Hidetoshi SANO

J-GLOBAL         Last updated: Apr 24, 2019 at 14:19
 
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Name
Hidetoshi SANO
URL
http://www.a.phys.nagoya-u.ac.jp/~sano/
Affiliation
Nagoya University
Section
Institute for Advanced Research
Job title
Designated Assistant Professor
Research funding number
50739472
ORCID ID
0000-0003-2062-5692

Academic & Professional Experience

 
Apr 2015
 - 
Today
Designated Assistant Professor, Nagoya University
 
Apr 2014
 - 
Mar 2015
postdoctoral fellow, Graduate School of Science, Nagoya University
 
Apr 2012
 - 
Mar 2014
JSPS Research Fellow, Graduate School of Science, Nagoya University
 

Awards & Honors

 
Nov 2016
Springer Thesis Award, Springer
 
Mar 2011
Graduate School of Science Award, Nagoya University
 

Published Papers

 
The Astrophysical Journal      Oct 2018   [Refereed]
The Astrophysical Journal      Oct 2018   [Refereed]
Quentin Roper, Miroslav Filipovi, Glenn E Allen, Hidetoshi Sano, Laurence Park, Thomas G Pannuti, Manami Sasaki, Frank Haberl, Patrick J Kavanagh, Yumiko Yamane, Satoshi Yoshiike, Kosuke Fujii, Yasuo Fukui, Ivo R Seitenzahl
Monthly Notices of the Royal Astronomical Society      Sep 2018   [Refereed]
The Astrophysical Journal      Aug 2018   [Refereed]
Tulun Ergin, Aytap Sezer, Ryo Yamazaki, Hidetoshi Sano, Yasuo Fukui, Shuta Tanaka
   Dec 2017
A new extended gamma-ray source (PS J1934.5+1845) was detected with a
significance of Tex13Tex at a location of 1Tex.83 away from
the radio location of the Galactic supernova remnant 3C 400.2 using about 9
years of Fermi-LAT dat...
Tulun Ergin, Satoru Katsuda, Aytap Sezer, Ryo Yamazaki, Miroslav Filipovic, Hidetoshi Sano, Yasuo Fukui, Shuta Tanaka
   Dec 2017
A new extended gamma-ray source, which was named as Source A, in the
southwest of Galactic supernova remnant (SNR) G306.3Tex0.9 was detected with a
significance of Tex13Tex at the location of R.A. (J2000) =
13Tex 17Tex 52$^...
{Elia} D, {Molinari} S, {Schisano} E, {Pestalozzi} M, {Pezzuto} S, {Merello} M, {Noriega-Crespo} A, {Moore} T.~J.~T, {Russeil} D, {Mottram} J.~C, {Paladini} R, {Strafella} F, {Benedettini} M, {Bernard} J.~P, {Di Giorgio} A, {Eden} D.~J, {Fukui} Y, {Plume} R, {Bally} J, {Martin} P.~G, {Ragan} S.~E, {Jaffa} S.~E, {Motte} F, {Olmi} L, {Schneider} N, {Testi} L, {Wyrowski} F, {Zavagno} A, {Calzoletti} L, {Faustini} F, {Natoli} P, {Palmeirim} P, {Piacentini} F, {Piazzo} L, {Pilbratt} G.~L, {Polychroni} D, {Baldeschi} A, {Beltr{á}n} M.~T, {Billot} N, {Cambr{é}sy} L, {Cesaroni} R, {Garc{\'{\i}}a-Lario} P, {Hoare} M.~G, {Huang} M, {Joncas} G, {Liu} S.~J, {Maiolo} B.~M.~T, {Marsh} K.~A, {Maruccia} Y, {M{è}ge} P, {Peretto} N, {Rygl} K.~L.~J, {Schilke} P, {Thompson} M.~A, {Traficante} A, {Umana} G, {Veneziani} M, {Ward-Thompson} D, {Whitworth} A.~P, {Arab} H, {Bandieramonte} M, {Becciani} U, {Brescia} M, {Buemi} C, {Bufano} F, {Butora} R, {Cavuoti} S, {Costa} A, {Fiorellino} E, {Hajnal} A, {Hayakawa} T, {Kacsuk} P, {Leto} P, {Li Causi} G, {Marchili} N, {Martinavarro-Armengol} S, {Mercurio} A, {Molinaro} M, {Riccio} G, {Sano} H, {Sciacca} E, {Tachihara} K, {Torii} K, {Trigilio} C, {Vitello} F, {Yamamoto} H.
\mnras   471 100-143   Oct 2017   [Refereed]
{Fujita} S, {Torii} K, {Kuno} N, {Nishimura} A, {Umemoto} T, {Minamidani} T, {Kohno} M, {Yamagishi} M, {Tosaki} T, {Matsuo} M, {Tsuda} Y, {Tachihara} K, {Ohama} A, {Sano} H, {Hayashi} K, {Enokiya} R, {Yoshiike} S, {Tsutsumi} D, {Okawa} K, {Fukui} Y, {FUGIN members} o.
ArXiv e-prints      Nov 2017   [Refereed]
Shinji Fujita, Kazufumi Torii, Nario Kuno, Atsushi Nishimura, Tomofumi Umemoto, Tetsuhiro Minamidani, Mikito Kohno, Mitsuyoshi Yamagishi, Tomoka Tosaki, Mitsuhiro Matsuo, Yuya Tsuda, Kengo Tachihara, Akio Ohama, Hidetoshi Sano, Katsuhiro Hayashi, Rei Enokiya, Satoshi Yoshiike, Daichi Tsutsumi, Kazuki Okawa, Yasuo Fukui, other FUGIN members
   Nov 2017
W51A is one of the most active star-forming region in our Galaxy, which
contains giant molecular clouds with a total mass of 10^6 Msun. The molecular
clouds have multiple velocity components over ~20 km/s, and interactions
between these components...
