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3 15:45-16:15 10:00 12:00-15:30 14:00 10:00 10:00-14:00 D - 24:00 24:
4 LAN PC 1 1 LAN LAN SS18***(***) SSID 19:15 AB 8:00-24:30 7:00 (ss18 info@astro-wakate.sakura.ne.jp) ( ) (7/22-7/25) 12:
5 URL USB (a,b ) a ( 12 3 ) b ( 3 ) PC PC 7 1 ID ID 3 19:30 15 ( 12 3 ) a 4 48
6 (b,c ) 9: :4516:15 16:3017:00 3 ID ID 3 19: ( 12 3 ) PDF 48 5
7 D2 a26 M1 a9 M1 a5 M1 a6 D2 c3 M1 c17 M1 c7 M1 a4 M2 c8 M1 c9 M2 c10 D1 a9 M2 c4 M1 c11 M2 c12 M1 c13 M2 b3 M1 c5 D1 c11 M1 c10 M2 a18 M2 c19 M2 c1 M1 c12 M1 a8 M1 c13 M1 c6 M1 c13 M1 c14 M2 a2 M2 a8 M1 a2 M1 c6 M1 c2 M1 a4 M1 a27 D2 c11 D2 c12 M1 c5 D1 M1 c9 M2 M1 c2 M1 b5 Miwa Yuya M1 a12 M1 a1 M1 b2 LUO Yudong M2 a21 M2 a21 M1 M2 a23 M1 a2 M1 b3 M1 a2 M2 a13 M1 a20 M1 a9 M1 a16 M1 a13 M1 a29 M1 a30 M1 c7 M2 M1 a5 M1 c13 M1 a8 M1 a9 M1 a3 M1 a2 D1 M1 b4 Kobayashi M1 c3 Yukiho M1 b5 M1 a3 M2 a17 M2 a17 M2 c6 D1 a15 M2 a12 M1 c15 M2 a1 M1 b3 D1 a19 D2 a11 M1 c16 M2 a10 M2 a1 M1 c2 M1 a2 M1 c14 M1 a3 M2 b2 M1 M2 a25 M2 a1 M1 c17 M1 c11 M2 c8 M1 M2 c15 M1 a16 D2 b3 M1 a14 M1 a13 M1 a11 M2 a18 D1 b4 M2 a3 M1 M1 M1 a15 M1 a14 M1 a13 M1 b6 M1 b2 M1 a17 M1 c3 M1 c14 M2 a6 M1 a3 M1 c17 M1 c22 M2 c21 M2 c30 M1 c31 M2 c29 M2 c20 M1 c19 M1 c1 M1 a20 M1 c7 M1 b1 M1 a14 M1 M1 a19 M1 c18 M1 a11 M1 a20 D1 c6 M1 a16 M1 a18 M1 c2 M1 c6 M2 b2 B4 c8 D2 c9 M1 M1 Liang Yongming M1 c1 M1 b1 M1 c21 M1 a10 M2 c2 M1 M1 a21 M1 a
8 M2 c6 M2 a22 M2 c7 Sato Tatsuki M1 a1 D2 c25 M1 a9 D1 a6 M2 a25 M1 c22 M2 c26 M2 c11 M2 c24 M1 a2 M1 a27 M1 a15 M2 c20 M2 c15 M2 c23 D1 c12 M1 a21 M2 c5 M2 c8 M1 a1 M1 a4 M2 a3 M2 a7 M1 b1 M1 c27 M1 a19 D1 c12 M1 a1 D1 a18 M1 a7 M1 M1 a5 M1 c17 D1 c3 M1 b3 M1 a14 M1 a20 M1 a5 D1 c9 M1 b1 M1 c1 M1 a22 M1 a5 M1 a6 M2 a10 M1 a9 M2 a7 M2 a28 M2 c4 M1 c10 M2 c1 M1 a8 M1 a24 M1 a19 M1 c20 M2 a11 M1 b3 D1 c1 D1 c2 M2 a10 M2 b7 M1 a10 M1 b6 M1 b2 M1 b4 D1 b1 Yun JeUng M1 c21 ZENKO TET- SUYA D2 M2 c9 D1 c3 D2 c4 M2 a12 D1 c1 M1 a6 M2 c5 M2 c3 M2 c4 M1 c7 M1 c13 M1 a4 M1 b4 D2 c4 M1 a15 M1 c10 M1 a7 M1 a5 M2 a14 M1 a16 OUCHI RY- D1 b1 OMA M1 b2 D1 c4 M1 a7 M1 a12 M1 a12 D2 c15 M1 a17 M1 a7 M1 a26 M1 a12 M1 a7 M1 a23 M1 a11 M2 a19 M1 a22 M2 a4 M2 c18 M1 c7 Sei Shuto M1 c8 M1 a18 M1 c8 M1 a8 M1 M2 c10 M2 M2 c11 M1 a4 M1 a5 M1 a16 M1 a4 M1 c16 M1 b4 M1 b4 M2 a4 M1 c28 D1 b3 M1 c10 M1 c16 Takeuchi M1 c14 Keito M1 a23 D1 a15 Iwashita M1 b8 Kohei M2 a13 M2 a10 M2 a3 M1 c7 M1 c18 M1 c19 D2 c5 D2 c4 D1 c9 M2 a6 M1 b1 D1 a8 M2 c3 M1 b7 M1 b8 M1 c2 M1 c6 M1 b4 M1 a17 D1 c5 D2 b2 48 7
