Prueban un método para investigar la inflación cósmica
Un equipo de astrónomos del Observatorio Astronómico Nacional de Japón (NAOJ), con la participación del Instituto de Astrofísica de Canarias (IAC), ha probado...
Pushing automated morphological classifications to their limits with the Dark Energy Survey
We present morphological classifications of ~27 million galaxies from the Dark Energy Survey (DES) Data Release 1 (DR1) using a supervised deep learning...
PyNeb: a new software for the analysis of emission lines
We describe an ongoing project to migrate the emission-line analysis package nebular from its current environment, IRAF, to a modern programming environment...
PyNeb: a new tool for analyzing emission lines. I. Code description and validation of results
Analysis of emission lines in gaseous nebulae yields direct measures of physical conditions and chemical abundances and is the cornerstone of nebular...
Pyodine: an open, flexible reduction software for iodine-calibrated precise radial velocities
Context. Many telescopes use an iodine (I 2) absorption cell to measure precise radial velocities (RVs), but their data reduction pipelines are all tailored to...
We describe a simple step-by-step guide to qualitative interpretation of galaxy spectra. Rather than an alternative to existing automated tools, it is put...
Quantifying the coherent outflows of galaxies around voids in the SDSS DR7
We report the detection, with a high level of confidence, of coherent outflows around voids found in the seventh data release of the Sloan Digital Sky Survey...
Quantifying the evidence for resonant damping of coronal waves with foot-point wave power asymmetry
We use Coronal Multi-channel Polarimeter (CoMP) observations of propagating waves in the solar corona together with Bayesian analysis to assess the evidence of...
QUEST1 Variability Survey. II. Variability Determination Criteria and 200k Light Curve Catalog
The QUEST (QUasar Equatorial Survey Team) Phase 1 camera has collected multibandpass photometry on a large strip of high Galactic latitude sky over a period of...