ALMA Band-to-band Phase Referencing: Imaging Capabilities on Long Baselines and High Frequencies
Yoshiharu Asaki, Luke T. Maud, Edward B. Fomalont, William R. F. Dent,, Loreto Barcos-Mu\~noz, Neil M. Phillips, Akihiko Hirota, Satoko Takahashi,, Stuartt Corder, John M. Carpenter, Eric Villard

TL;DR
This study demonstrates the imaging capabilities of ALMA at high frequencies using band-to-band phase referencing over long baselines, achieving high resolution and analyzing phase correction effectiveness under different atmospheric conditions.
Contribution
It provides the first detailed assessment of ALMA's high-frequency imaging with long baselines using B2B phase referencing, including optimal switching cycle times and phase correction performance.
Findings
Achieved 14x11 mas resolution at 405 GHz.
Phase rms stability varies with atmospheric conditions.
20 s switching cycle improves phase correction at high frequencies.
Abstract
High-frequency long-baseline experiments with the Atacama Large Millimeter/submillimeter Array were organized to test the high angular resolution imaging capabilities in the submillimeter wave regime using baselines up to 16 km. Four experiments were conducted, two Band 7 (289 GHz) and two Band 8 (405 GHz) observations. Phase correction using band-to-band (B2B) phase referencing was used with a phase calibrator only 0.7deg away observed in Band 3 (96 GHz) and Band 4 (135 GHz), respectively. In Band 8, we achieved the highest resolution of 14x11 mas. We compared the synthesis images of the target quasar using 20 and 60 s switching cycle times in the phase referencing. In Band 7, the atmosphere had good stability in phase rms (<0.5 rad over 2 minutes), and there was little difference in image coherence between the 20 and 60 s switching cycle times. One Band 8 experiment was conducted…
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