9 :45-15:45 A 14:45 a1 (M1) 15:00 a2 (M1) regular black hole 15:15 a3 (M1) 15:30 b1 ( D1) Gravitational redshift in void-galaxy cross-correlation function in redshift space 15:33 b2 (M1) 15:36 b3 ( D1) AdS 15:39 b4 (M1) :00-18:00 B 17:00 ( ) :00-10:00 A 09:00 a4 (M2) 09:15 a5 (M1) 09:30 a6 ( D1) non-singular 09:45 a7 (M1) Exotic Compact Object Echo Template :30-12:30 C 11:30 a8 (M1) 11:45 a9 (M1) GW :00 a10 (M2) 12:30 a11 () :30-14:30 A 13:30 a12 (M2) lensing baryon physics 13:45 a13 (M2) 14:00 a14 (M1) 14:15 a15 ( D1) 18: :15-19:15 B ( ) :00-10:00 B 09:00 a16 (M1) BAO 09:15 a17 (M1) CMB 21cm 09:30 a18 ( D1) 21-cm 09:45 a19 (M1) :30-12:30 A 11:30 a20 (M1) 11:45 a21 LUO Yudong ( M2) Fluctuations of Primordial Magnetic Field and Its Effect on Big bang Li Problem 12:00 a22 (M1) S 12:15 a23 (M1) :45-15:45 A 14:45 a24 () 15:00 a25 (M2) Higgs G Goldstone mode 15:15 a26 (M1) α-attractor 15:30 a27 (M1) Gravitational Reheating Constraints on Quintessential Inflation c1 (M2) 21-cm c2 (M1) Stacking 21cm 8 48
10 c3 ( D1) N c4 ( D1) c5 (M2) γ c6 ( D1) c7 (M1) Intrinsic Alignments c8 (M2) c9 ( D1) c10 (M1) c11 (M2) 2 c12 (M1) c13 (M1) Matched Filter c14 TakeuchiKeito ( M1) non- Gaussianity c15 ( D2) c16 (M1) Wald c17 (M1) c18 (M2) Primordial Black Holes c19 (M1) c20 (M2) c21 (M2) Multifractional theories c22 (M1) Multifractional theories c23 (M2) c24 (M2) K-Mouflage c25 ( D2) Positivity bound in modified gravity c26 (M2) c27 (M1) Holographic entanglement negativity conjecture c28 (M1) Proca star c29 (M2) c30 (M2) Metamaterial c31 (M1) Variable Hyperbolic Metamterial 48 9
11 :30-14:30 B 13:30 ( ) :00-18:00 A 17:00 a1 (M1) sl Suzaku/HXD-WAM GRB 17:15 a2 (M1) 17:30 a3 (M1) GRB 17:45 b1 (M1) Cooling 17:48 b2 (M2) Tomo-e Gozen Ia colorluminosity relation 17:51 b3 (M1) P 3 T 17:54 b4 (M1) :00-10:00 B 09:00 a4 (M1) 09:15 a5 (M1) X 09:30 a6 (M2) 09:45 b5 (M1) CTA 09:48 b6 (M1) MCMC FSRQ SED 09:51 b7 (M1) Astronomy Letters,2018 Vol.44 No.6 (2018) 09:54 b8 (M1) Hydrodynamically simulating the SS 433- W50 interaction :45-15:45 A 14:45 a7 (M1) 15:00 a8 ( D1) SS433 15:15 a9 ( D1) 15:30 a10 (M2) Swift NGC1275 X :00-18:00 C 17:00 a11 (M1) 17:15 a12 (M1) MAGIC S :30 a13 (M1) Ia 17:45 a14 (M1) WD-WD :15-11:15 A 10:15 a15 (M1) 10:30 a16 (M1) 10:45 a17 (M2) Failed Supernova 11:00 a18 (M1) :30-14:30 B 13:30 ( ) :00-18:00 C 17:00 a19 (M2) 17:15 a20 (M1) NuSTAR SGR X 17:30 a21 (M1) Synchro-Curvature radiation FRB 17:45 a22 (M1) EX c1 ( D1) c2 (M1) BH c3 (M1) CANS+ 3 c4 ( D2) 10 48
12 c6 (M1) c7 (M1) c8 (M1) c9 ( D1) 2 c10 (M2) c11 (M1) c12 ( D1) 4 c13 (M1) FRB c14 (M1) X c15 (M2) c16 (M1) c17 (M1) Common Envelope c18 (M1) c19 (M1) c20 (M2) 4 c21 Yun JeUng ( M1) Improvement points to get more accurate distance value to type Ia supernova through dust extinction c22 (M1) :30-14:30 A 13:30 a1 (M2) Gaia 13:45 a2 (M2) NGC891 14:00 a3 (M2) z 1.0 (2nd) 14:15 b1 (M1) 14:18 b2 (M1) 14:21 b3 (M1) 14:24 b4 (M1) PACS Mrk :15-19:15 A 18:15 a4 (M1) NGC253 18:30 a5 (M1) 18:45 a6 (M1) 19:00 b5 (M1) X 3.5keV 19:03 b6 (M1) NGC :06 b7 (M2) XMM MCXC J :09 b8 IwashitaKohei ( M1) Subaru / Hyper Suprime-Cam :15-11:15 A 10:15 a7 (M2) 10:30 a8 (M2) CO-H 2 X CO 10:45 a9 (M1) CO-H 2 11:00 a10 (M2) COSMOS 48 11