{Enokiya} R, {Sano} H, {Hayashi} K, {Tachihara} K, {Torii} K, {Yamamoto} H, {Hattori} Y, {Hasegawa} Y, {Ohama} A, {Kimura} K, {Ogawa} H, {Fukui} Y.
ArXiv e-prints      Nov 2017   [Refereed]
Rei Enokiya, Hidetoshi Sano, Katsuhiro Hayashi, Kengo Tachihara, Kazufumi Torii, Hiroaki Yamamoto, Yusuke Hattori, Yutaka Hasegawa, Akio Ohama, Kimihiro Kimura, Hideo Ogawa, Yasuo Fukui
   Nov 2017
We made CO (Tex=1--0, 2--1, and 3--2) observations toward an H{\sc ii} region
RCW~32 in the Vela Molecular Ridge. The CO gas distribution associated with the
H{\sc ii} region was revealed for the first time at a high resolution of 22
arcsec. The r...
{Ohama} A, {Kohno} M, {Hasegawa} K, {Torii} K, {Hattori} Y, {Hayakawa} T, {Inoue} T, {Nishimura} A, {Sano} H, {Yamamoto} H, {Tachihara} K, {Fukui} Y.
ArXiv e-prints      Sep 2017   [Refereed]
{Cherenkov Telescope Array Consortium} T, {:}, {Acharya} B.~S, {Agudo} I, {Samarai} I.~A, {Alfaro} R, {Alfaro} J, {Alispach} C, {Alves Batista} R, {Amans} J.-P, et al.
ArXiv e-prints      Sep 2017   [Refereed]
{Maxted} N, {Burton} M, {Braiding} C, {Rowell} G, {Sano} H, {Voisin} F, {Capasso} M, {P{ü}hlhofer} G, {Fukui} Y.
ArXiv e-prints      Oct 2017   [Refereed]
Nigel Maxted, Michael Burton, Catherine Braiding, Gavin Rowell, Hidetoshi Sano, Fabien Voisin, Massimo Capasso, Gerd Pühlhofer, Yasuo Fukui
   Oct 2017
The shell-type supernova remnant HESS J1731Tex347 emits TeV gamma-rays, and
is a key object for the study of the cosmic ray acceleration potential of
supernova remnants. We use 0.5-1 arcminute Mopra CO/CS(1-0) data in conjunction
with HI data to c...
{Sano} H, {Reynoso} E.~M, {Mitsuishi} I, {Nakamura} K, {Furukawa} N, {Mruganka} K, {Fukuda} T, {Yoshiike} S, {Nishimura} A, {Ohama} A, {Torii} K, {Kuwahara} T, {Okuda} T, {Yamamoto} H, {Tachihara} K, {Fukui} Y.
Journal of High Energy Astrophysics   15 1-18   Sep 2017   [Refereed]
{Acero} F, {Acharya} B.~S, {Ac{\'{\i}}n Portella} V, {Adams} C, {Agudo} I, {Aharonian} F, {Samarai} I.~A, {Alberdi} A, {Alcubierre} M, {Alfaro} R, et al.
ArXiv e-prints      Sep 2017   [Refereed]
Akio Ohama, Mikito Kohno, Keisuke Hasegawa, Kazufumi Torii, Yusuke Hattori, Takahiro Hayakawa, Tsuyoshi Inoue, Atsushi Nishimura, Hidetoshi Sano, Hiroaki Yamamoto, Kengo Tachihara, Yasuo Fukui
   Sep 2017
Understanding the mechanism of O star formation is one of the most important
issues in current astrophysics. It is also an issue of keen interest how O
stars affect their surroundings and trigger secondary star formation. An
H\,\emissiontype{II} r...
{Sano} H, {Torii} K, {Saeki} S, {Okawa} K, {Tsuge} K, {Tsutsumi} D, {Khono} M, {Hattori} Y, {Fujita} S, {Yoshiike} S, {Enokiya} R, {Okamoto} R, {Hayashi} K, {Nishimura} A, {Ohama} A, {Hayakawa} T, {Yamamoto} H, {Tachihara} K, {Elisabet Cappa} C, {Fukui} Y.
ArXiv e-prints      Aug 2017   [Refereed]
{Fukui} Y, {Sano} H, {Sato} J, {Okamoto} R, {Fukuda} T, {Yoshiike} S, {Hayashi} K, {Torii} K, {Hayakawa} T, {Rowell} G, {Filipovic} M.~D, {Maxted} N, {McClure-Griffiths} N.~M, {Kawamura} A, {Yamamoto} H, {Okuda} T, {Mizuno} N, {Tachihara} K, {Onishi} T, {Mizuno} A, {Ogawa} H.
ArXiv e-prints      Aug 2017   [Refereed]
{Sano} H, {Yamane} Y, {Voisin} F, {Fujii} K, {Yoshiike} S, {Inaba} T, {Tsuge} K, {Babazaki} Y, {Mitsuishi} I, {Yang} R, {Aharonian} F, {Rowell} G, {Filipovi{ć}} M.~D, {Mizuno} N, {Tachihara} K, {Kawamura} A, {Onishi} T, {Fukui} Y.
\apj   843 61   Jul 2017   [Refereed]
Hidetoshi Sano, Kazufumi Torii, Shun Saeki, Kazuki Okawa, Kisetsu Tsuge, Daichi Tsutsumi, Mikito Khono, Yusuke Hattori, Shinji Fujita, Satoshi Yoshiike, Rei Enokiya, Ryuji Okamoto, Katsuhiro Hayashi, Atsushi Nishimura, Akio Ohama, Takahiro Hayakawa, Hiroaki Yamamoto, Kengo Tachihara, Cristina Elisabet Cappa, Yasuo Fukui
   Aug 2017
NGC 2359 is an HII region located in the outer Galaxy that contains the
isolated Wolf-Rayet (WR) star HD 56925. We present new CO observations of NGC
2359 with the Nobeyama 45 m radio telescope and the Atacama Submillimeter
Telescope Experiment us...
