6.6k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Academia SinicaTW1.4k papers
- National Astronomical Observatory of JapanJP910 papers
- The University of TokyoJP744 papers
- Center for Astrophysics Harvard & SmithsonianUS671 papers
- Centre National de la Recherche ScientifiqueFR668 papers
- European Southern ObservatoryCL490 papers
- California Institute of TechnologyUS470 papers
- The Graduate University for Advanced Studies, SOKENDAIJP427 papers
- Kavli Institute for the Physics and Mathematics of the UniverseJP425 papers
- Jet Propulsion LaboratoryUS360 papers
- Max Planck Institute for AstronomyDE342 papers
- Leiden UniversityNL340 papers
139 papers · 1 filter
Star Formation and AGN activity in Galaxies classified using the 1.6 μm Bump and PAH features at
Hitoshi Hanami, Tsuyoshi Ishigaki, Naofumi Fujishiro +17
We have studied the star-formation and AGN activity of massive galaxies in the redshift range , which are detected in a deep survey field using the AKARI InfraRed (IR) ast…
Primordial Magnetic Field Effects on the CMB and Large Scale Structure
Dai G. Yamazaki, Kiyotomo Ichiki, Toshitaka Kajino +1
Magnetic fields are everywhere in nature and they play an important role in every astronomical environment which involves the formation of plasma and currents. It is natural theref…
Discovery of the Youngest Molecular Outflow associated with an Intermediate-mass protostellar Core, MMS-6/OMC-3
Satoko Takahashi, Paul Ho
We present sub-arcsecond resolution HCN (4-3) and CO (3-2) observations made with the Submillimeter Array (SMA), toward an extremely young intermediate-mass protostellar core, MMS…
The TW Hya Disk at 870 microns: Comparison of CO and Dust Radial Structures
Sean M. Andrews, David J. Wilner, A. M. Hughes +9
We present high resolution (0.3" = 16 AU), high signal-to-noise ratio Submillimeter Array observations of the 870 microns (345 GHz) continuum and CO J=3--2 line emission from the p…
The Extremely High-Velocity Outflow from the Luminous Young Stellar Object G5.89-0.39
Yu-Nung Su, Sheng-Yuan Liu, Huei-Ru Chen +1
We have imaged the extremely high-velocity outflowing gas in CO (2-1) and (3-2) associated with the shell-like ultracompact HII region G5.89-0.39 at a resolution of ~3" (correspond…
Baryon Content of Massive Galaxy Clusters at z=0-0.6
Yen-Ting Lin, S. Adam Stanford, Peter R. M. Eisenhardt +3
We study the relationship between two major baryonic components in galaxy clusters, namely the stars in galaxies, and the ionized gas in the intracluster medium (ICM), using 94 clu…
Exploring the central sub-pc region of the γ-ray bright radio galaxy 3C 84 with the VLBA at 43 GHz in the period of 2002-2008
Kenta Suzuki, Hiroshi Nagai, Motoki Kino +13
Following the discovery of a new radio component right before the GeV γ-ray detection since 2008 August by Fermi Gamma-ray Space Telescope, we present a detailed study of the kinem…
Surviving the hole I: Spatially resolved chemistry around Sgr A*
S. Martín, J. Martín-Pintado, M. Montero-Castaño +2
The interstellar region within the few central parsecs around the super-massive black hole, Sgr A* at the very Galactic center is composed by a number of overlapping molecular stru…
Magnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations
Miljenko Čemeljić, Hsien Shang, Tzu-Yang Chiang
The ejection of matter in the close vicinity of a young stellar object is investigated, treating the accretion disk as a gravitationally bound reservoir of matter. By solving the r…
Bolocam Observations of Two Unconfirmed Galaxy Cluster Candidates from the Planck Early SZ Sample
Jack Sayers, Nicole G. Czakon, Carrie Bridge +5
We present Bolocam observations of two galaxy cluster candidates reported as unconfirmed in the Planck early Sunyaev-Zel'dovich (eSZ) sample, PLCKESZ G115.71+17.52 and PLCKESZ G189…
Identification of Spitzer-IRS staring mode targets in the Magellanic Clouds
Paul M. E. Ruffle, Paul M. Woods, F. Kemper
The SAGE-LMC, SAGE-SMC and HERITAGE surveys have mapped the Magellanic Clouds in the infrared using the Spitzer and Herschel Space Telescopes. Over 8.5 million point sources were d…
