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MUSTANG-2 Overview
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MUSTANG-2 is a bolometer (continuum) camera with ~215 feedhorns and a bandpass from 75 to 105 GHz on the GBT. 

MUSTANG-2 is inherently a mapping instrument and observes by scanning “on-the-fly” (OTF). Our most common scan pattern is that of a Lissajous Daisy that can observe objects from our resolution (9″) to several arcminutes in size (more details on :ref:`mapping <references/receivers/mustang2/mustang2_mapping:MUSTANG-2 Mapping Information>`). For scans of ~a degree, we have switched to a raster scan. If you would like to consider another mapping strategy, please contact a member of :ref:`the MUSTANG-2 instrument <references/receivers/mustang2/mustang2_instrument_team:MUSTANG-2 Instrument Team>` team to inquire about it. The instantaneous field of view (FOV) is just over 4 arcminutes (4.2′). For full bandpass details see :ref:`this page <references/receivers/mustang2/mustang2_bandpass:MUSTANG-2 Bandpass Information>`.

MUSTANG-2 was commissioned on the GBT in spring 2016 (see development :ref:`timeline <references/receivers/mustang2/mustang2_dev:MUSTANG-2 Historical Development>`), and has been offered for observations on a shared risk basis, in collaboration with the instrument team, since the 2018A GBO proposal call. Several features distinguish it from its predecessor, MUSTANG:
	* A new, microstrip-coupled detector design yields higher sensitivity and less susceptibility to environmental microphonics.
	* Detectors are feedhorn coupled, with the sum of two linear polarizations measured by a single TES per feed.
	* The instantaneous field of view is 4 arcminutes (vs 42 arcseconds for MUSTANG)
	* The receiver design incorporates a tilted refrigerator and receiver rotator, resulting in much lower dependence of cooling performance on telescope elevation.
	* The detector readout is the first astronomical use of microwave resonators to multiplex TES bolometers.

MUSTANG-2 has been developed by a collaboration including the University of Pennsylvania, NIST, NRAO, the University of Michigan, and Cardiff University. All critical MUSTANG-2 systems have already been proven in operation on the GBT in early 2015 during an engineering run using a partially populated version of the receiver (“MUSTANG-1.5”, which had 64 populated feed horns).

Many :ref:`papers <references/receivers/mustang2/mustang2_publications:MUSTANG-2 Publications>` have been published using both MUSTANG and MUSTANG-2. 

Scientific Motivation for MUSTANG-2 and Future Upgrades
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See the `science cases for MUSTANG3 <https://greenbankobservatory.org/portal/gbt/instruments/mustang-3/>`__.
