Data reduction and analysis of our data follows closely that described in Buxton et al. (2012). The data on this site are public and may be used by other investigators. If you intend to make use of this data please inform our group by email to michelle.buxton@yale.edu and send copies of any resulting publications, including telegrams. Please acknowledge us in your paper by including a citation to the Buxton et al. (2012), mentioned above, and with the following: "This paper has made use of up-to-date SMARTS optical/near-infrared light curves that are available at www.astro.yale.edu/smarts/xrb/home.php. The Yale SMARTS XRB team is supported by NSF grants 0407063 and 070707 to Charles Bailyn." Please also include "SMARTS" as a facility keyword."

Buxton et al. (2012); "Optical and Near-Infrared Monitoring of the Black Hole X-ray Binary GX 339-4 during 2002-2010", AJ, 143, 130.