activity
19992019
most citedThe [OII]3727 Luminosity Function of the Local Universe

54 citations · 225 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2019

CASA 6: Modular Integration in Python

Ryan Raba, Darrell Schiebel, Bjorn Emonts +6

CASA, the Common Astronomy Software Applications, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and the Karl G. Jansky Very La…

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.IM2011

Reflex: Scientific Workflows for the ESO Pipelines

Pascal Ballester, Daniel Bramich, Vincenzo Forchi +5

The recently released Reflex scientific workflow environment supports the interactive execution of ESO VLT data reduction pipelines. Reflex is based upon the Kepler workflow engine…

astro-ph.CO2010★ 40 cited

The minor role of gas-rich major mergers in the rise of intermediate-mass early types at z <~ 1

C. López-Sanjuan, M. Balcells, P. G. Pérez-González +4

We study the evolution of galaxy structure since z ~ 1 to the present. From a GOODS-S multi-band catalog we define (blue) luminosity- and mass-weighted samples, limited by M_B <= -…

astro-ph.CO2009★ 38 cited

Robust determination of the major merger fraction at z = 0.6 in Groth Strip

C. López-Sanjuan, M. Balcells, C. E. García-Dabó +6

(Abridged) We measure the fraction of galaxies undergoing disk-disk major mergers (f_m) at intermediate redshifts (0.35 <= z < 0.85) by studying the asymmetry index A of galaxy ima…

astro-ph2008★ 11 cited

A maximum likelihood method for bidimensional experimental distributions, and its application to the galaxy merger fraction

C. López-Sanjuan, C. E. García-Dabó, M. Balcells

The determination of galaxy merger fraction of field galaxies using automatic morphological indices and photometric redshifts is affected by several biases if observational errors…