Tomofumi Umemoto, Tetsuhiro Minamidani, Nario Kuno, Shinji Fujita, Mitsuhiro Matsuo, Atsushi Nishimura, Kazufumi Torii, Tomoka Tosaki, Mikito Kohno, Mika Kuriki, Yuya Tsuda, Akihiko Hirota, Satoshi Ohashi, Mitsuyoshi Yamagishi, Toshihiro Handa, Hiroyuki Nakanishi, Toshihiro Omodaka, Nagito Koide, Naoko Matsumoto, Toshikazu Onishi, Kazuki Tokuda, Masumichi Seta, Yukinori Kobayashi, Kengo Tachihara, Hidetoshi Sano, Yusuke Hattori, Sachiko Onodera, Yumiko Oasa, Kazuhisa Kamegai, Masato Tsuboi, Yoshiaki Sofue, Aya E. Higuchi, James O. Chibueze, Norikazu Mizuno, Mareki Honma, Erik Muller, Tsuyoshi Inoue, Kana Morokuma-Matsui, Hiroko Shinnaga, Takeaki Ozawa, Ryo Takahashi, Satoshi Yoshiike, Jean Costes, Sho Kuwahara
   Jul 2017
The FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m
telescope (FUGIN) project is one of the legacy projects using the new
multi-beam FOREST receiver installed on the Nobeyama 45-m telescope. This
project aims to investigate th...
Mikito Kohno, Kazufumi Torii, Kengo Tachihara, Tomofumi Umemoto, Tetsuhiro Minamidani, Atsushi Nishimura, Shinji Fujita, Mitsuhiro Matsuo, Mitsuyoshi Yamagishi, Yuya Tsuda, Mika Kuriki, Nario Kuno, Akio Ohama, Yusuke Hattori, Hidetoshi Sano, Hiroaki Yamamoto, Yasuo Fukui
   Jun 2017
We observed molecular clouds in the W33 high-mass star-forming region
associated with compact and extended HII regions using the NANTEN2 telescope as
well as the Nobeyama 45-m telescope in the Tex1-0 transitions of TexCO,
TexCO, and C$^{1...
Atsushi Nishimura, Tetsuhiro Minamidani, Tomofumi Umemoto, Shinji Fujita, Mitsuhiro Matsuo, Yusuke Hattori, Mikito Kohno, Mitsuyoshi Yamagishi, Yuya Tsuda, Mika Kuriki, Nario Kuno, Kazufumi Torii, Daichi Tsutumi, Kazuki Okawa, Hidetoshi Sano, Kengo Tachihara, Akio Ohama, Yasuo Fukui
   Jun 2017
We present TexCO Tex1--0, TexCO Tex1--0 and CTexO Tex1--0
images of the M17 giant molecular clouds obtained as part of FUGIN (FOREST
Ultra-wide Galactic Plane Survey InNobeyama) project. The observations cover
the entire area of M17...
Atsushi Nishimura, Jean Costes, Tetsuta Inaba, Kengo Tachihara, Yusuke Hattori, Mikito Kohno, Akio Ohama, Kazufumi Torii, Hidetoshi Sano, Hiroaki Yamamoto, Yutaka Hasegawa, Kimihiro Kimura, Hideo Ogawa, Yasuo Fukui
   Jun 2017
M16, the Eagle Nebula, is an outstanding HII region where extensive high-mass
star formation is taking place in the Sagittarius Arm, and hosts the remarkable
"pillars" observed with HST. We made new CO observations of the region in the
12CO J=1--0...
Yasuo Fukui, Mikito Kohno, Keiko Yokoyama, Atsushi Nishimura, Kazufumi Torii, Yusuke Hatorri, Hidetoshi Sano, Akio Ohama, Hiroaki Yamamoto, Kengo Tachihara
   Jun 2017
High-mass star formation is an important step which controls galactic
evolution. GM 24 is a heavily obscured star cluster including a single O9 star
with more than Tex100 lower mass stars within a 0.3 pc radius toward
Tex (350.$^{\circ}...
Yasuo Fukui, Mikito Kohno, Keiko Yokoyama, Kazufumi Torii, Yusuke Hattori, Hidetoshi Sano, Atsushi Nishimura, Akio Ohama, Hiroaki Yamamoto, Kengo Tachihara
   Jun 2017
We carried out new CO (Tex1-0, 2-1 and 3-2) observations with NANTEN2 and
ASTE in the region of the twin Galactic mini-starbursts NGC6334 and NGC6357. We
detected two velocity molecular components of 12 km sTex velocity
separation, which is c...
{Ergin} T, {Sezer} A, {Sano} H, {Yamazaki} R, {Fukui} Y.
\apj   842 22   Jun 2017   [Refereed]
Katsuhiro Hayashi, Hidetoshi Sano, Rei Enokiya, Kazufumi Torii, Yusuke Hattori, Mikito Kohno, Shinji Fujita, Atsushi Nishimura, Akio Ohama, Hiroaki Yamamoto, Kengo Tachihara, Yutaka Hasegawa, Kimihiro Kimura, Hideo Ogawa, Yasuo Fukui
   Jun 2017
We report a possibility that the high-mass star located in the HII region RCW
34 was formed by a triggering induced by a collision of molecular clouds.
Molecular gas distributions of the TexCO and TexCO Tex2-1, and
TexCO Tex3-2 lines...
