-Obscured Galaxy discovered by the optical to millimeter observations\u201d, TTTT Seminar<\/a>, NTHU, Taiwan (December, 2017) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  63. Y.Toba*<\/strong>, H-J Bae, T.Nagao, J-H Woo, W-H Wang, A Y. Wagner, A-L Sun, Y-Y Chang, \u201cIonized Gas Outflows in Infrared-bright Dust-obscured Galaxies Selected with WISE and SDSS\u201d, East-Asia AGN Workshop 2017<\/a>, Kagoshima University, Japan (December, 2017)<\/li>\n\n\n\n
  64. Y.Toba*<\/strong>, \u201cDust-free quasars in the early Universe selected with HSC and MIRI\/JWST\u201d, HSC-AGN face-to-face meeting 2017, The University of Tokyo, Japan (December, 2017)<\/li>\n\n\n\n
  65. Y.Toba*<\/strong>, \u201cIonized Gas Outflows in Infrared-bright Dust-obscured Galaxies (DOGs) at 0 < z < 1\u201d, The East Asian Young Astronomers Meeting 2017<\/a>, Ishigaki Island, Japan (November, 2017)<\/li>\n\n\n\n
  66. Y.Toba*<\/strong>, \u201cWhere do infrared-bright dust-obscured galaxies lie on the star formation rate-stellar mass plane?\u201d,  The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life<\/a>, The University of Tokyo, Japan (October, 2017)<\/li>\n\n\n\n
  67. Y.Toba*,<\/strong> \u201cSearch for extremely-luminous infrared galaxies ~follow up observations with SCUBA-2\/JCMT and SMA~\u201d,  ASIAA lunch talk<\/a>, ASIAA, Taiwan (July, 2017)<\/li>\n\n\n\n
  68. Y.Toba*<\/strong>, T.Nagao, W-H.Wang, H.Matsuhara, M.Akiyama, T.Goto, Y.Koyama, Y. Ohyama, I.Yamamura , \u201cStellar mass and star formation rate relation of infrared-bright dust-obscured galaxies selected with IRAS and AKARI far-infrared all-sky survey\u201d, 2017 Asian-Pacific Regional IAU Meeting<\/a>, the International Convention Center (Taipei), Taiwan (July, 2017)<\/li>\n\n\n\n
  69. Y.Toba*<\/strong>, \u201cDust-obscured galaxies\/AGNs viewed with Subaru Hyper Suprime-Cam survey\u201d, Cross-Strait Symposium of Astrophysics<\/a>, ASIAA, Taiwan (July, 2017)<\/li>\n\n\n\n
  70. Y.Toba*<\/strong>, W-H.Wang, S.Komugi, T.Nagao, T.Yamashita, K.Kawasaki, M.Imanishi \u201cALMA observations of infrared-bright dust-obscured galaxies\u201d, East-Asian ALMA Science Workshop 2016-Taiwan<\/a>, NTHU, Taiwan, (March, 2017)<\/li>\n\n\n\n
  71. Y.Toba*<\/strong>, \u201cClustering properties of infrared bright dust-obscured galaxies selected with HSC and WISE\u201d, The 6th Subaru International Conference<\/a>, Hiroshima, Japan, (December, 2016)<\/li>\n\n\n\n
  72. Y.Toba*<\/strong>, \u201cSearch for Hyperluminous Infrared Dust-obscured Galaxies Selected with WISE and SDSS\u201d, East-Asia AGN workshop 2016<\/a> , SNU, Seoul, (September, 2016)<\/li>\n\n\n\n
  73. Y.Toba*<\/strong>, \u201cDust Obscured Galaxies viewed with Subaru Hyper Suprime-Cam\u201d,  ASIAA Colloquium<\/a>, ASIAA, Taiwan (June, 2016)<\/li>\n\n\n\n
  74. Y.Toba*<\/strong>, \u201cStatistical properties of Dust Obscured Galaxies revealed by HSC-SSP data with infrared data\u201d, NTHU Astronomy Colloquium, NTHU, Taiwan (April, 2016) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  75. Y.Toba*<\/strong>, \u201cClustering properties of IR-bright dust-obscured galaxies viewed with HSC and WISE\u201d, HSC collaboration meeting 2016, IPMU, Japan, (August, 2016)<\/li>\n\n\n\n
  76. Y.Toba*<\/strong>, \u201cStatistical Properties of Dust Obscured Galaxies discovered by HSC, VIKING, and WISE\u201d, Subaru Users\u2019 Meeting FY2015, Shizuoka, Japan, (January, 2016)<\/li>\n\n\n\n
  77. Y.Toba*<\/strong>, T.Nagao, M.Kajisawa, Y.Matsuoka, \u201cClustering properties of IR-bright DOGs discovered by HSC, VIKING, and WISE\u201d, HSC collaboration meeting 2016<\/a>, ASIAA, Taiwan (January 2016)<\/li>\n\n\n\n
  78. Y.Toba<\/strong>*, \u201cProgress report and future plan of studies on Dust Obscured Galaxies\u201d,  HSC\/AGN Conference, Kagoshima, Japan, (December, 2015)<\/li>\n\n\n\n
  79. Y.Toba*<\/strong>, \u201cIR Luminosity function and luminosity density of the IR bright Dust Obscured Galaxies newly discovered by the Hyper Suprime-Cam on Subaru Telescope\u201d, Demographics and environment of AGN from multi-wavelength surveys, Chania, Greece (September, 2015)<\/li>\n\n\n\n
  80. Y.Toba*<\/strong>, T.Nagao, M.A.Strauss,and HSC DOGs team, \u201cEarly science result from AGN WG (Hyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE)\u201d, HSC collaboration meeting, Princeton, USA (July, 2015)<\/li>\n\n\n\n
  81. Y.Toba*<\/strong>, T.Nagao, M. A. Strauss, K.Aoki, T. Goto, M.Imanishi, T.Kawaguchi, Y.Terashima, Y.Ueda, K.Bundy, H.Inami, Y.Komiyama, R H.Lupton, H.Matsuhara, Y.Matsuoka, T.Morokuma, N.Oi, M.Onoue, S.Oyabu, P.Price,  \u201cHyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE\u201d, East-Asia AGN Workshop 2015<\/a>, Changchun, China (July, 2015)<\/li>\n\n\n\n
  82. Y.Toba<\/strong>, T.Nagao, M.A Strauss, K.Aoki, T.Goto, M.Imanishi, T.Kawaguchi, Y.Terashima, Y.Ueda, H.Inami, H.Matsuhara, N.Oi, S.Oyabu, \u201cHyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru Telescope and WISE\u201d, Unveiling the AGN-galaxy evolution connection<\/a>, Puerto Varas, Chile, (March, 2015)<\/li>\n\n\n\n
  83. Y.Toba*<\/strong>, T.Nagao, M.A Strauss, K.Aoki, T.Goto, M.Imanishi, T.Kawaguchi, Y.Terashima, Y.Ueda, H.Inami, H.Matsuhara, N.Oi, S.Oyabu,  \u201cPhotometric properties of IR bright Dust Obscured Galaxies\u201d, Evolution of SMBHs with HSC: First results from initial dataset<\/a>, ASIAA, Taipei, Taiwan (December, 2014)<\/li>\n\n\n\n
  84. Y.Toba*<\/strong>, \u201cLuminosity and Redshift Dependence of the Covering Factor of Active Galactic Nuclei viewed with WISE and Sloan Digital Sky Survey\u201d, Friday Lunchtime Astronomy Talks, Durham  University, U.K. (July, 2014) [Invited]<\/strong><\/mark><\/li>\n\n\n\n
