papers

Publications (22)

astro-ph.IM2020

ALMA Band-to-band Phase Referencing: Imaging Capabilities on Long Baselines and High Frequencies

Yoshiharu Asaki, Luke T. Maud, Edward B. Fomalont +8

High-frequency long-baseline experiments with the Atacama Large Millimeter/submillimeter Array were organized to test the high angular resolution imaging capabilities in the submil…

astro-ph.GA2020

A kpc-scale resolved study of unobscured and obscured star-formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS

Cheng Cheng, Edo Ibar, Ian Smail +12

We present Atacama Large Millimeter/Submillimeter Array (ALMA) continuum observations of a sample of nine star-forming galaxies at redshifts 1.47 and 2.23 selected from the High-$z…

astro-ph.IM2023

The ALMA Interferometric Pipeline Heuristics

Todd R. Hunter, Remy Indebetouw, Crystal L. Brogan +25

We describe the calibration and imaging heuristics developed and deployed in the ALMA interferometric data processing pipeline, as of ALMA Cycle 9. The pipeline software framework…

astro-ph.IM2021

The ObsMode 2020 Process

Satoko Takahashi, Edward B. Fomalont, Yoshiharu Asaki +11

ObsMode is a yearly process which aims at preparing capabilities for future ALMA Observing cycles. The process has been running for a number of years tied to each ALMA observing cy…

astro-ph.IM2014

The human pipeline: distributed data reduction for ALMA

Scott Schnee, Crystal Brogan, Daniel Espada +5

Users of the Atacama Large Millimeter/submillimeter Array (ALMA) are provided with calibration and imaging products in addition to raw data. In Cycle 0 and Cycle 1, these products…

astro-ph.IM2020

Synergies between ground-based and space-based observations in the solar system and beyond

Vincent Kofman, Chris Moeckel, Glenn Orton +12

Telescope and detector developments continuously enable deeper and more detailed studies of astronomical objects. Larger collecting areas, improvement in dispersion and detector te…