{Sano} H, {Enokiya} R, {Hayashi} K, {Yamagishi} M, {Saeki} S, {Okawa} K, {Tsuge} K, {Tsutsumi} D, {Khono} M, {Hattori} Y, {Yoshiike} S, {Fujita} S, {Nishimura} A, {Ohama} A, {Tachihara} K, {Torii} K, {Hasegawa} Y, {Kimura} K, {Ogawa} H, {Wong} G.~F, {Braiding} C, {Rowell} G, {Burton} M.~G, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
Hidetoshi Sano, Rei Enokiya, Katsuhiro Hayashi, Mitsuyoshi Yamagishi, Shun Saeki, Kazuki Okawa, Kisetsu Tsuge, Daichi Tsutsumi, Mikito Khono, Yusuke Hattori, Satoshi Yoshiike, Shinji Fujita, Atsushi Nishimura, Akio Ohama, Kengo Tachihara, Kazufumi Torii, Yutaka Hasegawa, Kimihiro Kimura, Hideo Ogawa, Graeme F. Wong, Catherine Braiding, Gavin Rowell, Michael G. Burton, Yasuo Fukui
   Jun 2017
A collision between two molecular clouds is one possible candidate for
high-mass star formation. The HII region RCW 36, located in the Vela molecular
ridge, contains a young star cluster with two O-type stars. We present new CO
observations of RCW...
S. Yoshiike, T. Fukuda, H. Sano, A. Ohama, N. Moribe, K. Torii, T. Hayakawa, T. Okuda, H. Yamamoto, H. Tajima, N. Mizuno, N. Mizuno, A. Nishimura, K. Kimura, H. Maezawa, H. Maezawa, T. Onishi, T. Onishi, A. Mizuno, H. Ogawa, A. Giuliani, B. C. Koo, Y. Fukui
Astrophysical Journal   768(2,Pt.1) 1-179   May 2013   [Refereed]
We present an analysis of the interstellar medium (ISM) toward the γ-ray supernova remnant (SNR) W44. We used NANTEN2 12CO(J = 2-1) and 12CO(J = 1-0) data and Arecibo H I data in order to identify the molecular and atomic gas in the SNR. We confir...
{Ohama} A, {Kono} M, {Tsutsumi} D, {Hattori} Y, {Torii} K, {Nishimura} A, {Sano} H, {Yamamoto} H, {Tachihara} K, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
Akio Ohama, Daichi Tsutsumi, Hidetoshi Sano, Kazufumi Torii, Atsushi Nishimura, Kazuhiro Shima, Habe Asao Hiroaki Yamamoto, Kengo Tachihara, Yutaka Hasagawa, Kimihiro Kimura, Hideo Ogawa, Yasuo Fukui
   Jun 2017
We analyzed the NANTEN2 13CO (J=2-1 and 1-0) datasets in NGC 2024. We found
that the cloud consists of two velocity components, whereas the cloud shows
mostly single-peaked CO profiles. The two components are physically connected
to the HII region...
{Maxted} N.~I, {Rowell} G.~P, {Dawson} B.~R, {Burton} M.~G, {Fukui} Y, {Walsh} A, {Kawamura} A, {Horachi} H, {Sano} H, {Yoshiike} S, {Fukuda} T.
\mnras   434 2188-2201   Sep 2013   [Refereed]
Akio Ohama, Mikito Kono, Daichi Tsutsumi, Yusuke Hattori, Kazufumi Torii, Atsushi Nishimura, Hidetoshi Sano, Hiroaki Yamamoto, Kengo Tachihara, Yasuo Fukui
   Jun 2017
Young HII regions are an important site to study O star formation based on
distributions of ionized and molecular gas. We revealed that two molecular
clouds at 48 km s-1 and 53 km s-1 are associated with a compact HII region RCW
166 by using the J...
Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson, Michael G. Burton, Brent P. Nicholas, Yasuo Fukui, Andrew J. Walsh, Akiko Kawamura, Hirotaka Horachi, Hidetoshi Sano
Monthly Notices of the Royal Astronomical Society   430(3) 2511-2512   May 2013   [Refereed]
{Fukui} Y, {Kohno} M, {Yokoyama} K, {Torii} K, {Hattori} Y, {Sano} H, {Nishimura} A, {Ohama} A, {Yamamoto} H, {Tachihara} K.
ArXiv e-prints      Jun 2017   [Refereed]
Daich Tsutsumi, Akio Ohama, Kazuki Okawa, mikito Kohno, Yusuke Hattori, Shinji Fujita, Atsushi Nishimura, Kazufumi Torii, Hidetoshi Sano, Hiroaki Yamamoto, Kengo Tachihara, Yutaka Hasegawa, Kimihiro Kimura, Hideo Ogawa, Yasuo Fukui
   Jun 2017
We carried out a molecular line study toward the high-mass star forming
regions with reflection nebulae, NGC2068 and NGC2071, in Orion with NANTEN2 in
the Textransition. The Tex distribution
shows that there ar...
{Hayashi} K, {Sano} H, {Enokiya} R, {Torii} K, {Hattori} Y, {Kohno} M, {Fujita} S, {Nishimura} A, {Ohama} A, {Yamamoto} H, {Tachihara} K, {Hasegawa} Y, {Kimura} K, {Ogawa} H, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson, Michael G. Burton, Yasuo Fukui, Andrew J. Walsh, Akiko Kawamura, Hidetoshi Sano, Jasmina Lazendic
AIP Conference Proceedings   1505 253-256   Dec 2012   [Refereed]
A summary of results from a 7 mm-wavelength survey towards the young X-ray and γ-ray-bright supernova remnant, RXJ1713.7-3946 (SNR G347.3-0.5) is presented. Using the Mopra telescope, the high critical density tracer CS(1-0) was targeted, compleme...
{Ohama} A, {Tsutsumi} D, {Sano} H, {Torii} K, {Nishimura} A, {Shima} K, {Asao Hiroaki Yamamoto} H, {Tachihara} K, {Hasagawa} Y, {Kimura} K, {Ogawa} H, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
{Maxted} N.~I, {Rowell} G.~P, {Dawson} B.~R, {Burton} M.~G, {Nicholas} B.~P, {Fukui} Y, {Walsh} A.~J, {Kawamura} A, {Horachi} H, {Sano} H.
\mnras   422 2230-2245   May 2012   [Refereed]
{Fukui} Y, {Sano} H, {Sato} J, {Torii} K, {Horachi} H, {Hayakawa} T, {McClure-Griffiths} N.~M, {Rowell} G, {Inoue} T, {Inutsuka} S, {Kawamura} A, {Yamamoto} H, {Okuda} T, {Mizuno} N, {Onishi} T, {Mizuno} A, {Ogawa} H.