13 :30-12:30 A 11:30 a11 ( D2) 10 SDSS 11:45 a12 (M1) X Seyfart 1 IC 4329A 12:00 a13 (M2) 1 12:15 a14 (M2) NGC 5135 X :30-14:30 B 13:30 ( ) :00-18:00 A 17:00 a15 ( D1) Hyper Suprime-Cam 17:15 a16 (M1) M83 17:30 a17 (M1) 17:45 a18 (M2) Hyper Suprime-Cam z 1 quasar-red galaxy :00-10:00 A 09:00 a19 (M1) 09:15 a20 (M1) 09:30 a21 (M2) HSC z 4Brightest Cluster Galaxy 09:45 a22 (M1) HSC weak lensing X :30-12:30 B 11:30 ( ) :30-14:30 A 13:30 a23 (M2) ALMA 13:45 a24 (M1) ALMA 14:00 a25 (M2) AGN / 14:15 a26 ( D2) :00-18:00 A 17:00 a27 (M1) α 17:15 a28 (M2) VLA-COSMOS 17:30 a29 (M1) HSC Lyα 17:45 a30 (M1) HSC AGN c1 Liang Yongming ( M1) Search for the most massive overdensities at z=2.2 with Subaru HSC c2 (M1) - c3 ( D1) NGC1300 c4 ( D2) X Circinus galaxy c5 ( D1) c6 (M1) c7 (M1) c8 (M2) COSMOS c9 (M1) -HST- c10 (M1) Changing Look Quasar c11 (M1) HSC c12 (M2) Blue horizontal-branch stars 12 48
14 c13 (M1) Gaia DR2 c14 (M1) c15 (M1) JWST c16 (M1) COSMOS c17 (M1) r-process c18 (M1) c19 (M2) Seyfert AGN c20 (M1) ALMA z =6.110 [OIII] 88 µm c21 (M2) :30-14:30 C 13:30 a1 Sato Tatsuki ( M1) X 13:45 a2 (M1) WR 125 X 14:00 a3 (M1) WINERED Y,J 14:15 b1 OUCHI RYOMA ( D1) 14:18 b2 (M1) 14:21 b3 (M1) X 14:24 b4 (M1) :00-18:00 B 17:00 ( ) :00-10:00 C 09:00 a4 (M1) 09:15 a5 (M1) 09:30 a6 (M1) 09:45 a7 (M1) SMART :45-15:45 B 14:45 ( ) c1 (M2) c2 (M2) Hinode-IRIS-ALMA c3 (M2) c4 (M2) SMART/SDDI c5 (M2) II c6 (M2) Hα c7 (M2) G 48 13
15 :00-18:00 C 17:00 a1 (M1) 17:15 a2 (M1) 17:30 a3 (M1) : SNRshock 17:45 b1 (M1) 17:48 b2 ( D2) H 2 O 17:51 b3 (M1) CO :54 b4 (M1) ALMA :15-11:15 B 10:15 ( ) :30-14:30 C 13:30 a4 (M1) HB9 13:45 a5 (M1) 14:00 a6 (M1) : 14:15 a7 (M1) XMM-Newton RGS N49 X :15-11:15 B 10:15 ( ) :45-15:45 C 13:45 a8 (M1) 14:00 a9 (M1) Chandra X RX J hot-spot 14:15 a10 (M1) 14:30 a11 (M1) Boomerang c1 ( D1) CO c2 ( D1) l = 1.2 c3 ( D2) SED c4 (M2) c5 (M1) c6 (M2) c7 (M1) c8 Sei Shuto ( M1) c9 (M2) c10 (M2) Sgr A East c11 (M2) IC
16 :45-15:45 C 14:45 a1 (M2) 15:00 a2 (M1) 15:15 a3 (M2) 15:30 b1 (M1) A 15:33 b2 (M1) 15:36 b3 ( D2) 15:39 b4 ( D1) :15-19:15 B 18:15 ( ) :15-11:15 C 10:15 a4 (M1) -ALMA - 10:30 a5 (M1) Atacama Compact Array 10:45 a6 (M2) : 11:00 a7 (M2) SPH :45-15:45 C 14:45 a8 (M1) 15:00 a9 (M1) 15:15 a10 (M2) - 15:30 a11 (M1) : :15-19:15 C 18:15 a12 (M2) 18:30 a13 (M1) 18:45 a14 (M1) Gas flow around embedded planets: the dependence of outflow speed on the planetary mass 19:00 a15 (M1) N :30-12:30 C 11:30 a16 (M1) Condensation Growth Model of Cloud Particles with Size Distribution for Exoplanetary Atmospheres 11:45 a17 (M2) WASP-80b 12:00 a18 (M2) M habitability G 12:15 a19 ( D1) :00-18:00 B 17:00 (/ ) c1 (M1) c2 (M1) c3 (M2) Present day c4 ( D2) Star formation during collapsing phase in low metallicity environments c5 ( D2) Massive Outflow Driven by Magnetic Effects with High Mass Accretion Rates c6 (M1) c7 (M1) X c8 (B4) CaII c9 ( D2) Herbig Ae/Be ZCMa c10 (M1) c11 ( D1) c12 ( D1) - c13 (M1) : c14 (M1) (SPA) K Th c15 (M2) c16 (M1) SPART c17 (M1) 48 15