  85. Y.Toba<\/strong>, S.Oyabu, H.Matsuhara, M.Malkan, T.Wada, Y.Ohyama, S.Takita, and C.Yamauchi, \u201cLuminosity Dependence of the Covering Factor of the Dust Torus in Active Galactic Nuclei Revealed by AKARI\u201d, THE UNIVERSE IN THE LIGHT OF AKARI and Synergy with future Large Space Telescopes,<\/a> Oxford, U.K. (July, 2014)<\/li>\n\n\n\n
  86. Y.Toba<\/strong>, T.Nagao, Y.Terashima, Y.Ueda, S.Oyabu, H.Matsuhara, N.Oi, T.Goto, M.Imanishi, K.Aoki, T.Kawaguchi, H.Inami, M.Strauss, \u201cSearch for “growing up BHs” in the Dust Obscured Galaxies at z~2\u201d, Quasar science with HSC: Toward the first results<\/a>, ASIAA, Taipei (January, 2014)<\/li>\n\n\n\n
  87. Y.Toba*<\/strong>, S.Oyabu, H.Matsuhara, M.Malkan, P.Gandhi, T.Nakagawa, N.Isobe, M.Shirahata, N.Oi, Y.Ohyama, S.Takita, C.Yamauchi, K.Yano, \u201cLuminosity and redshift dependence of covering factor of dust torus viewed with WISE and SDSS\u201d, EAST-ASIA AGN WORKSHOP 2013<\/a>, Hokkaido, Japan (September, 2013)<\/li>\n\n\n\n
  88. Y.Toba<\/strong>, \u201cSearch for dust-free quasars at z > 6 using SPICA MCS photometry\u201d, SPICA Science Conference 2013 From Exoplanets to Distant Galaxies:SPICA’s New Window on the Cool Universe, Tokyo, Japan (June, 2013)<\/li>\n\n\n\n
  89. Y.Toba*<\/strong>, S.Oyabu, D.Ishihara, H.Matsuhara, T.Wada, S.Takita, Y.Ohyama, M.Malkan, \u201cLuminosity and redshift dependence of covering factor of dust torus viewed with AKARI and WISE\u201d, Torus Workshop 2012<\/a>, University of Texas, San Antonio, USA (December, 2012)<\/li>\n\n\n\n
  90. Y.Toba*<\/strong>, S.Oyabu, D.Ishihara, H.Matsuhara, T.Wada, S.Takita, Y.Ohyama, M.Malkan, \u201cLuminosity dependent covering factor of the dust torus around AGN viewed with AKARI and WISE\u201d, Workshop on: Nuclei of Seyfert galaxies and QSOs-Central engine & conditions of star formation<\/a>, Max-Planck-Institute for Radioastronomy (MPIfR), Bonn, Germany (November, 2012)<\/li>\n\n\n\n
  91. Y.Toba<\/strong>, S.Oyabu, H.matsuhara, M.Malkan, D.Ishihara, T.Wada, Y.Ohyama, S.Takita, C.Yamauchi,  \u201cThe mid-infrared Luminosity Function of Galaxies with AKARI to WISE\u201d, AGN Workshop 2012 in Jeju<\/a>, Korea, (September, 2012)<\/li>\n\n\n\n
  92. Y.Toba*<\/strong>, S.Oyabu, H.Matsuhara, D.Ishihara, T.Wada, Y.Ohyama, H.Kataza, M.Malkan, S.Takita, \u201cThe Mid-Infrared Luminosity Function of Galaxies using AKARI mid-infrared All-Sky Survey Catalogue\u201d, The Second AKARI Conference: A Panoramic View of the Dusty Universe, Jeju, Korea (February, 2012)<\/li>\n\n\n\n
  93. Y.Toba<\/strong>, S.Oyabu, H.Matsuhara, D.Ishihara, T.Wada , Y.Ohyama, H.Kataza, M.Malkan, S.Takita, \u201cThe Mid-Infrared Luminosity Function of Galaxies using AKARI mid infrared All-Sky Survey Catalogue\u201d, Through the Infrared Looking Glass: A Dusty View of Galaxy and AGN Evolution<\/a>, Pasadena, USA, (October, 2011)<\/li>\n\n\n\n
  94. Y.Toba<\/strong>, S.Oyabu, H.Matsuhara, M.Malkan, D.Ishihara, T.Wada, H.Kataza, Y.Ohyama, S.Takita, \u201cThe Mid-Infrared luminosity function of galaxies using the AKARI mid-infrared All-Sky Survey Catalogue\u201d, IAU Symposium 284 The Spectral Energy Distribution 2011<\/a>, University of Central Lancashire, Preston, UK (September, 2011)<\/li>\n\n\n\n
  95. Y.Toba<\/strong>, S.Oyabu, D.Ishihara, H.Matsuhara, T.Wada, Y.Ohyama, M.Malkan, \u201cThe optical spectrum classification of mid-infrared excess sources found by AKARI All-Sky Survey\u201d, The first year of MAXI 4th Work Shop<\/a>,  Aoyama, Tokyo, Japan (December, 2010)<\/li>\n\n\n\n
  96. Y.Toba<\/strong>, S.Oyabu, H.Matsuhara, D.Ishihara, T.Wada, Y.Ohyama, H.Kataza, S.Takita, “Search for Active Galactic Nuclei by using AKARI mid-infrared All-Sky Survey Catalogue”, JSPS Summer Program 2010, Kanagawa, Japan (June, 2010)<\/li>\n<\/ol>\n\n\n\n

    \u203b \u4e3b\u8457\u767a\u8868\u306e\u307f\u63b2\u8f09 \uff08*\u306f\u53e3\u982d\u767a\u8868\uff09<\/strong><\/p>\n\n\n\n

    Domestic Conference\/Seminar\uff08\u56fd\u5185\u5b66\u4f1a\/\u30bb\u30df\u30ca\u30fc\uff09\u8a0876\u4ef6<\/h2>\n\n\n\n
      \n
    1. \u9ce5\u7fbd \u5100\u6a39<\/strong>*\u3001\u300c\u3059\u3070\u308bPFS\u30fbEuclid\u30fbLSST\u6642\u4ee3\u306e\u30d3\u30c3\u30b0\u30c7\u30fc\u30bf\u306b\u57fa\u3065\u304f\u6d3b\u52d5\u9280\u6cb3\u6838\u7814\u7a76\u300d\u3001\u30d3\u30c3\u30af\u30c7\u30fc\u30bf\u30a2\u30b9\u30c8\u30ed\u30ce\u30df\u30fc<\/a>\u3001\u7b51\u6ce2\u5927\u5b66\uff082025\u5e745\u6708) [\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    2. Yoshiki Toba<\/strong>, Keito Masu, Naomi Ota, Zhen-Kai Gao, Masatoshi Imanishi, Anri Yanagawa, Satoshi Yamada, Itsuki Dosaka, Takumi Kakimoto, Seira Kobayashi, Neiro Kurokawa, Aika Oki, Sorami Soga, Kohei Shibata, Sayaka Takeuchi, Yukana Tsujita, Tohru Nagao, Masayuki Tanaka, Yoshihiro Ueda, Wei-Hao Wang, Discovery of a hyperluminous quasar at z = 1.62 with Eddington ratio > 3 in the eFEDS field confirmed by KOOLS-IFU on Seimei Telescope, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u6c34\u6238\u5e02\u6c11\u4f1a\u9928\uff082025\u5e743\u6708)<\/li>\n\n\n\n
    3. Yoshiki Toba*<\/strong>, Aoi Hashiguchi, Naomi Ota, Masamune Oguri, Nobuhiro Okabe, Yoshihiro Ueda, Masatoshi Imanishi and CAMIRA-AGN collaboration, AGN properties of about 1 million member galaxies of galaxy groups and clusters at z < 1.4 based on the Subaru Hyper Suprime-Cam survey, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u6c34\u6238\u5e02\u6c11\u4f1a\u9928\uff082025\u5e743\u6708)<\/li>\n\n\n\n
