activity
19962023
most citedLas Cumbres Observatory Global Telescope Network

1.2k citations · 4.8k across the 56 of their papers we have counts for

collaborators

57 papers

astro-ph.IM2023★ 28 cited

Data Combination: Interferometry and Single-dish Imaging in Radio Astronomy

Adele Plunkett, Alvaro Hacar, Lydia Moser-Fischer +11

Modern interferometers routinely provide radio-astronomical images down to subarcsecond resolution. However, interferometers filter out spatial scales larger than those sampled by…

astro-ph.IM2022★ 1.1k cited

CASA, the Common Astronomy Software Applications for Radio Astronomy

THE CASA TEAM, Ben Bean, Sanjay Bhatnagar +46

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.IM2022★ 27 cited

CASA on the fringe -- Development of VLBI processing capabilities for CASA

Ilse M. van Bemmel, Mark Kettenis, Des Small +14

New functionality to process Very Long Baseline Interferometry (VLBI) data has been implemented in the CASA package. This includes two new tasks to handle fringe fitting and VLBI-s…

astro-ph.IM2021

Using script generators for pipeline prototyping

Dirk Petry

Fully automated astronomical data calibration and imaging pipelines are difficult to develop without a good prototyping method which permits to bridge the time between observatory…

astro-ph.IM2021★ 1 cited

Improving ALMA's data processing effciency using a holistic approach

Theodoros Nakos, Harold Francke, Kouichiro Nakanishi +7

ALMA (Atacama Large Millimeter/submillimeter Array) is the world's largest ground-based facility for observations in the millimeter/submillimeter regime. One of ALMA's outstanding…

astro-ph.IM2020

New methods for ALMA angular-scale based observation scheduling, quality assessment, and beam shaping

Dirk Petry, María Díaz Trigo, Rüdiger Kneissl +2

Up to now, the completion of an ALMA interferometric observation is determined based on the achievement of a given shape and size of the synthesized beam and the noise RMS in the r…