Maser observations with new instruments

TL;DR

This paper discusses recent and upcoming advancements in maser science enabled by new high-sensitivity radio telescopes like ALMA and JVLA, highlighting their potential for groundbreaking spectral line observations.

Contribution

It provides an overview of current and future instruments that will enhance maser research capabilities across various observatories.

Findings

ALMA and JVLA offer unprecedented sensitivity for maser observations

Upcoming telescopes will significantly expand maser science potential

Enhanced global networks will improve millimeter wavelength maser studies

Abstract

The Atacama Large Millimeter/submillimeter Array (ALMA), and the Jansky Very Large Array (JVLA) have recently begun probing the Universe. Both provide the largest collecting area available at locations on a high dry site, endowing them with unparalleled potential for sensitive spectral line observations. Over the next few years, these telescopes will be joined by other telescopes to provide advances in maser science, including NOEMA and the LMT. Other instruments of note for maser science which may commence construction include the North American Array, the CCAT, and an enlarged worldwide VLB network outfitted to operate into the millimeter wavelength regime.