    4. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300ceROSITA \u00d7 Seimei \u00d7 JCMT\u3067\u63a2\u308b\u9280\u6cb3\u3068\u8d85\u5de8\u5927\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u5171\u9032\u5316\u306e\u6700\u76db\u671f\u300d\u3001\u7b2c2\u56de\u4fe1\u5dde\u5927\u5b66\uff0b\u611b\u5a9b\u5927\u5b66\u5408\u540c\u7814\u7a76\u4f1a<\/a>\u3001\u611b\u5a9b\u5927\u5b66\uff082024\u5e7411\u6708\uff09<\/li>\n\n\n\n
    5. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u3059\u3070\u308bHyper Suprime-Cam\u3067\u898b\u3064\u304b\u3063\u305f\u9280\u6cb3\u7fa4\u30fb\u9280\u6cb3\u56e3\u306b\u304a\u3051\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u767a\u73fe\u3068\u74b0\u5883\u4f9d\u5b58\u6027\u300d\u3001\u7b2c157\u56de\u5b87\u5b99\u9032\u5316\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\u8ac7\u8a71\u4f1a\u3001\u611b\u5a9b\u5927\u5b66 (2024\u5e7411\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    6. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300ceROSITA\u00d7\u305b\u3044\u3081\u3044\u7269\u8a9e ~\u5b87\u5b99\u3067\u4e00\u756a\u660e\u308b\u3044\u9280\u6cb3\u63a2\u3057~\u300d\u3001\u30cf\u30ef\u30a4\u89b3\u6e2c\u6240-\u79d1\u5b66\u7814\u7a76\u90e8 \u5408\u540c\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\u3001\u56fd\u7acb\u5929\u6587\u53f0\uff082024\u5e7411\u6708\uff09<\/li>\n\n\n\n
    7. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300ceROSITA\u3068KOOLS-IFU\u306e\u30bf\u30c3\u30b0\u3067\u5b9f\u73fe\u3057\u305f\u5b87\u5b99\u306e\u6b63\u5348\u306b\u8f1d\u304fSuper-Eddington\u30af\u30a8\u30fc\u30b5\u30fc\u306e\u767a\u898b\u300d\u30012024\u5e74\u5ea6\u305b\u3044\u3081\u3044\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0 \u301c\u4e16\u754c\u3092\u99c6\u3051\u306c\u3051\u308b\u305b\u3044\u3081\u3044\u306e\u6280\u8853\u301c<\/a>\u3001\u5009\u6577\u82b8\u6587\u9928 (2024\u5e749\u6708)<\/li>\n\n\n\n
    8. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u8d85\u5de8\u5927\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u306e\u6210\u9577\u3068\u74b0\u5883\u300d\u3001\u7b2c183\u56de\u7d20\u7c92\u5b50\u30fb\u5b87\u5b99\u7269\u7406\u5b66\u7814\u7a76\u4f1a<\/a>\u3001\u4fe1\u5dde\u5927\u5b66 (2024\u5e746\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    9. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cHSC\u3067\u898b\u3064\u304b\u3063\u305f\u9280\u6cb3\u56e3\u30e1\u30f3\u30d0\u30fc\u9280\u6cb3100\u4e07\u5929\u4f53\u4e2d\u306b\u6f5c\u3080AGN\u6d3b\u52d5\u3068\u74b0\u5883\u4f9d\u5b58\u6027\u300d\u3001\u6700\u5148\u7aef\u306e\u89b3\u6e2c\u88c5\u7f6e\u3068\u7406\u8ad6\u306e\u4e21\u8f2a\u3067\u63a2\u308b\u964d\u7740\u73fe\u8c61\u306e\u7269\u7406\u3001\u4eac\u90fd\u5927\u5b66 (2024\u5e745\u6708)<\/li>\n\n\n\n
    10. Yoshiki Toba*<\/strong>, Yoshiki Matsuoka, Tohru Nagao, Masayuki Akiyama, Kohei Ichikawa, Mitsuru Kokubo, Hisakazu Uchiyama, Hideki Umehata, and PFS-SSP GE AGN subWG, AGN sciences with PFS-SSP galaxy evolution survey, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u6771\u4eac\u5927\u5b66 (2024\u5e743\u6708)<\/li>\n\n\n\n
    11. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cPFS-SSP\u306b\u3088\u308bAGN\u30b5\u30a4\u30a8\u30f3\u30b9\u691c\u8a0e\u72b6\u6cc1\u306e\u7d39\u4ecb\u300d\u3001\u7b2c1\u56de PFS-AGN \u30bf\u30a6\u30f3\u30df\u30fc\u30c6\u30a3\u30f3\u30b0<\/a>\u3001\u65e9\u7a32\u7530\u5927\u5b66\uff082024\u5e743\u6708\uff09[\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    12. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u3059\u3070\u308bHSC\u306b\u3088\u308bAGN\u30b5\u30a4\u30a8\u30f3\u30b9\u3068\u4eca\u5f8c\u306e\u5c55\u671b\u300d\u3001\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u5927\u7814\u7a76\u4f1a ~\u661f\u8cea\u91cf\u304b\u3089\u8d85\u5de8\u5927\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u307e\u3067~<\/a>\u3001\u5fa1\u6bbf\u5834\u9ad8\u539f\u30db\u30c6\u30eb\uff082024\u5e742\u6708\uff09[\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    13. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u767a\u73fe\u3068\u74b0\u5883\u300d\u3001\u30cf\u30ef\u30a4\u89b3\u6e2c\u6240-\u79d1\u5b66\u7814\u7a76\u90e8 \u5408\u540c\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\u3001\u56fd\u7acb\u5929\u6587\u53f0\uff082023\u5e7410\u6708\uff09<\/li>\n\n\n\n
    14. \u9ce5\u7fbd\u5100\u6a39*<\/strong>, \u6a4b\u53e3\u8475, \u592a\u7530\u76f4\u7f8e, \u67f4\u7530\u5b9f\u685c, \u67f3\u5ddd\u664f\u91cc, \u5409\u672c\u611b\u4f7f, \u5927\u6817\u771f\u5b97, \u5ca1\u90e8\u4fe1\u5e83, \u4e0a\u7530\u4f73\u5b8f, \u4eca\u897f\u660c\u4fca, \u5c71\u4e0b\u62d3\u6642, \u5c71\u7530\u667a\u53f2, \u5f8c\u85e4\u53cb\u55e3, \u5c0f\u5c71\u821c\u5e73, \u674e\u5efa\u92d2, \u4e09\u77f3\u90c1\u4e4b, \u4f5c\u7530\u7693\u57fa, \u9577\u5c3e\u900f, \u5927\u6728\u5e73, \u5bfa\u5cf6\u96c4\u4e00 , \u897f\u6fa4\u6df3, \u767b\u53e3\u6681, Malte Schramm, “AGN number fraction in galaxy groups and clusters at z < 1.4 from the Subaru Hyper Suprime-Cam survey,” \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u540d\u53e4\u5c4b\u5927\u5b66 (2023\u5e749\u6708)<\/li>\n\n\n\n
    15. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u8d64\u5916\u7dda (WISE) \u00d7 X\u7dda (eROSITA) \u5168\u5929\u63a2\u67fb\u3067\u63a2\u308b\u5b87\u5b99\u3067\u6700\u3082\u660e\u308b\u3044\u9280\u6cb3\u63a2\u67fb\u300d\u3001\u30d7\u30e9\u30cd\u30bf\u30ea\u30a6\u30e0\u3067\u4fef\u77b0\u3059\u308b\u591a\u6ce2\u9577\u5168\u5929\/\u5e83\u57df\u30b5\u30fc\u30d9\u30a4<\/a>\u3001\u540d\u53e4\u5c4b\u5e02\u79d1\u5b66\u9928 \uff082023\u5e747\u6708)<\/li>\n\n\n\n
