output
19922026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2016Show all

620 papers · 1 filter

astro-ph.GA2016★ 23 cited

ALMA reveals Strong [CII] emission in a galaxy embedded in a giant Lyman-alpha blob at z=3.1

Hideki Umehata, Yuichi Matsuda, Yoichi Tamura +21

We report the result from observations conducted with the Atacama Large Millimeter/submillimeter Array (ALMA) to detect [CII] 158 um fine structure line emission from galaxies embe…

astro-ph.SR2016★ 22 cited

First determination of s-process element abundances in pre-main sequence clusters: Y, Zr, La, and Ce in IC 2391, the Argus association and IC 2602

Valentina D'Orazi, Gayandhi De Silva, Claudio Melo

Several high-resolution spectroscopic studies have provided compelling observational evidence that open clusters display a decreasing trend of their barium abundances as a function…

astro-ph.GA2016★ 168 cited

The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies

F. S. Tabatabaei, E. Schinnerer, M. Krause +17

We study the spectral energy distribution (SED) of the radio continuum emission from the KINGFISH sample of nearby galaxies to understand the energetics and origin of this emission…

astro-ph.GA2016★ 24 cited

The southern leading and trailing wraps of the Sagittarius tidal stream around the globular cluster Whiting1

Julio A. Carballo-Bello, Jesus M. Corral-Santana, David Martinez-Delgado +6

We present a study of the kinematics of 101 stars observed with VIMOS around Whiting1, a globular cluster embedded in the Sagittarius tidal stream. The obtained velocity distributi…

astro-ph.GA2016★ 5 cited

HCN hyperfine ratio analysis of massive molecular clumps

W. J. Schap, P. J. Barnes, A. Ordonez +3

We report a new analysis protocol for HCN hyperfine data, based on the PYSPECKIT package, and results of using this new protocol to analyse a sample area of seven massive molecular…

astro-ph.SR2016★ 10 cited

New ATCA, ALMA and VISIR observations of the candidate LBV SK-67266 (S61): the nebular mass from modelling 3D density distributions

C. Agliozzo, R. Nikutta, G. Pignata +10

We present new observations of the nebula around the Magellanic candidate Luminous Blue Variable S61. These comprise high-resolution data acquired with the Australia Telescope Comp…

astro-ph.SR2016★ 72 cited

SPHERE/SHINE reveals concentric rings in the debris disk of HIP 73145

M. Feldt, J. Olofsson, A. Boccaletti +22

The debris disk of HIP73145 has been detected in scattered light in the near-IR, and at far-IR wavelengths before, but no substructure has been seen so far. Detection of such subst…

astro-ph.EP2016★ 46 cited

First scattered-light images of the gas-rich debris disk around 49 Ceti

É. Choquet, J. Milli, Z. Wahhaj +31

We present the first scattered-light images of the debris disk around 49 ceti, a ~40 Myr A1 main sequence star at 59 pc, famous for hosting two massive dust belts as well as large…

astro-ph.SR2016★ 471 cited

X-Shooter spectroscopy of young stellar objects in Lupus: Accretion properties of class II and transitional objects

J. M. Alcala', C. F. Manara, A. Natta +11

We present the results of a study of the stellar and accretion properties of the (almost) complete sample of class II and transitional YSOs in the Lupus I, II, III and IV clouds, b…

astro-ph.GA2016★ 29 cited

In and out star formation in z~1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared

Raphael Gobat, Emanuele Daddi, Veronica Strazzullo +18

We present a sample of 34 spectroscopically confirmed BzK-selected ~1e11 Msun quiescent galaxies (pBzK) in the COSMOS field. The targets were initially observed with VIMOS on the V…

astro-ph.GA2016★ 36 cited

A Comparative Study of Multiwavelength Theoretical and Observed Light Curves of Cepheid Variables

Anupam Bhardwaj, Shashi M. Kanbur, Marcella Marconi +3

We analyse the theoretical light curves of Cepheid variables at optical ({\it UBVRI}) and near-infrared ({\it JKL}) wavelengths using the Fourier decomposition and principal compon…

astro-ph.EP2016★ 20 cited

Interferometric Evidence for Quantum Heated Particles in the Inner Region of Protoplanetary Disks around Herbig Stars

