output
19962026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations

Showing 2019Show all

242 papers · 1 filter

astro-ph.GA2019★ 33 cited

ALMA observations reveal no preferred outflow--filament and outflow--magnetic field orientations

T. Baug, Ke Wang, Tie Liu +12

We present a statistical study on the orientation of outflows with respect to large-scale filaments and the magnetic fields. Although filaments are widely observed toward Galactic…

astro-ph.SR2019★ 4 cited

High-Resolution Near-Infrared Polarimetry and Sub-Millimeter Imaging of FS Tau A: Possible Streamers in Misaligned Circumbinary Disk System

Yi Yang, Eiji Akiyama, Thayne Currie +56

We analyzed the young (2.8-Myr-old) binary system FS Tau A using near-infrared (H-band) high-contrast polarimetry data from Subaru/HiCIAO and sub-millimeter CO (J=2-1) line emissio…

astro-ph.GA2019★ 29 cited

Balmer Break Galaxy Candidates at : a Potential View on the Star-Formation Activity at

Ken Mawatari, Akio K. Inoue, Takuya Hashimoto +15

We search for galaxies with a strong Balmer break (Balmer Break Galaxies; BBGs) at over a 0.41 deg effective area in the COSMOS field. Based on rich imaging data, in…

astro-ph.IM2019★ 6 cited

The CASA software for radio astronomy: status update from ADASS 2019

B. Emonts, R. Raba, G. Moellenbrock +28

CASA, the Common Astronomy Software Applications package, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and NSF's Karl G. Jans…

astro-ph.GA2019★ 60 cited

LLAMA: The - Relation of the most luminous local AGNs

Turgay Caglar, Leonard Burtscher, Bernhard Brand +17

The - relation is considered a result of co-evolution between the host galaxies and their super-massive black holes. For elliptical-bulge hosting inactive gala…

astro-ph.SR2019★ 8 cited

SUBARU Near-Infrared Imaging Polarimetry of Misaligned Disks Around The SR24 Hierarchical Triple System

Satoshi Mayama, Sebastián Pérez, Nobuhiko Kusakabe +65

The SR24 multi-star system hosts both circumprimary and circumsecondary disks, which are strongly misaligned from each other. The circumsecondary disk is circumbinary in nature. In…

astro-ph.SR2019★ 5 cited

Evolution from Spherical AGB Wind to Multipolar Outflow in Pre-Planetary Nebula IRAS 17150-3224

Po-Sheng Huang, Chin-Fei Lee, Raghvendra Sahai

We have mapped the pre-planetary nebula IRAS 17150-3224 in 350 GHz continuum and CO J=3-2 line at an angular resolution of about 0".09 using the Atacama Large Millimeter/submillime…

astro-ph.GA2019★ 18 cited

SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy, WISE1013+6112

Yoshiki Toba, Wei-Hao Wang, Tohru Nagao +6

We present far-infrared (FIR) properties of an extremely luminous infrared galaxy (ELIRG) at = 3.703, WISE J101326.25+611220.1 (WISE1013+6112). This ELIRG is selecte…

astro-ph.EP2019★ 5 cited

FLAMINGOS-2 infrared photometry of 2I/Borisov

Chien-Hsiu Lee, Hsing-Wen Lin, Ying-Tung Chen +1

2I/Borisov is the second interstellar object (ISO) after 'Oumuamua (Meech et al. 2017), but differs from 'Oumuamua drastically with its extensive cometary activity. A key ingredien…

astro-ph.GA2019★ 4 cited

Chemical properties of two dense cores in a Planck Galactic Cold Clump G168.72-15.48

Mengyao Tang, J. X. Ge, Sheng-Li Qin +8

To deepen our understanding of the chemical properties of the Planck Galactic Cold Clump (PGCC) G168.72-15.48, we performed observations of nine molecular species, namely, \ce{c-C3…

astro-ph.SR2019★ 29 cited

V346 Nor: the post-outburst life of a peculiar young eruptive star

Á. Kóspál, Zs. M. Szabó, P. Ábrahám +5

FU Orionis-type objects (FUors) are young low-mass stars undergoing powerful accretion outbursts. The increased accretion is often accompanied by collimated jets and energetic, lar…

astro-ph.CO2019★ 38 cited

XXL Survey groups and clusters in the Hyper Suprime-Cam Survey. Scaling relations between X-ray properties and weak lensing mass

