activity
20112026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations · 12.8k across the 98 of their papers we have counts for

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Showing astro-ph.COShow all

5 papers · 1 filter

astro-ph.CO2013★ 181 cited

CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies

G. Barro, S. M. Faber, P. G. Perez-Gonzalez +32

We analyze the star-forming and structural properties of 45 massive (log(M/Msun)>10) compact star-forming galaxies (SFGs) at 2<z<3 to explore whether they are progenitors of compac…

astro-ph.CO2013★ 60 cited

Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2

Michael V. Maseda, Arjen van der Wel, Elisabete da Cunha +21

Spectroscopic observations from the Large Binocular Telescope and the Very Large Telescope reveal kinematically narrow lines (~50 km/s) for a sample of 14 Extreme Emission Line Gal…

astro-ph.CO2013★ 92 cited

How dead are dead galaxies? Mid-Infrared fluxes of quiescent galaxies at redshift 0.3 < z < 2.5: implications for star formation rates and dust heating

Mattia Fumagalli, Ivo Labbe, Shannon G. Patel +17

We investigate the star formation rates of quiescent galaxies at high redshift (0.3 < z < 2.5) using 3D-HST WFC3 grism spectroscopy and Spitzer mid-infrared data. We select quiesce…

astro-ph.CO2012★ 132 cited

Relative merits of different types of rest-frame optical observations to constrain galaxy physical parameters

Camilla Pacifici, Stephane Charlot, Jeremy Blaizot +1

We present a new approach to constrain galaxy physical parameters from the combined interpretation of stellar and nebular emission in wide ranges of observations. This approach rel…

astro-ph.CO2011★ 224 cited

Empirical determination of the shape of dust attenuation curves in star-forming galaxies

Vivienne Wild, Stephane Charlot, Jarle Brinchmann +4

We present a systematic study of the shape of the dust attenuation curve in star-forming galaxies from the far ultraviolet to the near infrared (0.15-2microns), as a function of sp…