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[not part of Research Note] We report the discovery of a widely-separatedlow-mass binary as a candidate member of the $\sim$40 Myr Argus Association.Resolved imaging and astrometry with 2MASS and LDSS-3 reveal a common propermotion pair of red sources separated by 4.23''$\pm$0.11'', with the secondaryroughly one magnitude fainter at $i$, $z$ and $J$. Resolved spectroscopyindicates component types of M8pec and M9pec, the peculiarities arising fromweak Na I and strong VO absorption characteristic of low gravity sources. Withits small proper motion and estimated 75$\pm$25 pc distance, the BANYAN II toolindicates a membership probability of 93% in Argus, which would be consistentwith a pair of brown dwarfs of mass $\sim$0.04 M$_{\odot}$ separated by$\sim$300 AU.

A Candidate Wide Brown Dwarf Binary in the Argus Association: 2MASS J14504216-7841413 and 2MASS J14504113-7841383