SIMBAD references

Rudy, Lynch, Mazuk, Russell, Pearson, Woodward, Puetter, and Perry, also report 0.4- to 2.5-micron spectroscopy of V2615 Oph (cf. IAUC 8824), obtained at Lick as above on May 7 UT, and 0.8- to 5.5-micron spectroscopy, obtained at the IRTF as above on May 31. This nova evolved dramatically between the two observations due to the formation of dust. The reddening derived from the O I lines jumped from E(B-V) = 1.0 to 1.3. The emission-line spectrum remained very rich and of low excitation with numerous features of Fe II and N I. The infrared Ca II triplet was present, and the C I lines were unusually strong, even for a nova. The carbon-monoxide emission reported by Das et al. on CBET 925 was no longer present.