17 :45-15:45 B 14:45 ( ) :15-19:15 C 18:15 a1 (M2) 18:30 a2 (M1) SWIMS 18:45 a3 (M2) WINERED:Magellan ADC 19:00 b1 (M1) MEMS X 19:03 b2 (M2) MALLS CCD 19:06 b3 (M2) c 19:09 b4 (M1) GHz :00-10:00 C 09:00 a4 (M1) 09:15 a5 (M1) 09:30 a6 (M2) 1.85m 09:45 a7 (M1) :30-12:30 B 11:30 a8 (M1) NANTEN2 NECST 11:45 a9 (M1) NANTEN2 NASCO 12:00 a10 (M1) LiteBIRD 12:15 a11 (M2) DESHIMA: De:code :45-15:45 B 14:45 ( ) CTA :15-19:15 A 18:15 a12 MiwaYuya ( M1) Suzaku/HXD- WAM 18:30 a13 (M1) 18:45 a14 (M1) X 19:00 a15 (M1) Kanazawa SAT 3 X :15-11:15 C 10:15 a16 (M1) X SOI- CMOS 10:30 a17 (M1) X SOI 10:45 a18 (M1) XARM Xtend CCD 11:00 a19 (M1) X :30-14:30 C 13:30 a20 (M1) Lobster eye X 13:45 a21 (M1) Axion TES X 14:00 a22 (M2) X 14:15 a23 (M1) MeV :SMILE-2+ c1 (M1) TES X c2 (M1) SXS c3 Kobayashi Yukiho ( M1) CTA c4 (M2) c5 (M1) 16 48
18 c6 (M1) c7 (M1) c8 (M2) c9 (M1) 45m MKID c10 (M1) NANTEN2 c11 ( D2) c12 ( D2) COMING c13 (M1) CMB LiteBIRD 48 17
19 () :00-18:00 B J.Gleyzes et al. 2013, 2014 () :15-19:15 B LambdaCDM CMB sigma8 tension 18 48
20 () :30-14:30 B GW () :30-14:30 B 1. Takiwaki, T., Kotake, K., and Suwa, Y. 2016, Monthly Notices of the Royal Astronomical Society: Letters, 461, L
21 () :30-14:30 B (1) (2) (3) () :30-12:30 B Active Galactic Nucleus = AGN) (SuperMassive Black Hole = SMBH) AGN ( (1) (2) AGN (3) SMBH SMBH ALMA AGN 20 48
22 ( (Ta )) :00-18:00 B 1859 Carington Skylab mission X 1. Shibata and Takasao, 2016, Astrophysics and Space Science Library, 427, James A. McLaughlin, Valery M. Nakariakov, Maria Dominique, Petr Jelinek, and Shinsuke Takasao, 2018, Space Science Review 3. Shinsuke Takasao and Kazunari Shibata, 2016, ApJ, 823, 150 () :45-15:45 B X AI SDO 30 X 1. N. Nishizuka et al. ApJ (2018) in print 2. N. Nishizuka et al. ApJ (2017) 3. Bishop, C. M. Pattern Recognition and Machine Learning (1992) 48 21
23 () :15-11:15 B 45m FUGIN ( (A )) :15-11:15 B X 10 X 4 () (e.g., Fukui et al. 2012) X (Inoue et al. 2012; Sano et al. 2010, 2013, 2015, 2017) Cherenkov Telescope Array 1. Fukui et al. ApJ, 746, 82 (2012) 2. Inoue et al. ApJ, 774, 71 (2012) 3. Sano et al. ApJ, 779, 175 (2015) 22 48
24 () :15-19:15B / AU (/) :00-18:00 B ALMA 48 23
25 () :45-15:45 B 1. R. Davies, M. Kasper ARAA, 50, MEMS () :45-15:45 B CTA CTA CTA 1. Science with the CTA,
26 :15-19:15 AB ( D2) ( D2) ( D2) ( D3) ()
27 AED () ( 4.0km) Tel: () ( 2.5km) Tel:
28 () (7/22) 11:30 13:30 (7/25) 12:30 13: JR 48 27