    16. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u9280\u6cb3\u7fa4\u30fb\u9280\u6cb3\u56e3 vs. \u30d5\u30a3\u30fc\u30eb\u30c9: \u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u767a\u73fe\u3068\u74b0\u5883\u4f9d\u5b58\u6027\u300d\u3001\u7b2c11\u56de \u5c71\u7530\u7814\u7a76\u4f1a\u300c\u5b87\u5b99\u306b\u304a\u3051\u308b\u964d\u7740\u73fe\u8c61 \uff5e\u6d3b\u52d5\u6027\u30fb\u591a\u69d8\u6027\u306e\u6e90\uff5e\u300d<\/a>\u3001\u4eac\u90fd\u5927\u5b66 (2023\u5e746\u6708)<\/li>\n\n\n\n
    17. Yoshiki Toba*<\/strong>, Satoshi Yamada, Kazuya Matsubayashi, Shuhei Koyama, Koki Terao, Hideyuki Izumiura, Hiroyuki Maehara, Aoi Moriya, Aoi Hashiguchi, Naomi Ota, Mio Shibata, Anri Yanagawa Yoshihiro Ueda, Kouji Ohta, Shoji Ogawa, Naoki Yonekura, Tohru Nagao, Masaru Kajisawa, Yoshiki Matsuoka, Masayuki Akiyama, Akatoki Noboriguchi, and collaborators, “Optical IFU Observations of GOALS Sample with KOOLS-IFU on Seimei Telescope: Initial results of 9 U\/LIRGs at z < 0.04\u201d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u7acb\u6559\u5927\u5b66 (2023\u5e743\u6708)<\/li>\n\n\n\n
    18. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cAGN\u30b5\u30a4\u30a8\u30f3\u30b9\uff1a\u5149\u8d64\u5916\u30c7\u30fc\u30bf\u3068JEDI\u3068\u306e\u30b7\u30ca\u30b8\u30fc\u300d\u3001\u7b2c22\u56de\u9ad8\u5b87\u9023\u7814\u7a76\u4f1a<\/a>\u3001\u95a2\u6771\u5b66\u9662\u5927\u5b66 (2023\u5e743\u6708) [\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    19. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u677e\u5ca1\u826f\u6a39\u3001\u9577\u5c3e\u900f\u3001\u4e09\u6fa4\u900f\u3001John Silverman\u3001\u300cPFS\u4f59\u5270\u30d5\u30a1\u30a4\u30d0\u30fc\u3092\u7528\u3044\u305fAGN\u30b5\u30a4\u30a8\u30f3\u30b9\u6848\u300d\u3001PFS\u79d1\u5b66\u904b\u7528\u306b\u95a2\u3059\u308b\u30b3\u30df\u30e5\u30cb\u30c6\u30a3\u30fc\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\u3001\u30aa\u30f3\u30e9\u30a4\u30f3 (2022\u5e7410\u6708\uff09<\/li>\n\n\n\n
    20. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u8d85\/\u9ad8\u5149\u5ea6\u8d64\u5916\u7dda\u9280\u6cb3 (U\/LIRGs) \u306e\u53ef\u8996\u9762\u5206\u5149\u89b3\u6e2c\u3067\u3055\u3050\u308b\u9280\u6cb3\u5408\u4f53\u3068\u96fb\u96e2\u30ac\u30b9\u30a2\u30a6\u30c8\u30d5\u30ed\u30fc\u306e\u95a2\u4fc2\u300d\u3001\u4eac\u90fd\u5927\u5b663.8m\u671b\u9060\u93e1\u5354\u8b70\u4f1a\u3001\u30aa\u30f3\u30e9\u30a4\u30f3\uff082022\u5e749\u6708\uff09[\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    21. Yoshiki Toba*<\/strong>, Teng Liu, Tanya Urrutia, Mara Salvato, Junyao Li, Yoshihiro Ueda, and eROSITA\u2013HSC AGN collaboration, “The eROSITA Final Equatorial-Depth Survey (eFEDS): A multiwavelength view of WISE mid-infrared galaxies\/active galactic nuclei”\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u65b0\u6f5f\u5927\u5b66 (2022\u5e749\u6708)<\/li>\n\n\n\n
    22. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u8fd1\u508dU\/LIRGs \u306e\u53ef\u8996\u9762\u5206\u5149\u89b3\u6e2c\u3067\u3055\u3050\u308b\u9280\u6cb3\u5408\u4f53\u3068\u96fb\u96e2\u30ac\u30b9\u30a2\u30a6\u30c8\u30d5\u30ed\u30fc\u306e\u95a2\u4fc2\u300d\u30012022\u5e74\u5ea6\u305b\u3044\u3081\u3044\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0<\/a>\u3001\u30aa\u30f3\u30e9\u30a4\u30f3\uff082022\u5e747\u6708\uff09[\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    23. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cSPICA\u3067\u691c\u8a0e\u3057\u305f high-z AGN \u30b5\u30a4\u30a8\u30f3\u30b9\u306e\u7d39\u4ecb\u3068\u5357\u6975\u30c6\u30e9\u30d8\u30eb\u30c4\u671b\u9060\u93e1\u3078\u306e\u5c55\u671b\u300d\u3001\u5357\u6975\u304b\u3089\u9060\u8d64\u5916\u7dda-\u30c6\u30e9\u30d8\u30eb\u30c4\u6ce2\u3067\u63a2\u308b\u5b87\u5b99\u3001\u56fd\u7acb\u6975\u5730\u7814\u7a76\u6240\u3068online\u306e\u30cf\u30a4\u30d6\u30ea\u30c3\u30c9\uff082022\u5e743\u6708\uff09[\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    24. Yoshiki Toba*<\/strong>, Marcella Brusa, Teng Liu, Johannes Buchner, Yuichi Terashima, Tanya Urrutia, Mara Salvato, and eROSITA-HSC AGN collaboration, “eROSITA view of an extremely infrared-luminous AGN at z = 1.87″\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001zoom\u306b\u3088\u308bweb\u4f1a\u8b70 (2022\u5e743\u6708)<\/li>\n\n\n\n
    25. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u4e2d\u9593\u8d64\u5916\u7dda\u30b5\u30fc\u30d9\u30a4\u306b\u3088\u308b\u57cb\u3082\u308c\u305fAGN\u306e\u63a2\u67fb\uff1a\u73fe\u72b6\u306e\u307e\u3068\u3081\u3068FORCE\u3078\u306e\u671f\u5f85\u300d\u3001\u7b2c\uff15\u56deFORCE\u7814\u7a76\u4f1a (\u57cb\u3082\u308c\u305fAGN\u306e\u5b87\u5b99\u8ad6\u7684\u9032\u5316)<\/a>\u3001\u4eac\u90fd\u5927\u5b66\uff082021\u5e7412\u6708\uff09[\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    26. Yoshiki Toba*<\/strong>, Yoshihiro Ueda, Poshak Gandhi, Claudio Ricci, Denis Burgarella, Veronique Buat, Tohru Nagao, Shinki Oyabu, Hideo Matsuhara, Bau-Ching Hsieh, “How does the polar dust affect the correlation between dust covering factor and Eddington ratio in type 1 quasars selected from the SDSS DR16?”\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001zoom\u306b\u3088\u308bweb\u4f1a\u8b70 (2021\u5e749\u6708)<\/li>\n\n\n\n
    27. \u9ce5\u7fbd\u5100\u6a39<\/strong>\u3001\u5b88\u5c4b\u78a7\u3001\u592a\u7530\u76f4\u7f8e\u3001\u5c71\u7530\u667a\u53f2\u3001\u57ce\u77e5\u78e8\u3001 \u677e\u6797\u548c\u4e5f\u3001\u6a4b\u53e3\u8475\u3001\u67f4\u7530\u5b9f\u685c \u3001\u7f8e\u91cc\u3089\u306a\u3001\u4e0a\u7530\u4f73\u5b8f\u3001\u300c\u305b\u3044\u3081\u3044\u671b\u9060\u93e1 KOOLS-IFU \u53ef\u8996\u9762\u5206\u5149\u89b3\u6e2c\u3067\u63a2\u308b NGC 7674 \u306e AGN\u6d3b\u52d5\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001zoom\u306b\u3088\u308bweb\u4f1a\u8b70 (2021\u5e749\u6708)<\/li>\n\n\n\n