Mauro Sereno, Keiichi Umetsu, Stefano Ettori +13

Scaling relations trace the formation and evolution of galaxy clusters. We exploited multi-wavelength surveys -- the XXL survey at \emph{XMM-Newton} in the X-ray band, and the Hype…

astro-ph.GA2019★ 10 cited

The HASHTAG project I. A Survey of CO(3-2) Emission from the Star Forming Disc of M31

Zongnan Li, Zhiyuan Li, Matthew W. L. Smith +26

We present a CO(3-2) survey of selected regions in the M31 disc as part of the JCMT large programme, HARP and SCUBA-2 High-Resolution Terahertz Andromeda Galaxy Survey (HASHTAG). T…

astro-ph.GA2019★ 109 cited

The East Asian Observatory SCUBA--2 survey of the COSMOS field: unveiling 1147 bright sub-millimeter sources across 2.6 square degrees

J. M. Simpson, Ian Smail, A. M. Swinbank +28

We present sensitive 850m imaging of the COSMOS field using 640hr of new and archival observations taken with SCUBA-2 at the East Asian Observatory's James Clerk Maxwell Telesco…

astro-ph.HE2019★ 1 cited

A geomagnetic filter for the Fermi-LAT background

D. A. Prokhorov, A. Moraghan

One of the unsolved questions in gamma-ray astronomy is whether the extragalactic gamma-ray background is of the discrete-source origin. To respond to this question, one first need…

astro-ph.IM2019★ 43 cited

Wideband 67-116 GHz receiver development for ALMA Band 2

P. Yagoubov, T. Mroczkowski, V. Belitsky +43

ALMA has been operating since 2011, but has not yet been populated with the full suite of intended frequency bands. In particular, ALMA Band 2 (67-90 GHz) is the final band in the…

astro-ph.GA2019★ 16 cited

Unveiling the importance of magnetic fields in the evolution of dense clumps formed at the waist of bipolar H II regions: a case study on Sh2-201 with JCMT SCUBA-2/POL-2

Chakali Eswaraiah, Di Li, Manash R. Samal +10

We present the properties of magnetic fields (B-fields) in two clumps (clump 1 and clump 2), located at the waist of the bipolar H II region Sh2-201, based on JCMT SCUBA-2/POL-2 ob…

astro-ph.CO2019★ 231 cited

TDCOSMO. I. An exploration of systematic uncertainties in the inference of from time-delay cosmography

M. Millon, A. Galan, F. Courbin +22

Time-delay cosmography of lensed quasars has achieved 2.4% precision on the measurement of the Hubble constant, . As part of an ongoing effort to uncover and control systemati…

astro-ph.CO2019★ 17 cited

Gas Density Perturbations in Cool Cores of CLASH Galaxy Clusters

Shutaro Ueda, Yuto Ichinohe, Sandor M. Molnar +2

We present a systematic study of gas density perturbations in cool cores of high-mass galaxy clusters. We select 12 relaxed clusters from the Cluster Lensing And Supernova survey w…

astro-ph.CO2019★ 39 cited

Anisotropies of galaxy ellipticity correlations in real and redshift space: angular dependence in linear tidal alignment model

Teppei Okumura, Atsushi Taruya

Investigating intrinsic alignments (IAs) of galaxy shapes is important not only to constrain cosmological parameters unbiasedly from gravitational lensing but also to extract cosmo…

astro-ph.GA2019★ 37 cited

SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-m-selected galaxies

Chen-Fatt Lim, Wei-Hao Wang, Ian Smail +35

We construct a SCUBA-2 450-m map in the COSMOS field that covers an area of 300 arcmin and reaches a 1 noise level of 0.65 mJy in the deepest region. We extract 256 sou…

astro-ph.GA2019★ 1.5k cited

The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

Romina Ahumada, Carlos Allende Prieto, Andres Almeida +310

This paper documents the sixteenth data release (DR16) from the Sloan Digital Sky Surveys; the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of…

astro-ph.CO2019★ 14 cited

RELICS: A Very Large () Cluster Lens -- RXC J0032.1+1808

Ana Acebron, Adi Zitrin, Dan Coe +38

Extensive surveys with the \textit{Hubble Space Telescope} (HST) over the past decade, targeting some of the most massive clusters in the sky, have uncovered dozens of galaxy-clust…

astro-ph.EP2019★ 15 cited

The detection of dust gap-ring structure in the outer region of the CR Cha protoplanetary disk

Seongjoong Kim, Sanemichi Takahashi, Hideko Nomura +13

We observe the dust continuum at 225 GHz and CO isotopologue (12CO, 13CO, and C18O) J=2-1 emission lines toward the CR Cha protoplanetary disk using the Atacama Large Millimeter/Su…