L. Klarmann, M. Benisty, M. Min +6

To understand the chemical composition of planets, it is important to know the chemical composition of the region where they form in protoplanetary disks. Due to its fundamental ro…

astro-ph.GA2016★ 534 cited

The Chandra Deep Field-South Survey: 7 Ms Source Catalogs

B. Luo, W. N. Brandt, Y. Q. Xue +23

We present X-ray source catalogs for the Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2 arcmin. Utilizing WAVDETECT for init…

astro-ph.CO2016★ 36 cited

A Type II Supernova Hubble diagram from the CSP-I, SDSS-II, and SNLS surveys

T. de Jaeger, S. González-Gaitán, M. Hamuy +15

The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in…

astro-ph.SR2016★ 39 cited

ALMA Observations of the Water Fountain Pre-Planetary Nebula IRAS 16342-3814: High-velocity bipolar jets and an Expanding Torus

R. Sahai, W. H. T. Vlemmings, T. Gledhill +4

We have mapped 12CO J=3-2 and other molecular lines from the "water-fountain" bipolar pre-planetary nebula (PPN) IRAS 16342-3814 with ~0."35 resolution using ALMA. We find (i) two…

astro-ph.CO2016★ 30 cited

Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data

Seth R. Siegel, Jack Sayers, Andisheh Mahdavi +17

We present a joint analysis of Chandra X-ray observations, Bolocam thermal Sunyaev-Zel'dovich (SZ) effect observations, Hubble Space Telescope (HST) strong lensing data, and HST an…

astro-ph.GA2016★ 35 cited

A Deconvolution Technique to Correct Deep Images of Galaxies from Instrumental Scattered Light

Emin Karabal, Pierre-Alain Duc, Harald Kuntschner +3

Deep imaging of the diffuse light emitted by the stellar fine structures and outer halos around galaxies is now often used to probe their past mass assembly. Because the extended h…

astro-ph.SR2016★ 38 cited

The VMC survey - XXIII. Model fitting of light and radial velocity curves of Small Magellanic Cloud classical Cepheids

Marcella Marconi, Roberto Molinaro, Vincenzo Ripepi +7

We present the results of the chi2 minimization model fitting technique applied to optical and near-infrared photometric and radial velocity data for a sample of 9 fundamental and…

astro-ph.SR2016★ 2 cited

On the age of the magnetically active WW Psa and TX Psa members of the beta Pictoris association

S. Messina, R. Santallo, T. G. Tan +6

There are a variety of different techniques available to estimate the ages of pre-main-sequence stars. Components of physical pairs, thanks to their strict coevality and the mass d…

astro-ph.SR2016★ 9 cited

Period-Color and Amplitude-Color Relations at Maximum and Minimum Light for RR Lyrae Stars in the SDSS Stripe 82 Region

Chow-Choong Ngeow, Shashi M. Kanbur, Anupam Bhardwaj +2

Investigation of period-color (PC) and amplitude-color (AC) relations at the maximum and minimum light can be used to probe the interaction of the hydrogen ionization front (HIF) w…

astro-ph.GA2016★ 133 cited

ALMA observations of atomic carbon in z~4 dusty star-forming galaxies

M. S. Bothwell, J. E. Aguirre, M. Aravena +15

We present ALMA [CI]() (rest frequency 492 GHz) observations for a sample of 13 strongly-lensed dusty star-forming galaxies originally discovered at 1.4mm in a blank-field sur…

astro-ph.GA2016★ 53 cited

Carbon monoxide in an extremely metal-poor galaxy

Yong Shi, Junzhi Wang, Zhi-Yu Zhang +4

Extremely metal-poor galaxies with metallicity below 10% of the solar value in the local universe are the best analogues to investigating the interstellar medium at a quasi-primiti…

astro-ph.GA2016★ 20 cited

Population mixtures and searches of lensed and extended quasars across photometric surveys

Peter Williams, Adriano Agnello, Tommaso Treu

Wide-field photometric surveys enable searches of rare yet interesting objects, such as strongly lensed quasars or quasars with a bright host galaxy. Past searches for lensed quasa…

astro-ph.GA2016★ 201 cited

The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

M. Bischetti, E. Piconcelli, G. Vietri +19

Models and observations suggest that both power and effects of AGN feedback should be maximised in hyper-luminous (L_Bol>10^47 erg/s) quasars, i.e. objects at the brightest end of…