    28. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001eROSITA early science highlights\u3001\u6c34\u66dc\u96d1\u8a8c\u4f1a\u3001\u4eac\u90fd\u5927\u5b66 (2021\u5e747\u6708)<\/li>\n\n\n\n
    29. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cG-REX\u3067\u63a2\u308b dust-obscured galaxies\/AGNs\u300d\u3001G-REX (+\u4e2d\u9593\u8d64\u5916\u9ad8\u5206\u6563\u5206\u5149) \u30b5\u30a4\u30a8\u30f3\u30b9\u691c\u8a0e\u4f1a<\/a>\u3001zoom\u306b\u3088\u308bweb\u4f1a\u8b70 (2021\u5e743\u6708) [\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    30. Yoshiki Toba<\/strong>*, Tomotsugu Goto, Nagisa Oi, Ting-Wen Wang Seong Jin Kim, Simon C.-C. Ho, and the AKARI-NEP team, “Search for Optically Dark Infrared Galaxies without Counterparts of Subaru Hyper Suprime-Cam in the AKARI North Ecliptic Pole Wide Survey Field, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001zoom\u306b\u3088\u308bweb\u4f1a\u8b70 (2021\u5e743\u6708)<\/li>\n\n\n\n
    31. Yoshiki Toba<\/strong>*, Wei-Hao Wang, Tohru Nagao, Yoshihiro Ueda, Junko Ueda, Chen-Fatt Lim, Yu-Yen Chang, Toshiki Saito, Ryohei Kawabe, “SOFIA View of an Extremely Luminous Infrared Galaxy: WISE 1013+6112″\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u5f18\u524d\u5927\u5b66 (zoom\u306b\u3088\u308bweb\u4f1a\u8b70\uff09 (2020\u5e749\u6708)<\/li>\n\n\n\n
    32. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u3042\u304b\u308a\u300d\u5317\u9ec4\u6975\u9818\u57df\u591a\u6ce2\u9577\u30c7\u30fc\u30bf\u3092\u7528\u3044\u305f\u53ef\u8996\u5149\u7dda\u3067 “dark” \u306a\u8d64\u5916\u7dda\u9280\u6cb3\u63a2\u67fb\u3001\u6c34\u66dc\u96d1\u8a8c\u4f1a\u3001\u4eac\u90fd\u5927\u5b66 (2020\u5e747\u6708)<\/li>\n\n\n\n
    33. \u9ce5\u7fbd\u5100\u6a39<\/strong>*\u3001\u300cIRSA\u306e\u7d39\u4ecb\u3068\u591a\u6ce2\u9577\u30c7\u30fc\u30bf\u306e\u91cd\u8981\u6027\u300d, \u7b2c\u4e8c\u56de\u30c7\u30fc\u30bf\u30a2\u30fc\u30ab\u30a4\u30d6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7<\/a>\u3001\u56fd\u7acb\u5929\u6587\u53f0\uff08zoom\u306b\u3088\u308bweb\u4f1a\u8b70\uff09 (2020\u5e743\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    34. Yoshiki Toba<\/strong>, Satoshi Yamada, Yoshihiro Ueda, Claudio Ricci, Yuichi Terashima, Tohru Nagao, Wei-Hao Wang, Atsushi Tanimoto, Taiki Kawamuro, “NuSTAR Discovery of a Compton-thick Dust-obscured Galaxy WISEJ0825+3002″\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u7b51\u6ce2\u5927\u5b66 (2020\u5e743\u6708)<\/li>\n\n\n\n
    35. \u9ce5\u7fbd\u5100\u6a39<\/strong>*\u3001”Dust properties of AGNs in the early Universe”, SPICA\u30b5\u30a4\u30a8\u30f3\u30b9\u691c\u8a0e\u4f1a\u30fb\u4e2d\u9593\u5831\u544a\u4f1a\u3001\u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240 (2019\u5e7411\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    36. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cKOOLS IFU\u3092\u7528\u3044\u305f\u8fd1\u508d\u8d85\/\u9ad8\u5149\u5ea6\u8d64\u5916\u7dda\u9280\u6cb3\u306e\u89b3\u6e2c\u300d\u3001\u9762\u5206\u5149\u7814\u7a76\u4f1a2019<\/a>\u3001\u56fd\u7acb\u5929\u6587\u53f0 (2019\u5e7411\u6708) [\u62db\u5f85\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    37. Yoshiki Toba*<\/strong>, Takuji Yamashita, Tohru Nagao, Wei-Hao Wang, Yoshihiro Ueda, Kohei Ichikawa, WERGS project, “A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties derived from the SED Fitting with Optical, Infrared, and Radio Data”, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u718a\u672c\u5927\u5b66 (2019\u5e749\u6708)<\/li>\n\n\n\n
    38. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cGOALS\u3067\u767a\u898b\u3055\u308c\u305f\u8fd1\u508d\u8d85\/\u9ad8\u5149\u5ea6\u8d64\u5916\u7dda\u9280\u6cb3\u306eKOOLS-IFU\u9762\u5206\u5149\u89b3\u6e2c\u300d\u30012019\u5e74\u5ea6\u305b\u3044\u3081\u3044\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0<\/a>\u3001\u4eac\u90fd\u5927\u5b66 (2019\u5e748\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    39. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u3059\u3070\u308b\u671b\u9060\u93e1 Hyper Suprime-Cam \u3068 \u96fb\u6ce2\u671b\u9060\u93e1 VLA FIRST \u3067\u767a\u898b\u3055\u308c\u305f\u96fb\u6ce2\u9280\u6cb3\u306e\u6027\u8cea\u306b\u3064\u3044\u3066 \u300d\u3001\u7b2c117\u56de \u5b87\u5b99\u9032\u5316\u7814\u7a76\u30bb\u30f3\u30bf\u30fc \u8ac7\u8a71\u4f1a\u3001\u611b\u5a9b\u5927\u5b66 (2019\u5e747\u6708)<\/li>\n\n\n\n
    40. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u3059\u3070\u308b HSC\u3068 VLA FIRST \u3067\u898b\u3064\u304b\u3063\u305f\u96fb\u6ce2\u9280\u6cb3\u306e\u6027\u8cea\u300d\u3001\u6c34\u66dc\u96d1\u8a8c\u4f1a\u3001\u4eac\u90fd\u5927\u5b66 (2019\u5e744\u6708)<\/li>\n\n\n\n
    41. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cHSC\u3068FIRST\u3067\u767a\u898b\u3055\u308c\u305f\u53ef\u8996\u5149\u7dda\u3067\u6697\u3044\u96fb\u6ce2\u9280\u6cb3\u306e\u6bcd\u9280\u6cb3\u304a\u3088\u3073\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u306e\u6027\u8cea\u8abf\u67fb\u300d\u3001HSC-AGN \u7406\u8ad6\u73ed\u4f1a\u8b70\u3001\u9e7f\u5150\u5cf6\u5927\u5b66 (2019\u5e743\u6708)<\/li>\n\n\n\n
    42. Yoshiki Toba*<\/strong>, Yoshihiro Ueda, Kenta Matsuoka, Megumi Shidatsu, Tohru Nagao, Yuichi Terashima, Wei-Hao Wang, Yu-Yen Chang, “Does the mid-infrared\u2013hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio?”\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u6cd5\u653f\u5927\u5b66 (2019\u5e743\u6708)<\/li>\n\n\n\n