\apj   746 82   Feb 2012   [Refereed]
Kazufumi Torii, Yasuo Fukui, Hidetoshi Sano, Junki Sato, Takeshi Okuda, Hiroaki Yamamoto, Akiko Kawamura, Norikazu Mizuno, Toshikazu Onishi, Hideo Ogawa
Proceedings of the International Astronomical Union   7(S284) 389-392   Sep 2011   [Refereed]
Galactic-scale studies of γ-rays and sub-mm radiation suggest that a significant amount of neutral interstellar medium is not detectable either in CO or HI (Grenier et al. 2005; Ade et al. 2011). This component is called "dark gas". Here we argue ...
{Tsutsumi} D, {Ohama} A, {Okawa} K, {Kohno} m, {Hattori} Y, {Fujita} S, {Nishimura} A, {Torii} K, {Sano} H, {Yamamoto} H, {Tachihara} K, {Hasegawa} Y, {Kimura} K, {Ogawa} H, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
{Fukui} Y, {Tsuge} K, {Sano} H, {Bekki} K, {Yozin} C, {Tachihara} K, {Inoue} T.
\pasj   69 L5   Jun 2017   [Refereed]
{Fukui} Y, {Kohno} M, {Yokoyama} K, {Nishimura} A, {Torii} K, {Hatorri} Y, {Sano} H, {Ohama} A, {Yamamoto} H, {Tachihara} K.
ArXiv e-prints      Jun 2017   [Refereed]
{Kohno} M, {Torii} K, {Tachihara} K, {Umemoto} T, {Minamidani} T, {Nishimura} A, {Fujita} S, {Matsuo} M, {Yamagishi} M, {Tsuda} Y, {Kuriki} M, {Kuno} N, {Ohama} A, {Hattori} Y, {Sano} H, {Yamamoto} H, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
{Nishimura} A, {Minamidani} T, {Umemoto} T, {Fujita} S, {Matsuo} M, {Hattori} Y, {Kohno} M, {Yamagishi} M, {Tsuda} Y, {Kuriki} M, {Kuno} N, {Torii} K, {Tsutumi} D, {Okawa} K, {Sano} H, {Tachihara} K, {Ohama} A, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
{Nishimura} A, {Costes} J, {Inaba} T, {Tachihara} K, {Hattori} Y, {Kohno} M, {Ohama} A, {Torii} K, {Sano} H, {Yamamoto} H, {Hasegawa} Y, {Kimura} K, {Ogawa} H, {Fukui} Y.
ArXiv e-prints      Jun 2017   [Refereed]
A. Giuliani, M. Tavani, M. Tavani, A. Bulgarelli, E. Striani, E. Striani, S. Sabatini, M. Cardillo, Y. Fukui, A. Kawamura, A. Ohama, N. Furukawa, K. Torii, H. Sano, F. A. Aharonian, F. A. Aharonian, F. Verrecchia, A. Argan, G. Barbiellini, P. A. Caraveo, P. W. Cattaneo, A. W. Chen, V. Cocco, E. Costa, F. D'ammando, F. D'ammando, E. Del Monte, G. De Paris, G. Di Cocco, I. Donnarumma, Y. Evangelista, M. Feroci, M. Fiorini, T. Froysland, T. Froysland, F. Fuschino, M. Galli, F. Gianotti, C. Labanti, Y. Lapshov, F. Lazzarotto, P. Lipari, F. Longo, M. Marisaldi, S. Mereghetti, A. Morselli, E. Moretti, L. Pacciani, A. Pellizzoni, F. Perotti, P. Picozza, P. Picozza, M. Pilia, M. Prest, G. Pucella, M. Rapisarda, A. Rappoldi, P. Soffitta, M. Trifoglio, A. Trois, E. Vallazza, S. Vercellone, V. Vittorini, V. Vittorini, A. Zambra, D. Zanello, C. Pittori, P. Santolamazza, P. Giommi, S. Colafrancesco, L. Salotti
Astronomy and Astrophysics   516 L11   Jul 2010   [Refereed]
Aims. Supernova remnants (SNRs) are believed to be the main sources of Galactic cosmic rays. Molecular clouds associated with SNRs can produce gamma-ray emission by means of the interaction of accelerated particles with the concentrated gas. The m...
{Acero} F, {Aloisio} R, {Amans} J, {Amato} E, {Antonelli} L.~A, {Aramo} C, {Armstrong} T, {Arqueros} F, {Asano} K, {Ashley} M, et al.
\apj   840 74   May 2017   [Refereed]
{Nakamichi} K, {Ishihara} D, {Kaneda} H, {Oyabu} S, {Kondo} T, {Amatsutsu} T, {Sano} H, {Onaka} T.
Publication of Korean Astronomical Society   32 29-31   Mar 2017   [Refereed]
{Amatsutsu} T, {Ishihara} D, {Kondo} T, {Kaneda} H, {Oyabu} S, {Yamagishi} M, {Nakamichi} K, {Sano} H, {Onaka} T.
Publication of Korean Astronomical Society   32 25-27   Mar 2017   [Refereed]
{Kondo} T, {Ishihara} D, {Kaneda} H, {Oyabu} S, {Amatsutsu} T, {Nakamichi} K, {Sano} H, {Ootsubo} T, {Onaka} T.
Publication of Korean Astronomical Society   32 59-61   Mar 2017   [Refereed]
{Hattori} Y, {Kaneda} H, {Ishihara} D, {Yamagishi} M, {Kondo} T, {Sano} H.
Publication of Korean Astronomical Society   32 123-125   Mar 2017   [Refereed]
{Sano} H, {Amatsutsu} T, {Kondo} T, {Nakamichi} K, {Yamagishi} M, {Ishihara} D, {Oyabu} S, {Kaneda} H, {Tachihara} K, {Fukui} Y.
