<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Rau, A.</style></author><author><style face="normal" font="default" size="100%">Burwitz, V.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Cenko, S. B.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Correction to ATel 1152: Optical Spectroscopy of Nova M31N 2007-07c</style></title><short-title><style face="normal" font="default" size="100%">The Astronomer's Telegram</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Novae</style></keyword><keyword><style  face="normal" font="default" size="100%">Optical</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2007</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2007/07/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2007ATel.1153....1R</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">1153</style></volume><pages><style face="normal" font="default" size="100%">1</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">The Author list was incomplete in ATel#1152. On 2007 July 21.46 UT a spectrum of the nova candidate M31N 2007-07c (see ATel#1146, ATel#1149) was obtained with Double-Beam Spectrograph on the Palomar Hale-5m telescope. The 400/6000 grism (3.5 angstrom FWHM) and 158/7500 grating (8.6 angstrom FWHM) were used with 1200s exposure, each. The H-alpha line displays a P-Cygni profile. The measured expansion velocity is -1630+/-20 km/ sec (blue shifted), based on measurements of the Ca H+K lines, the G Band, H-beta, Mg lines and the near-infrared Ca-triplet.</style></abstract></record></records></xml>