    43. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cAGN \u306e\u8d64\u5916\u7dda-\u30a8\u30c3\u30af\u30b9\u7dda\u5149\u5ea6\u306e\u30a8\u30c7\u30a3\u30f3\u30c8\u30f3\u6bd4\u4f9d\u5b58\u6027\u306e\u691c\u8a3c\u300d\u3001\u5449AGN\u7814\u7a76\u4f1a\u3001\u5449\u9ad8\u7b49\u5c02\u9580\u5b66\u6821 (2019\u5e742\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    44. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cDust-Obscured Galaxies (DOGs) \u5165\u9580~\u5b87\u5b99\u306b\u6f5c\u3080\u300c\u72ac\u300d\u306e\u898b\u3064\u3051\u65b9~\u300d\u30012018\u5e74\u5ea6\u5f8c\u671f\u7b2c1\u56de\u9662\u751f\u30bb\u30df\u30ca\u30fc\u3001\u5948\u826f\u5973\u5b50\u5927\u5b66 (2018\u5e7412\u6708) [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    45. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001”What is dust-obscured galaxy? “\u3001\u6c34\u66dc\u96d1\u8a8c\u4f1a\u3001\u4eac\u90fd\u5927\u5b66 (2018\u5e7410\u6708)<\/li>\n\n\n\n
    46. Yoshiki Toba*<\/strong>, Junko Ueda, Chen-Fatt Lim, Wei-Hao Wang, Tohru Nagao, Yu-Yen Chang, Toshiki Saito, and Ryohei Kawabe, “Discovery of an Extremely Luminous Dust-obscured Galaxy Observed with SDSS, WISE, JCMT, and SMA”\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u5175\u5eab\u770c\u7acb\u5927\u5b66 (2018\u5e749\u6708)<\/li>\n\n\n\n
    47. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u3059\u3070\u308bHSC-SSP\u3068FIRST\u3067\u898b\u3064\u304b\u3063\u305f \u96fb\u6ce2\u9280\u6cb3\u306e\u8d64\u5916\u7dda\u306e\u6027\u8cea\u300d\u3001HSC-AGN \u7406\u8ad6\u73ed\u4f1a\u8b70\u3001\u611b\u5a9b\u5927\u5b66 (2018\u5e743\u6708)<\/li>\n\n\n\n
    48. Yoshiki Toba*<\/strong>, Shinya Komugi, Tohru Nagao, Takuji Yamashita, Wei-Hao Wang, Masatoshi Imanishi, Ai-Lei Sun, \u201cALMA Observation of an Infrared-bright Dust-Obscured Galaxy with Strong Ionized Gas Outflow\u201d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u5343\u8449\u5927\u5b66 (2018\u5e743\u6708)<\/li>\n\n\n\n
    49. Yoshiki Toba*<\/strong>, Hyun-Jin Bae, Tohru Nagao, Jong-Hak Woo, Wei-Hao Wang, Alexander Y.Wagner, Ai-Lei Sun, Yu-Yen Chang, “Ionized gas outflows in infrared-bright dust-obscured galaxies selected with WISE and SDSS\u201d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u5317\u6d77\u9053\u5927\u5b66\uff082017\u5e749\u6708\uff09<\/li>\n\n\n\n
    50. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cDust-Obscured Galaxies (DOGs) \u5165\u9580\u3000~\u898b\u3064\u3051\u65b9\u3068\u7d71\u8a08\u8abf\u67fb~\u300d\u3001\u7b2c98\u56de\u5b87\u5b99\u9032\u5316\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\u8ac7\u8a71\u4f1a\u3001\u611b\u5a9b\u5927\u5b66\uff082017\u5e747\u6708\uff09[\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    51. Yoshiki Toba*<\/strong>, Tohru Nagao, Wei-Hao Wang, Hideo Matsuhara, Masayuki Akiyama, Tomotsugu Goto, Yusei Koyama, Youich Ohyama, Issei Yamamura, \u201cStellar mass and star formation rate relation of infrared-bright dust-obscured galaxies selected with AKARI far-infrared all-sky survey\u201d\u3001 \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u4e5d\u5dde\u5927\u5b66\uff082017\u5e743\u6708\uff09<\/li>\n\n\n\n
    52. Yoshiki Toba*<\/strong>, Tohru Nagao, Masaru Kajisawa, Taira Oogi, Hiroyuki Ikeda, Wei-Hao Wang, Hideo Matsuhara, HSC-DOGs project member, \u201cTwo-point angular correlation function of Dust Obscured Galaxies discovered by HSC and WISE\u201d\u3001 \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u611b\u5a9b\u5927\u5b66\uff082016\u5e749\u6708\uff09<\/li>\n\n\n\n
    53. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cIntroduction to Infrared-bright dust-obscured galaxies (DOGs) ~Statistical properties revealed by Subaru\/HSC and WISE~ \u300d\u3001\u901f\u5831\u30bb\u30df\u30ca\u30fc\u3001\u5317\u6d77\u9053\u5927\u5b66\uff082017\u5e741\u6708\uff09[\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    54. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cHSC-SSP view of Dust Obscured Galaxies\u300d\u3001\u9280\u6cb3\u9032\u5316\u7814\u7a76\u4f1a2016\u3001\u6771\u5317\u5927\u5b66 (2016\u5e746\u6708)<\/li>\n\n\n\n
    55. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u4e2d\u9593\u8d64\u5916\u7dda\u6e90\u30d5\u30a9\u30ed\u30fc\u30a2\u30c3\u30d7\u300d\u3001PFS \u6226\u7565\u67a0\u89b3\u6e2cAGN\u63a2\u67fb\u691c\u8a0e\u4f1a\u3001\u56fd\u7acb\u5929\u6587\u53f0 (2015\u5e7410\u6708)<\/li>\n\n\n\n
    56. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u9577\u5c3e \u900f\u3001\u300cWISE\u3068SDSS\u3092\u4f75\u7528\u3057\u305fExtremely IR luminous Dust Obscured Galaxies \u63a2\u67fb\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u7532\u5357\u5927\u5b66\uff082015\u5e749\u6708\uff09<\/li>\n\n\n\n
    57. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300cPFS\u6642\u4ee3\u306b\u304a\u3051\u308bAGN\u30b5\u30a4\u30a8\u30f3\u30b9\u30b1\u30fc\u30b9\uff1a(i) 1\u578b\u30fb2\u578bAGN\u306e\u500b\u6570 \u5bc6\u5ea6\u6bd4\u306e\u6c7a\u5b9a(ii) Dust Obscured Galaxies\u306e\u74b0\u5883\u8abf\u67fb\u300d\u3001\u300c\u6d3b\u52d5\u9280\u6cb3\u6838\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d72015 \uff5e\u3059\u3070\u308bPFS\u306e\u767b\u5834\u306b\u5411\u3051\u3066\uff5e\u300d\u3001\u56fd\u7acb\u5929\u6587\u53f0\uff082015\u5e745\u6708\uff09<\/li>\n\n\n\n
    58. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u9577\u5c3e \u900f\u3001\u5bfa\u5cf6 \u96c4\u4e00\u3001\u4eca\u897f \u660c\u4fca\u3001\u9752\u6728 \u8ce2\u592a\u90ce\u3001\u5ddd\u53e3\u4fca\u5b8f\u3001\u5f8c\u85e4 \u53cb\u55e3\u3001\u5927\u85ae \u9032\u559c\u3001\u4e0a\u7530 \u4f73\u5b8f\u3001\u5927\u4e95 \u6e1a\u3001\u677e\u539f \u82f1\u96c4\u3001\u7a32\u898b \u83ef\u6075\u3001Michael A. Strauss\u3001\u300cHSC \u521d\u671f\u30c7\u30fc\u30bf\u3068WISE \u3092\u4f75\u7528\u3057\u305f Dust Obscured Galaxies \u63a2\u67fb\u300d\u3001 \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u5927\u962a\u5927\u5b66\uff082015\u5e743\u6708\uff09<\/li>\n\n\n\n