Publication of Korean Astronomical Society   32 21-23   Mar 2017   [Refereed]
Yasuo Fukui, Kisetsu Tsuge, Hidetoshi Sano, Kenji Bekki, Cameron Yozin, Kengo Tachihara, Tsuyoshi Inoue
   Mar 2017
Understanding of massive cluster formation is one of the important issues of
astronomy. By analyzing the HI data, we have identified that the two HI
velocity components (L- and D-components) are colliding toward the HI Ridge, in
the southeastern e...
{Katsuda} S, {Acero} F, {Tominaga} N, {Ballet} J, {Fukui} Y, {Hiraga} J.~S, {Koyama} K, {Lee} S.-H, {Mori} K, {Nagataki} S, {Ohira} Y, {Petre} R, {Sano} H, {Takeuchi} Y, {Tamagawa} T, {Tsuji} N, {Tsunemi} H, {Uchiyama} Y.
Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their Aftermaths   331 206-212   Feb 2017   [Refereed]
{Sano} H, {Fujii} K, {Yamane} Y, {Inaba} T, {Yoshiike} S, {Fukuda} T, {Voisin} F, {Rowell} G, {Fukui} Y.
6th International Symposium on High Energy Gamma-Ray Astronomy   1792 040038   Jan 2017   [Refereed]
{Yoshiike} S, {Fukuda} T, {Sano} H, {Fukui} Y.
6th International Symposium on High Energy Gamma-Ray Astronomy   1792 040039   Jan 2017   [Refereed]
{Voisin} F, {Rowell} G, {Burton} M.~G, {Fukui} Y, {Sano} H, {Aharonian} F.
6th International Symposium on High Energy Gamma-Ray Astronomy   1792 040011   Jan 2017   [Refereed]
{Fukui} Y, {Torii} K, {Hattori} Y, {Nishimura} A, {Ohama} A, {Shimajiri} Y, {Shima} K, {Habe} A, {Sano} H, {Yamamoto} H, {Tachihara} K, {Onishi} T.
ArXiv e-prints      Jan 2017   [Refereed]
{Sano} H.
Shock-Cloud Interaction in RX J1713.7-3946, Springer Thesis Series.~ISBN 978-4-431-55636-7.~Springer Japan, 2017.~134 p.      Nov 2016   [Refereed]
Yasuo Fukui, Kazufumi Torii, Yusuke Hattori, Atsushi Nishimura, Akio Ohama, Yoshito Shimajiri, Kazuhiro Shima, Asao Habe, Hidetoshi Sano, Hiroaki Yamamoto, Kengo Tachihara, Toshikazu Onishi
   Jan 2017
The Orion Nebula Cluster toward the HII region M42 is the most outstanding
young cluster at the smallest distance 410pc among the rich high-mass stellar
clusters. By newly analyzing the archival molecular data of the 12CO(J=1-0)
emission at 21" re...
{CTA Consortium} T, {:}, {Abchiche} A, {Abeysekara} U, {Abril} {Ó}, {Acero} F, {Acharya} B.~S, {Adams} C, {Agnetta} G, {Aharonian} F, et al.
ArXiv e-prints      Oct 2016   [Refereed]
{Sano} H, {Fukui} Y.
XMM-Newton: The Next Decade   62   Jun 2016   [Refereed]
{Fukui} Y, {Torii} K, {Ohama} A, {Hasegawa} K, {Hattori} Y, {Sano} H, {Ohashi} S, {Fujii} K, {Kuwahara} S, {Mizuno} N, {Dawson} J.~R, {Yamamoto} H, {Tachihara} K, {Okuda} T, {Onishi} T, {Mizuno} A.
\apj   820 26   Mar 2016   [Refereed]
{Babazaki} Y, {Mitsuishi} I, {Sano} H, {Yoshiike} S, {Fukuda} T, {Maruyama} S, {Fujii} K, {Fukui} Y, {Tawara} Y, {Matsumoto} H.
IAU Focus Meeting   29 737-737   2016   [Refereed]
{Sano} H, {Fukui} Y, {Yoshiike} S, {Fukuda} T, {Tachihara} K, {Inutsuka} S, {Kawamura} A, {Fujii} K, {Mizuno} N, {Inoue} T, {Onishi} T, {Acero} F, {Vink} J.
Revolution in Astronomy with ALMA: The Third Year   499 257   Dec 2015   [Refereed]
{Katsuda} S, {Acero} F, {Tominaga} N, {Fukui} Y, {Hiraga} J.~S, {Koyama} K, {Lee} S.-H, {Mori} K, {Nagataki} S, {Ohira} Y, {Petre} R, {Sano} H, {Takeuchi} Y, {Tamagawa} T, {Tsuji} N, {Tsunemi} H, {Uchiyama} Y.
\apj   814 29   Nov 2015   [Refereed]
{Hattori} Y, {Kaneda} H, {Ishihara} D, {Yamagishi} M, {Kondo} T, {Sano} H.
\planss   116 57-63   Oct 2015   [Refereed]
Hidetoshi Sano, Tomoya Amatsutsu, Toru Kondo, Keichiro Nakamichi, Mitsuyoshi Yamagishi, Daisuke Ishihara, Shinki Oyabu, Hidehiro Kaneda, Kengo Tachihara, Yasuo Fukui
   Feb 2016
We present a comparative study of CO and polycyclic aromatic hydrocarbon
(PAH) emission toward a region including the massive star-forming regions of
NGC 6334 and NGC 6357. We use the NANTEN TexCO(Tex = 1--0) data and the
Tex 9 Texm All-...
{Nakamori} T, {Katagiri} H, {Sano} H, {Yamazaki} R, {Ohira} Y, {Bamba} A, {Fukui} Y, {Mori} K, {Lee} S.-H, {Fujita} Y, {Tajima} H, {Inoue} T, {Gunji} S, {Hanabata} Y, {Hayashida} M, {Kubo} H, {Kushida} J, {Inoue} S, {Ioka} K, {Kohri} K, {Murase} K, {Nagataki} S, {Naito} T, {Okumura} A, {Saito} T, {Sawada} M, {Tanaka} T, {Terada} Y, {Uchiyama} Y, {Yanagita} S, {Yoshida} T, {Yoshikoshi} T, {CTA Consortium} f.~t.