Interferometric CO(3-2) Observations toward the Central Region of NGC 1068
Mengchun Tsai, Chorng-Yuan Hwang, Satoki Matsushita +2
We present CO(3-2) interferometric observations of the central region of the Seyfert 2 galaxy NGC 1068 using the Submillimeter Array, together with CO(1-0) data taken with the Owen…
Late-time Light Curves of Type II Supernovae: Physical Properties of SNe and Their Environment
Masaaki Otsuka, Margaret Meixner, Nino Panagia +9
We present BVRIJHK band photometry of 6 core-collapse supernovae, SNe 1999bw, 2002hh, 2003gd, 2004et, 2005cs, and 2006bc measured at late epochs (>2 yrs) based on Hubble Space Tele…
NGC3801 caught in the act: A post-merger starforming early-type galaxy with AGN-jet feedback
Ananda Hota, Soo-Chang Rey, Yongbeom Kang +3
In the current models of galaxy formation and evolution, AGN feedback is crucial to reproduce galaxy luminosity function, colour-magnitude relation and M-sigma relation. However, i…
X-ray and Gamma-ray Emissions from Different Evolutionary Stage of Rotation Powered Millisecond Pulsars
J. Takata, K. S. Cheng, R. E. Taam
The -LAT has revealed that rotation powered millisecond pulsars (MSPs) are a major contributor to the Galactic -ray source population. Such pulsars may also be important…
Probing Helical Magnetic Fields in AGN by Rotation Measure Gradients Studies
J. C. Algaba
One of the tools that can provide evidence about the existence of helical magnetic fields in AGN is the observation of rotation measure gradients across the jet. Such observations…
Clustering properties of BzK-selected galaxies in GOODS-N: environmental quenching and triggering of star formation at z ~ 2
Lihwai Lin, Mark Dickinson, Hung-Yu Jian +19
Using a sample of BzK-selected galaxies at z~2 identified from the CFHT/WIRCAM near-infrared survey of GOODS-North, we discuss the relation between star formation rate (SFR), speci…
How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?
Kyoung-Soo Lee, Henry C. Ferguson, Tommy Wiklind +8
We investigate how star-forming galaxies typically assemble their masses at high redshift. Using the deep multi-wavelength coverage of the GOODS dataset, we measure stellar mass of…
Damping of tensor modes in inflation
Kin-Wang Ng
We discuss the damping of tensor modes due to anisotropic stress in inflation. The effect is negligible in standard inflation and may be significantly large in inflation models tha…
Panchromatic observations of the textbook GRB 110205A: constraining physical mechanisms of prompt emission and afterglow
W. Zheng, R. F. Shen, T. Sakamoto +56
We present a comprehensive analysis of a bright, long duration (T90 ~ 257 s) GRB 110205A at redshift z= 2.22. The optical prompt emission was detected by Swift/UVOT, ROTSE-IIIb and…
Magnetic Interactions in Pre-Main-Sequence Binaries
Fred C. Adams, Michael J. Cai, Daniele Galli +2
Young stars typically have strong magnetic fields, so that the magnetospheres of newly formed close binaries can interact, dissipate energy, and produce synchrotron radiation. The…
Quantum noise in the mirror-field system: A field theoretic approach
Jen-Tsung Hsiang, Tai-Hung Wu, Da-Shin Lee +2
We employ the field theoretic approach to study the quantum noise problem in the mirror-field system, where a perfectly reflecting mirror is illuminated by a single-mode coherent s…
Dust properties in afterglow of GRB 071025 at z~5
Minsung Jang, Myungshin Im, Induk Lee +5
At high redshift, the universe was so young that core-collapse supernovae (SNe) are suspected to be the dominant source of dust production. However, some observations indicate that…
Unveiling the physical properties and kinematics of molecular gas in the Antennae Galaxies (NGC 4038/9) through high resolution CO (J = 3-2) observations
Junko Ueda, Daisuke Iono, Glen Petitpas +12
We present a ~ 1" (100 pc) resolution 12CO (3-2) map of the nearby intermediate stage interacting galaxy pair NGC 4038/9 (the Antennae galaxies) obtained with the Submillimeter Arr…