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20022026
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 11.6k across the 119 of their papers we have counts for

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Showing 2017Show all

8 papers · 1 filter

astro-ph.GA2017★ 109 cited

The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses

Yiping Shu, Joel R. Brownstein, Adam S. Bolton +8

We present the full sample of 118 galaxy-scale strong-lens candidates in the Sloan Lens ACS (SLACS) Survey for the Masses (S4TM) Survey, which are spectroscopically selected from t…

astro-ph.GA2017★ 126 cited

Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z~2-4 as probed by multi-J CO lines

C. Yang, A. Omont, A. Beelen +18

(abridged) We present the IRAM-30m observations of multiple-J CO and CI line emission in a sample of redshift ~2-4 Herschel-ATLAS SMGs. A non-negligible effect of differential lens…

astro-ph.GA2017★ 41 cited

Planck's dusty GEMS. IV. Star formation and feedback in a maximum starburst at z=3 seen at 60-pc resolution

R. Canameras, N. Nesvadba, R. Kneissl +7

We present an analysis of high-resolution ALMA interferometry of CO(4-3) line emission and dust continuum in the "Ruby" (PLCK_G244.8+54.9), a bright, gravitationally lensed galaxy…

astro-ph.GA2017★ 41 cited

Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass

Francesco Shankar, Alessandro Sonnenfeld, Gary A. Mamon +9

We carry out a systematic investigation of the total mass density profile of massive (Mstar>2e11 Msun) early-type galaxies and its dependence on galactic properties and host halo m…

astro-ph.GA2017★ 23 cited

Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5

R. Canameras, N. P. H. Nesvadba, R. Kneissl +8

We study the properties of the foreground galaxy of the Ruby, the brightest gravitationally lensed high-redshift galaxy on the sub-millimeter sky as probed by the Planck satellite,…

astro-ph.CO2017★ 22 cited

Multipolar moments of weak lensing signal around clusters. Weighing filaments in harmonic space

C. Gouin, R. Gavazzi, S. Codis +3

Context. Upcoming weak lensing surveys such as Euclid will provide an unprecedented opportunity to quantify the geometry and topology of the cosmic web, in particular in the vicini…