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NGC1068 Dark Matter Halo baryon gas stars SMBH SMBH 1 SMBHs? (AGN) AGN Seyfertization Taniguchi 1987, ApJ, 317, L57 AGN The dead quasar problem (Rees 1990, Science, 247, 817) T AGN ~ 10 8 yrs AGN AGN
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Independent discoveries of a tidally disrupting dwarf galaxy around NGC 253! A Tidally Disrupting Dwarf Galaxy in the Halo of NGC 253 Toloba, E. et al. 2016, ApJL, 816, L5 (hereafter T16, accepted 2015.12.07)
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Numerical Modeling of the Interstellar Medium WADA Keiichi (National Astronomical Observatory of Japan) Abstract The interstellar medium in galaxies has a complicated multi-phase structure. However, in
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THE STAR FORMATION NEWSLETTER No.291-14 March 2017 2017/04/28 16-20 16. X-Shooter spectroscopy of young stellar objects in Lupus. Atmospheric parameters, membership and activity diagnostics 17. The evolution
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LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep. 初代星 初代銀河研究会, Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi
LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep., Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi Imanishi, Kazuhiro Shimasaku, Fumiaki Nakata, Yoshiki Matsuoka
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Fermi ( ) Outline Introduction Blazar Spectral Energy Distribution (SED) Predictions for the Fermi mission (Prospects for CTA) Summary The Blazar Sequence and the Cosmic Gamma-ray Background Radiation
Title ブラックホールと重力波天文学 Author(s) 長峯, 健太郎 Citation 高大連携物理教育セミナー報告書. 28 Issue Date Text Version publisher URL DO
Title ブラックホールと重力波天文学 Author(s) 長峯, 健太郎 Citation 高大連携物理教育セミナー報告書. 28 Issue Date 2017-03 Text Version publisher URL http://hdl.handle.net/11094/60516 DOI rights Osaka University Knowledge Archive : OUKA
3 6 6.1: ALMA 6.1 galaxy, galaxies the Galaxy, our Galaxy, Milky Way Galaxy G. Galilei W. Herschel cm J.C. Kapteyn H. Sharpley 30 E.P. Hubble 6.2 6.2.1 b l 6.2 b = 0 6.2: l = 0 6.2.2 6.1 6.3 ( 60-100µm)
Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
Type Ia Supernova Survey w/ WISH Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5. Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5. Type Ia Supernova + +?? (single degenerate)?
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Mathews Grant J. (University of Notre Dame) Boyd Richard N. (Lawrence Livermore National Laboratory) 2009/5/21
Mathews Grant J. (University of Notre Dame) Boyd Richard N. (Lawrence Livermore National Laboratory) 2009/5/21 Abstract strongly interacting massive particles (SIMPs, X) Big Bang (BBN) X heavy colored
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kawaguchi2.pdf
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