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
191 papers · 1 filter
Fe-vacancy order and superconductivity in PbO-type tetragonal β-Fe1-xSe
Ta-Kun Chen, Chung-Chieh Chang, Hsian-Hong Chang +12
Several superconducting transition temperatures in the range of 30-40 K were reported in the recently discovered intercalated FeSe sytem (A1-xFe2-ySe2, A = K, Rb, Cs, Tl). Although…
Observed relationship between CO2-1 and dust emission during post-AGB phase
J. H. He, R. Szczerba, T. I. Hasegawa +1
A CO\,2-1 line survey is performed toward a sample of 58 high Galactic latitude post-AGB (pAGB) stars. To complement the observations, a compilation of literature CO\,2-1 line data…
The Atlas3D project -- XXVII. Cold Gas and the Colours and Ages of Early-type Galaxies
L. M. Young, N. Scott, P. Serra +22
We present a study of the cold gas contents of the Atlas3D early-type galaxies, in the context of their optical colours, near-UV colours, and Hβ absorption line strengths. Early-ty…
The Pan-STARRS1 Medium-Deep Survey: The role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to
Lihwai Lin, Hung-Yu Jian, Sebastien Foucaud +26
Using a large sample of field and group galaxies drawn from the Pan-STARRS1 Medium-Deep Survey, we present the specific star formation rate (SSFR) - stellar mass (M*) relation, as…
A Measurement of the Kinetic Sunyaev-Zel'dovich Signal Toward MACS J0717.5+3745
Jack Sayers, Tony Mroczkowski, Michael Zemcov +18
We report our analysis of MACS J0717.5+3745 using 140 and 268 GHz Bolocam data collected at the Caltech Submillimeter Observatory. We detect extended Sunyaev-Zel'dovich (SZ) effect…
Method of Successive Projections for Nonnegative Inverse Singular Value problems with Prescribed Structure
Sheng-Jhih Wu, Matthew M. Lin
The study of solving inverse singular value problems for nonnegative matrices has been around for decades. It is clear that an inverse singular problem is trivial if the desirable…
On the origin of the molecular outflows in IRAS 16293-2422
Josep M. Girart, Robert Estalella, Aina Palau +2
We present CO 3-2, SiO 8-7, C34S 7-6, and 878 mum dust continuum subarcsecond angular resolution observations with the SMA toward IRAS 16293-2422 (I16293). The C34S emission traces…
A survey of infrared supernova remnants in the Large Magellanic Cloud
Ji Yeon Seok, Bon-Chul Koo, Takashi Onaka
We present a comprehensive infrared study of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) using near- to mid-infrared images taken by Infrared Array Camera (IRAC;…
Planck 2013 results. XI. All-sky model of thermal dust emission
Planck Collaboration, A. Abergel, P. A. R. Ade +244
This paper presents an all-sky model of dust emission from the Planck 857, 545 and 353 GHz, and IRAS 100 micron data. Using a modified black-body fit to the data we present all-sky…
Three Gravitationally Lensed Supernovae Behind CLASH Galaxy Clusters
Brandon Patel, Curtis McCully, Saurabh W. Jha +42
We report observations of three gravitationally lensed supernovae (SNe) in the Cluster Lensing And Supernova survey with Hubble (CLASH) Multi-Cycle Treasury program. These objects,…
Detection of a Magnetized Disk around a Very Young Protostar
Ramprasad Rao, Josep M. Girart, Shih-Ping Lai +1
We present subarcsecond resolution polarimetric observations of the 878 mum thermal dust continuum emission obtained with the Submillimeter Array (SMA) towards the IRAS 16293-2422…
Discovery of Sub- to Superluminal Motions in the M87 Jet: An Implication of the Acceleration from Sub-relativistic to Relativistic Speeds
Keiichi Asada, Masanori Nakamura, Akihiro Doi +2