    59. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u9577\u5c3e \u900f\u3001\u4eca\u897f\u660c\u4fca\u3001\u4e0a\u7530\u4f73\u5b8f\u3001\u5f8c\u85e4\u53cb\u55e3\u3001\u5927\u4e95 \u6e1a\u3001\u5927\u85ae\u9032\u559c\u3001\u9752\u6728\u8ce2\u592a\u90ce\u3001\u677e\u539f\u82f1\u96c4\u3001\u7a32\u898b\u83ef\u6075\u3001\u5bfa\u5cf6\u96c4\u4e00\u3001\u5ddd\u53e3\u4fca\u5b8f\u3001Strauss, M.\u3001\u300c\u4e2d\u9593\u8d64\u5916\u7dda\u3068\u53ef\u8996\u5149\u7dda\u3092\u4f75\u7528\u3057\u305fAGN\/\u9280\u6cb3\u7814\u7a76\u300d, \u8d85\u5de8\u5927\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u7814\u7a76\u63a8\u9032\u9023\u7d61\u4f1a\u30fb\u7b2c2\u56de\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, \u7b51\u6ce2\u5927\u5b66\uff082014\u5e7411\u6708\uff09<\/li>\n\n\n\n
    60. \u9ce5\u7fbd\u5100\u6a39<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u677e\u539f\u82f1\u96c4\u3001\u4e2d\u5ddd\u8cb4\u96c4\u3001\u78ef\u90e8\u76f4\u6a39\u3001\u5927\u4e95\u6e1a\u3001\u7027\u7530\u601c\u3001Gandhi, P\u3001Malkan, M\u3001\u767d\u65d7\u9ebb\u8863\u3001\u5927\u5c71\u967d\u4e00\u3001\u5c71\u5185\u5343\u91cc\u3001\u77e2\u91ce\u5065\u4e00, \u300c\u6bcd\u9280\u6cb3\u304b\u3089\u306e\u8d64\u5916\u7dda\u653e\u5c04\u306e\u5f71\u97ff\u3092\u8003\u616e\u3057\u305f\u6d3b\u52d5\u9280\u6cb3\u6838\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u306e\u8d64\u65b9\u504f\u79fb\u4f9d\u5b58\u6027\u306e\u691c\u8a3c\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a, \u5c71\u5f62\u5927\u5b66\uff082014\u5e749\u6708\uff09<\/li>\n\n\n\n
    61. \u9ce5\u7fbd\u5100\u6a39<\/strong>\u3001\u300c\uff11\u578b\uff12\u578bAGN\u306e\u500b\u6570\u5bc6\u5ea6\u6bd4\u306fAGN\u5149\u5ea6\u3084\u8d64\u65b9\u504f\u79fb\u306b\u4f9d\u5b58\u3059\u308b\u306e\u304b\u300d, \u9280\u6cb3\u9032\u5316\u7814\u7a76\u4f1a2014, \u56fd\u7acb\u5929\u6587\u53f0\u3001\u4e09\u9df9\uff082014\u5e746\u6708\uff09<\/li>\n\n\n\n
    62. \u9ce5\u7fbd\u5100\u6a39*<\/strong>,\u300c\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u30ab\u30d0\u30fc\u30ea\u30f3\u30b0\u30d5\u30a1\u30af\u30bf\u30fc\u306e\u5149\u5ea6\u304a\u3088\u3073\u8d64\u65b9\u504f\u79fb\u4f9d\u5b58\u6027\u306e\u691c\u8a3c\u30682020\u5e74\u4ee3\u306e\u30c8\u30fc\u30e9\u30b9\u7814\u7a76\u300d\u3001\u6d3b\u52d5\u9280\u6cb3\u6838\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7 \uff5e2020\u5e74\u4ee3\u3078\u306e\u5c55\u671b\uff5e, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\uff082014\u5e744\u6708\uff09<\/li>\n\n\n\n
    63. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u677e\u539f\u82f1\u96c4\u3001\u4e2d\u5ddd\u8cb4\u96c4\u3001\u767d\u65d7\u9ebb\u8863\u3001\u78ef\u90e8\u76f4\u6a39\u3001\u5927\u4e95\u6e1a\u3001\u7027\u7530\u601c\u3001Poshak Gandhi, Matt Malkan, \u5927\u5c71\u967d\u4e00\u3001\u5c71\u5185\u5343\u91cc\u3001\u77e2\u91ce\u5065\u4e00\u3001\u300c \u6bcd\u9280\u6cb3\u304b\u3089\u306e\u8d64\u5916\u7dda\u653e\u5c04\u306e\u5f71\u97ff\u3092\u8003\u616e\u3057\u305f\u6d3b\u52d5\u9280\u6cb3\u6838\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u306e\u5149\u5ea6\u4f9d\u5b58\u6027\u306e\u691c\u8a3c\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff082014\u5e743\u6708\uff09<\/li>\n\n\n\n
    64. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u8d64\u5916\u7dda\u5929\u6587\u885b\u661f\u300e\u3042\u304b\u308a\u300f\u30fbWISE\u3092\u7528\u3044\u305f\u8d64\u5916\u7dda\u89b3\u6e2c\u306b\u57fa\u3065\u304f\u6d3b\u52d5\u9280\u6cb3\u6838\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u306e\u4e2d\u5fc3\u6838\u906e\u853d\u7387\u306e\u5149\u5ea6\u304a\u3088\u3073\u8d64\u65b9\u504f\u79fb\u4f9d\u5b58\u6027\u306e\u691c\u8a3c\u300d\u3001\u7b2c54\u56de\u5b87\u5b99\u9032\u5316\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\u8ac7\u8a71\u4f1a\u3001\u611b\u5a9b\u5927\u5b66\uff082014\u5e743\u6708\uff09[\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    65. Y.Toba*<\/strong>, \u201cLuminosity and Redshift Dependence of the Covering Factor of the Dust Torus in Active galactic Nuclei Revealed by Infrared Observations with AKARI and WISE\u201d, LIRA Colloquium, ISAS\/JAXA (2014\u5e742\u6708\uff09<\/li>\n\n\n\n
    66. \u9ce5\u7fbd\u5100\u6a39<\/strong>*\u3001\u300cWISE\u885b\u661f\u3092\u7528\u3044\u305f\u6d3b\u52d5\u9280\u6cb3\u6838\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u306e\u5149\u5ea6\u304a\u3088\u3073\u8d64\u65b9\u504f\u79fb\u4f9d\u5b58\u6027\u306e\u691c\u8a3c]\u300d\u3001\u3064\u304f\u3070\u5b87\u5b99\u30d5\u30a9\u30fc\u30e9\u30e0\u3001\u7b51\u6ce2\u5927\u5b66\u30012013\u5e746\u6708 [\u4f9d\u983c\u8b1b\u6f14]<\/strong><\/mark><\/li>\n\n\n\n
    67. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u677e\u539f\u82f1\u96c4\u3001\u4e2d\u5ddd\u8cb4\u96c4\u3001\u767d\u65d7\u9ebb\u8863\u3001\u78ef\u90e8\u76f4\u6a39\u3001\u7027\u7530\u601c\u3001\u77e2\u91ce\u5065\u4e00\u3001\u5927\u5c71\u967d\u4e00\u3001Matt Malkan\u3001\u5c71\u5185\u5343\u91cc\u3001\u300cWISE\u885b\u661f\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u306e\u5149\u5ea6\u304a\u3088\u3073\u8d64\u65b9\u504f\u79fb\u4f9d\u5b58\u6027\u306e\u691c\u8a3c\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u57fc\u7389\u5927\u5b66\uff082013\u5e743\u6708\uff09<\/li>\n\n\n\n
    68. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u77f3\u539f\u5927\u52a9\u3001\u677e\u539f\u82f1\u96c4\u3001\u548c\u7530\u6b66\u5f66\u3001\u7247\u3056\u5b8f\u4e00\u3001\u7027\u7530\u601c\u3001\u5927\u5c71\u967d\u4e00\u3001 Matt Malkan\u3001\u300c\u300c\u3042\u304b\u308a\u300d\u4e2d\u9593\u8d64\u5916\u7dda\u5168\u5929\u30b5\u30fc\u30d9\u30a4\u3067\u63a2\u308bAGN\u306e\u30c0\u30b9\u30c8\u30c8\u30fc\u30e9\u30b9\u306e\u69cb\u9020\u300d\u3001\u6b21\u4e16\u4ee3\u8d64\u5916\u7dda\u5929\u6587\u885b\u661fSPICA\u304c\u76ee\u6307\u3059\u5b87\u5b99\u661f\u5f62\u6210\u53f2\u3068\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u9032\u5316\u306e\u89e3\u660e\u3001\u540d\u53e4\u5c4b\u5927\u5b66\uff082011\u5e7410\u6708\uff09<\/li>\n\n\n\n