ArXiv e-prints      Aug 2015   [Refereed]
{CTA Consortium} T, {:}, {Abchiche} A, {Abeysekara} U, {Abril} {Ó}, {Acero} F, {Acharya} B.~S, {Actis} M, {Agnetta} G, {Aguilar} J.~A, et al.
ArXiv e-prints      Aug 2015   [Refereed]
{Nakamori} T, {Katagiri} H, {Sano} H, {Yamazaki} R, {Ohira} Y, {Bamba} A, {Fukui} Y, {Mori} K, {Lee} S.-H, {Fujita} Y, {Tajima} H, {Inoue} T, {Gunji} S, {Hanabata} Y, {Hayashida} M, {Kubo} H, {Kushida} J, {Inoue} S, {Ioka} K, {Kohri} K, {Murase} K, {Nagataki} S, {Naito} T, {Okumura} A, {Saito} T, {Sawada} M, {Tanaka} T, {Terada} Y, {Uchiyama} Y, {Yanagita} S, {Yoshida} T, {Yoshikoshi} T, {Consortium} C.
34th International Cosmic Ray Conference (ICRC2015)   34 774   Jul 2015   [Refereed]
Satoru Katsuda, Fabio Acero, Nozomu Tominaga, Yasuo Fukui, Junko S. Hiraga, Katsuji Koyama, Shiu-Hang Lee, Koji Mori, Shigehiro Nagataki, Yutaka Ohira, Robert Petre, Hidetoshi Sano, Yoko Takeuchi, Toru Tamagawa, Naomi Tsuji, Hiroshi Tsunemi, Yasunobu Uchiyama
   Oct 2015
We report the first detection of thermal X-ray line emission from the
supernova remnant (SNR) RX J1713.7-3946, the prototype of the small class of
synchrotron dominated SNRs. A softness-ratio map generated using XMM-Newton
data shows that faint in...
{Gozzini} S.~R, {Hanabata} Y, {Colin} P, {Zanin} R, {Pedaletti} G, {de O{ñ}a Wilhelmi} E, {Torres} D.~F, {Krause} J, {Fukui} Y, {Yoshiike} S, {Sano} H, {Giordano} F, {Di Venere} L.
34th International Cosmic Ray Conference (ICRC2015)   34 870   Jul 2015   [Refereed]
{Torii} K, {Hasegawa} K, {Hattori} Y, {Sano} H, {Ohama} A, {Yamamoto} H, {Tachihara} K, {Soga} S, {Shimizu} S, {Okuda} T, {Mizuno} N, {Onishi} T, {Mizuno} A, {Fukui} Y.
\apj   806 7   Jun 2015   [Refereed]
T. Nakamori, H. Katagiri, H. Sano, R. Yamazaki, Y. Ohira, A. Bamba, Y. Fukui, K. Mori, S. -H. Lee, Y. Fujita, H. Tajima, T. Inoue, S. Gunji, Y. Hanabata, M. Hayashida, H. Kubo, J. Kushida, S. Inoue, K. Ioka, K. Kohri, K. Murase, S. Nagataki, T. Naito, A. Okumura, T. Saito, M. Sawada, T. Tanaka, Y. Terada, Y. Uchiyama, S. Yanagita, T. Yoshida, T. Yoshikoshi, for the CTA Consortium
   Aug 2015
We perform simulations of Cherenkov Telescope Array (CTA) observations of a
young supernova remnant RX J1713.7-3946. This target is not only one of the
brightest sources ever discovered in very high-energy gamma rays but also well
observed in othe...
{Sano} H, {Fukuda} T, {Yoshiike} S, {Sato} J, {Horachi} H, {Kuwahara} T, {Torii} K, {Hayakawa} T, {Tanaka} T, {Matsumoto} H, {Inoue} T, {Yamazaki} R, {Inutsuka} S, {Kawamura} A, {Yamamoto} H, {Okuda} T, {Tachihara} K, {Mizuno} N, {Onishi} T, {Mizuno} A, {Acero} F, {Fukui} Y.
\apj   799 175   Feb 2015   [Refereed]
{Fukui} Y, {Torii} K, {Onishi} T, {Yamamoto} H, {Okamoto} R, {Hayakawa} T, {Tachihara} K, {Sano} H.
\apj   798 6   Jan 2015   [Refereed]
{Abramowski} A, {Aharonian} F, {Ait Benkhali} F, {Akhperjanian} A.~G, {Ang{ü}ner} E.~O, {Backes} M, {Balenderan} S, {Balzer} A, {Barnacka} A, {Becherini} Y, et al.
\apjl   794 L1   Oct 2014   [Refereed]
Y. Fukui, K. Torii, A. Ohama, K. Hasegawa, Y. Hattori, H. Sano, S. Ohashi, K. Fujii, S. Kuwahara, N. Mizuno, J. R. Dawson, H. Yamamoto, K. Tachihara, T. Okuda, T. Onishi, A. Mizuno
   Apr 2015
We present distributions of two molecular clouds having velocities of 2 km
sTex and 14 km sTex toward RCW 38, the youngest super star cluster in
the Milky Way, in the TexCO (Tex1--0 and 3--2) and TexCO (Tex1--0)
transitions. The ...
H. Sano, Y. Fukui, S. Yoshiike, T. Fukuda, K. Tachihara, S. Inutsuka, A. Kawamura, K. Fujii, N. Mizuno, T. Inoue, T. Onishi, F. Acero, J. Vink
   Mar 2015
We report preliminary results of large-scale distribution toward the
Magellanic supernova remnant N132D using Mopra and Chandra archival datasets.
We identified a cavity-like CO structure along the X-ray shell toward the
southern half of it. The t...