The velocity field of the M87 jet from milli-arcsecond (mas) to arcsecond scales is extensively investigated together with new radio images taken by EVN observations. We detected p…
Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis
Hauyu Baobab Liu, Roberto Galván-Madrid, Jan Forbrich +9
We report JVLA 8-10 GHz (=3.0-3.7 cm) monitoring observations toward the YSO cluster R Coronae Australis (R\,CrA), taken in 2012, from March 15 to September 12. These observatio…
Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
Jae-Woo Kim, Alastair C. Edge, David A. Wake +11
We measure the angular clustering of 33 415 extremely red objects (EROs) in the Elais-N1 field covering 5.33 deg, which cover the redshift range to . This sample w…
The mass-metallicity relation at z~1.4 revealed with Subaru/FMOS
Kiyoto Yabe, Kouji Ohta, Fumihide Iwamuro +16
We present a stellar mass-metallicity relation at z~1.4 with an unprecedentedly large sample of ~340 star-forming galaxies obtained with FMOS on the Subaru Telescope. We observed K…
Mapping Compound Cosmic Telescopes Containing Multiple, Projected Cluster-Scale Halos
S. Mark Ammons, Kenneth C. Wong, Ann I. Zabludoff +1
Lines of sight with multiple, projected, cluster-scale halos have high total masses and complex lens plane interactions that can boost the area of magnification, or etendue, making…
From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N
Keping Qiu, Qizhou Zhang, Karl M. Menten +2
We report on detection of an ordered magnetic field (B field) threading a massive star-forming clump in the molecular cloud G35.2-0.74, using Submillimeter Array observations of po…
SMA observations on faint Submillimeter Galaxies with S < 2 mJy: Ultra Dusty Low-Luminosity Galaxies at High Redshift
Chian-Chou Chen, Lennox L. Cowie, Amy J. Barger +2
We obtained SMA observations of eight faint (intrinsic 850 m fluxes 2 mJy) submillimeter galaxies (SMGs) discovered in SCUBA images of the massive lensing cluster fields A37…
A Keplerian disk around a Class 0 source: ALMA observations of VLA1623A
Nadia M. Murillo, Shih-Ping Lai, Simon Bruderer +2
Context: Rotationally supported disks are critical in the star formation process. The questions of when do they form and what factors influence or hinder their formation have been…
Molecular Jet of IRAS 04166+2706
Liang-Yao Wang, Hsien Shang, Yu-Nung Su +5
The molecular outflow from IRAS 04166+2706 was mapped with the Submillimeter Array (SMA) at 350 GHz continuum and CO J = 32 at an angular resolution of ~1 arcsec. The field of v…
Physical Properties of Fullerene-containing Galactic Planetary Nebulae
Masaaki Otsuka, F. Kemper, J. Cami +2
We searched the Spitzer Space Telescope data archive for Galactic planetary nebulae (PNe), that show the characteristic 17.4 and um features due to C60, also known as buckminsterfu…
The Small Numbers of Large Kuiper Belt Objects
Megan E. Schwamb, Michael E. Brown, Wesley C. Fraser
We explore the brightness distribution of the largest and brightest (m(R)<22) Kuiper belt objects (KBOs). We construct a luminosity function of the dynamically excited or hot Kuipe…
CLASH-VLT: spectroscopic confirmation of a z=6.11 quintuply lensed galaxy in the Frontier Fields Cluster RXC J2248.7-4431
I. Balestra, E. Vanzella, P. Rosati +41
We present VIsible Multi-Object Spectrograph (VIMOS) observations of a z 6 galaxy quintuply imaged by the Frontier Fields galaxy cluster RXC J2248.7-4431 (z=0.348). This sub-L^*, h…
Pan-STARRS1: Galaxy Clustering in the Small Area Survey 2
Daniel J. Farrow, Shaun Cole, N. Metcalfe +11
The Pan-STARRS1 survey is currently obtaining imaging in 5 bands (grizy) for the steradian survey, one of the largest optical surveys ever conducted. The finished survey will…