Resolving the extended atmosphere and the inner wind of Mira (o Ceti) with long ALMA baselines

K. T. Wong; T. Kamiński; K. M. Menten; F. Wyrowski

doi:10.1051/0004-6361/201527867

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Volume 590 (June 2016)

A&A, 590 (2016) A127

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Table B.1

ALMA antenna pads deployed in Mira’s SV observation.


Nominal 2014 LBC array^a				Additional antennae^b


A113	A131	W207	P401	A001	A029	A078
A118	A132	W210	P402	A004	A035	A082
A121	A133	S301	P404	A005	A058	T701
A122	W201	S303	P405	A006	A072	T703
A124	W204	S306	P410	A011	A075
A127	W206	S309		A024	A076

Notes.

^(a)

23 antennae in the nominal 2014 ALMA Long Baseline Campaign (LBC) configuration with a minimum baseline of about 400 m (cf. Fig. 1 of ALMA Partnership et al. 2015).

^(b)

16 additional antennae of short spacings that were available during either day, or both days, of the Science Verification observation of Mira in ALMA Band 6.

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