{Fukuda} T, {Yoshiike} S, {Sano} H, {Torii} K, {Yamamoto} H, {Acero} F, {Fukui} Y.
\apj   788 94   Jun 2014   [Refereed]
K. Torii, K. Hasegawa, Y. Hattori, H. Sano, A. Ohama, H. Yamamoto, K. Tachihara, S. Soga, S. Shimizu, T. Okuda, N. Mizuno, T. Onishi, A. Mizuno, Y. Fukui
Astrophysical Journal   806    Feb 2015
RCW120 is a Galactic HII region having a beautiful ring shape bright in
infrared. Our new CO J=1-0 and J=3-2 observations performed with the NANTEN2,
Mopra, and ASTE telescopes have revealed that two molecular clouds with a
velocity separation of ...
{Cardillo} M, {Tavani} M, {Giuliani} A, {Yoshiike} S, {Sano} H, {Fukuda} T, {Fukui} Y, {Castelletti} G, {Dubner} G.
åp   565 A74   May 2014   [Refereed]
H. E. S. S. Collaboration, :, A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. O. Angüner, M. Backes, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, D. Berge, S. Bernhard, K. Bernlöhr, E. Birsin, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Bregeon, F. Brun, P. Brun, M. Bryan, T. Bulik, S. Carrigan, S. Casanova, P. M. Chadwick, N. Chakraborty, R. Chalme-Calvet, R. C. G. Chaves, M. Chrétien, S. Colafrancesco, G. Cologna, J. Conrad, C. Couturier, Y. Cui, M. Dalton, I. D. Davids, B. Degrange, C. Deil, P. deWilt, A. Djannati-Ataï, W. Domainko, A. Donath, L. O'C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, P. Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernandez, A. Fiasson, G. Fontaine, A. Förster, M. Füßling, S. Gabici, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, D. Gottschall, M. -H. Grondin, M. Grudzińska, D. Hadasch, S. Häffner, J. Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, A. Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Ivascenko, A. Jacholkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung-Richardt, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lau, J. Lefaucheur, V. Lefranc, A. Lemière, M. Lemoine-Goumard, J. -P. Lenain, T. Lohse, A. Lopatin, C. -C. Lu, V. Marandon, A. Marcowith, R. Marx, G. Maurin, N. Maxted, M. Mayer, T. J. L. McComb, J. Méhault, P. J. Meintjes, U. Menzler, M. Meyer, A. M. W. Mitchell, R. Moderski, M. Mohamed, K. Morå, E. Moulin, T. Murach, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, H. Odaka, S. Ohm, B. Opitz, M. Ostrowski, I. Oya, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, P. -O. Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, I. Reichardt, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, F. Rieger, C. Romoli, S. Rosier-Lees, G. Rowell, B. Rudak, C. B. Rulten, V. Sahakian, D. Salek, D. A. Sanchez, A. Santangelo, R. Schlickeiser, F. Schüssler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, F. Spanier, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, J. -P. Tavernet, T. Tavernier, A. M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, B. van Soelen, G. Vasileiadis, J. Veh, C. Venter, A. Viana, P. Vincent, J. Vink, H. J. Völk, F. Volpe, M. Vorster, T. Vuillaume, S. J. Wagner, P. Wagner, R. M. Wagner, M. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, R. Yang, V. Zabalza, D. Zaborov, M. Zacharias, A. A. Zdziarski, A. Zech, H. -S. Zechlin, Y. Fukui, H. Sano, T. Fukuda, S. Yoshiike
The Astrophysical Journal Letters, 794:L1 (6pp), 2014      Aug 2014
This letter reports the discovery of a remarkably hard spectrum source, HESS
J1641-463, by the High Energy Stereoscopic System (H.E.S.S.) in the very-high
energy (VHE) domain. HESS J1641-463 remained unnoticed by the usual analysis
techniques due ...
{Furukawa} N, {Ohama} A, {Fukuda} T, {Torii} K, {Hayakawa} T, {Sano} H, {Okuda} T, {Yamamoto} H, {Moribe} N, {Mizuno} A, {Maezawa} H, {Onishi} T, {Kawamura} A, {Mizuno} N, {Dawson} J.~R, {Dame} T.~M, {Yonekura} Y, {Aharonian} F, {de O{ñ}a Wilhelmi} E, {Rowell} G.~P, {Matsumoto} R, {Asahina} Y, {Fukui} Y.
\apj   781 70   Feb 2014   [Refereed]
T. Fukuda, S. Yoshiike, H. Sano, K. Torii, H. Yamamoto, F. Acero, Y. Fukui
Astrophysical Journal   788    May 2014
HESS J1731-347 (G353.6-0.7) is one of the TeV gamma-ray SNRs which shows the
shell-like morphology. We have made a new analysis of the interstellar protons
toward the SNR by using both the 12CO(J=1-0) and HI datasets. The results
indicate that the...
{Enokiya} R, {Torii} K, {Schultheis} M, {Asahina} Y, {Matsumoto} R, {Furuhashi} E, {Nakamura} K, {Dobashi} K, {Yoshiike} S, {Sato} J, {Furukawa} N, {Moribe} N, {Ohama} A, {Sano} H, {Okamoto} R, {Mori} Y, {Hanaoka} N, {Nishimura} A, {Hayakawa} T, {Okuda} T, {Yamamoto} H, {Kawamura} A, {Mizuno} N, {Onishi} T, {Morris} M.~R, {Fukui} Y.
\apj   780 72   Jan 2014   [Refereed]
M. Cardillo, M. Tavani, A. Giuliani, S. Yoshiike, H. Sano, T. Fukuda, Y. Fukui, G. Castelletti, G. Dubner
Astronomy and Astrophysics   565    Mar 2014
The middle-aged supernova remnant (SNR) W44 has recently attracted attention
because of its relevance regarding the origin of Galactic cosmic-rays. The
gamma-ray missions AGILE and Fermi have established, for the first time for a
SNR, the spectral...