    69. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u77f3\u539f\u5927\u52a9\u3001\u677e\u539f\u82f1\u96c4\u3001\u548c\u7530\u6b66\u5f66\u3001\u7247\u3056 \u5b8f\u4e00\u3001\u7027\u7530 \u601c\u3001\u5927\u5c71\u967d\u4e00\u3001 Matt Malkan\u3001\u300c\u8d64\u5916\u7dda\u5929\u6587\u885b\u661f\u300c\u3042\u304b\u308a\u300d\u4e2d\u9593\u8d64\u5916\u7dda\u5168\u5929\u30b5\u30fc\u30d9\u30a4\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u63a2\u67fb:\u5149\u5ea6\u95a2\u6570\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u79cb\u5b63\u5e74\u4f1a\u3001\u9e7f\u5150\u5cf6\u5927\u5b66\uff082011\u5e749\u6708\uff09<\/li>\n\n\n\n
    70. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u77f3\u539f\u5927\u52a9\u3001\u677e\u539f\u82f1\u96c4\u3001\u548c\u7530\u6b66\u5f66\u3001\u5927\u5c71\u967d\u4e00\u3001Matt Malkan\u3001\u300c\u8d64\u5916\u7dda\u5929\u6587\u885b\u661f\u300c\u3042\u304b\u308a\u300d\u3092\u7528\u3044\u305f\u6d3b\u52d5\u9280\u6cb3\u6838\u63a2\u67fb\u3067\u898b\u3064\u304b\u3063\u305f\u9280\u6cb3\u306e\u5149\u5ea6\u95a2\u6570\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u7b51\u6ce2\uff082011\u5e743\u6708\uff09<\/li>\n\n\n\n
    71. \u9ce5\u7fbd\u5100\u6a39<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u677e\u539f\u82f1\u96c4\u3001\u300c\u8d64\u5916\u7dda\u5929\u6587\u885b\u661f\u300c\u3042\u304b\u308a\u300d\u4e2d\u9593\u8d64\u5916\u7dda\u5168\u5929\u30b5\u30fc\u30d9\u30a4\u30ab\u30bf\u30ed\u30b0\u3068\u53ef\u8996\u30fb\u8fd1\u8d64\u5916\u8ffd\u89b3\u6e2c\u306b\u57fa\u3065\u304fAGN\u63a2\u67fb\u300d\u3001\u8d85\u5e83\u57df\u30b5\u30fc\u30d9\u30a4\u3067\u660e\u304b\u3059\u5de8\u5927\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u3068\u9280\u6cb3\u306e\u5171\u9032\u5316\uff1a\u7406\u8ad6\u30e2\u30c7\u30eb\u3068\u89b3\u6e2c\u6226\u7565\u3001\u6771\u5317\u5927\u5b66\uff082010 \u5e749\u6708\uff09<\/li>\n\n\n\n
    72. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u304d\u3063\u3068\u898b\u3064\u304b\u308b\uff01\u50d5\u3068\u306e\u5171\u540c\u7814\u7a76~SQL\u3068\u5929\u6587\u5b66~\u300d\u3001SOKENDAI Workshop 2010\u3001JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\uff082010\u5e7410\u6708\uff09<\/li>\n\n\n\n
    73. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u5927\u85ae\u9032\u559c\u3001\u677e\u539f\u82f1\u96c4\u3001\u548c\u7530\u6b66\u5f66, \u7247\u3056\u5b8f\u4e00\u3001\u77f3\u539f\u5927\u52a9\u3001\u5927\u5c71\u967d\u4e00\u3001\u7027\u7530\u601c\u3001\u300c\u8d64\u5916\u7dda\u5929\u6587\u885b\u661f\u300c\u3042\u304b\u308a\u300d\u4e2d\u9593\u8d64\u5916\u7dda\u5168\u5929\u30b5\u30fc\u30d9\u30a4\u30ab\u30bf\u30ed\u30b0\u3067\u767a\u898b\u3055\u308c\u305fAGN\u306e\u53ef\u8996\u5206\u5149\u89b3\u6e2c\u7d50\u679c\u300d\u3001\u65e5\u672c\u5929\u6587\u5b66\u4f1a \u6625\u5b63\u5e74\u4f1a\u3001\u5e83\u5cf6\u5927\u5b66\uff082010\u5e743\u6708\uff09<\/li>\n\n\n\n
    74. Y.Toba<\/strong>, S.Oyabu, H.Matsuhara, D.Ishihara, T.Wada, Y.Ohyama, H.Kataza, S.Takita, Search for Active Galactic Nuclei by using AKARI mid-infrared All-Sky Survey Catalogue, \u7dcf\u5408\u7814\u7a76\u5927\u5b66\u9662\u5927\u5b66\u7269\u7406\u79d1\u5b66\u7814\u7a76\u79d1\u5b66\u751f\u30bb\u30df\u30ca\u30fc\u3001\u8c4a\u6a4b\uff082010\u5e743\u6708\uff09<\/li>\n\n\n\n
    75. Y.Toba*<\/strong>, Search for Active Galactic Nuclei by using AKARI mid-infrared All-Sky Survey Catalogue, SOKENDAI Workshop 2009,\u3001\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u52a0\u901f\u5668\u7814\u7a76\u6a5f\u69cb\uff082009\u5e749\u6708\uff09<\/li>\n\n\n\n
    76. \u9ce5\u7fbd\u5100\u6a39*<\/strong>\u3001\u300c\u8d64\u5916\u5929\u6587\u885b\u661f\u300c\u3042\u304b\u308a\u300d\u4e2d\u9593\u8d64\u5916\u7dda\u5168\u5929\u30b5\u30fc\u30d9\u30a4\u30ab\u30bf\u30ed\u30b0\u3092\u7528\u3044\u305f\u300c\u96a0\u3055\u308c\u305f\u300d\u6d3b\u52d5\u9280\u6cb3\u4e2d\u5fc3\u6838\u63a2\u67fb\u300d\u3001\u7b2c39 \u56de\u5929\u6587\u5929\u4f53\u7269\u7406\u82e5\u624b\u590f\u306e\u5b66\u6821\u3001\u7fa4\u99ac\uff082009\u5e747\u6708)<\/li>\n<\/ol>\n\n\n\n

      \u203b \u4e3b\u8457\u767a\u8868\u306e\u307f\u63b2\u8f09 \uff08*\u306f\u53e3\u982d\u767a\u8868\uff09\u8f09<\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"

      International Conference\/Seminar\uff08\u56fd\u969b\u5b66\u4f1a\/\u30bb\u30df\u30ca\u30fc\uff09\u8a0896\u4ef6 \u203b \u4e3b\u8457\u767a\u8868\u306e\u307f\u63b2\u8f09 \uff08*\u306f\u53e3\u982d\u767a\u8868\uff09 Domestic Conference\/Seminar\uff08\u56fd\u5185\u5b66\u4f1a\/\u30bb\u30df\u30ca\u30fc\uff09\u8a0876\u4ef6…<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"tags":[],"_links":{"self":[{"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=\/wp\/v2\/pages\/187"}],"collection":[{"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=187"}],"version-history":[{"count":175,"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=\/wp\/v2\/pages\/187\/revisions"}],"predecessor-version":[{"id":1817,"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=\/wp\/v2\/pages\/187\/revisions\/1817"}],"wp:attachment":[{"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=187"}],"wp:term":[{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/cosmos.phys.sci.ehime-u.ac.jp\/~toba\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=187"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}