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19962026
most citedHigher Charmonia

809 citations · 28.2k across the 927 of their papers we have counts for

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Showing 2020 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA2020★ 37 cited

A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time

M. Lacy, J. A. Surace, D. Farrah +60

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main…

astro-ph.GA2020★ 5 cited

Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation

Maria Babakhanyan Stone, Daniela Bettoni, Renato Falomo +4

We present optical spectroscopy of the close companions of 22 low redshift (z<0.5) quasars (QSO) selected from a larger sample of QSO in the SDSS Stripe82 region for which both the…

astro-ph.GA2020★ 48 cited

Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations

S. Pezzuto, M. Benedettini, J. Di Francesco +20

(Abridged) In this paper, we present analyses of images taken with the Herschel ESA satellite from 70mu to 500mu. We first constructed column density and dust temperature maps. Nex…

astro-ph.GA2020★ 24 cited

Probing Interstellar Grain Growth Through Polarimetry in the Taurus Cloud Complex

John E. Vaillancourt, B-G Andersson, Dan P. Clemens +4

The optical and near-infrared (OIR) polarization of starlight is typically understood to arise from the dichroic extinction of that light by dust grains whose axes are aligned with…

astro-ph.GA2020★ 60 cited

Preliminary Target Selection for the DESI Milky Way Survey (MWS)

Carlos Allende Prieto, Andrew P. Cooper, Arjun Dey +31

The DESI Milky Way Survey (MWS) will observe 8 million stars between mag, supplemented by observations of brighter targets under poor observing conditions. The s…

astro-ph.GA2020★ 51 cited

The GOGREEN and GCLASS Surveys: First Data Release

Michael L. Balogh, Remco F. J. van der Burg, Adam Muzzin +42

We present the first public data release of the GOGREEN and GCLASS surveys of galaxies in dense environments, spanning a redshift range . The surveys consist of deep, mu…

astro-ph.GA2020★ 62 cited

FEEDBACK: a SOFIA Legacy Program to Study Stellar Feedback in Regions of Massive Star Formation

N. Schneider, R. Simon, C. Guevara +37

FEEDBACK is a SOFIA legacy program dedicated to study the interaction of massive stars with their environment. It performs a survey of 11 galactic high mass star forming regions in…

astro-ph.GA2020★ 23 cited

Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers

Onur Çatmabacak, Robert Feldmann, Daniel Anglés-Alcázar +3

The concurrent growth of supermassive black holes (SMBHs) and their host galaxies remains to be fully explored, especially at high redshift. While often understood as a consequence…

astro-ph.GA2020★ 42 cited

C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud: An analysis of the precision achievable when modeling spectral line within the Local Thermodynamic Equilibrium approximation

Antoine Roueff, Maryvonne Gerin, Pierre Gratier +23

CO isotopologue transitions are routinely observed in molecular clouds to probe the column density of the gas, the elemental ratios of carbon and oxygen, and to trace the kinematic…

astro-ph.GA2020★ 34 cited

Probing the circumnuclear absorbing medium of the buried AGN in NGC 1068 through NuSTAR observations

A. Zaino, S. Bianchi, A. Marinucci +9

We present the results of the latest NuSTAR monitoring campaign of the Compton-thick Seyfert 2 galaxy NGC 1068, composed of four 50 ks observations performed between July 201…

astro-ph.GA2020★ 11 cited

Galaxy And Mass Assembly (GAMA): Defining Passive Galaxy Samples and Searching for the UV Upturn

S. Phillipps, S. S. Ali, M. N. Bremer +16

We use data from the GAMA and GALEX surveys to demonstrate that the UV upturn, an unexpected excess of ultraviolet flux from a hot stellar component, seen in the spectra of many ea…