@article{schaefer_eclipses_2011,
title = {Eclipses During the 2010 Eruption of the Recurrent Nova U Scorpii},
author = {Schaefer, Bradley E. and Pagnotta, Ashley and LaCluyze, Aaron and Reichart, Daniel E. and Ivarsen, Kevin M. and Haislip, Joshua B. and Nysewander, Melissa C. and Moore, Justin P. and Oksanen, Arto and Worters, Hannah L. and Sefako, Ramotholo R. and Mentz, Jaco and Dvorak, Shawn and Gomez, Tomas and Harris, Barbara G. and Henden, Arne and Tan, Thiam Guan and Templeton, Matthew and Allen, W. H. and Monard, Berto and Rea, Robert D. and Roberts, George and Stein, William and Maehara, Hiroyuki and Richards, Thomas and Stockdale, Chris and Krajci, Tom and Sjoberg, George and McCormick, Jennie and Revnivtsev, Mikhail and Molkov, Sergei and Suleimanov, Valery and Darnley, Matthew J. and Bode, Michael F. and Handler, Gerald and Lepine, Sebastien and Shara, Michael},
url = {http://arxiv.org/abs/1108.1214},
doi = {10.1088/0004-637X/742/2/113},
issn = {0004-637X, 1538-4357},
year = {2011},
date = {2011-12-01},
urldate = {2016-12-24},
journal = {The Astrophysical Journal},
volume = {742},
number = {2},
pages = {113},
abstract = {The eruption of the recurrent nova U Scorpii on 28 January 2010 is now the all-time best observed nova event. We report 36,776 magnitudes throughout its 67 day eruption, for an average of one measure every 2.6 minutes. This unique and unprecedented coverage is the first time that a nova has any substantial amount of fast photometry. With this, two new phenomena have been discovered: the fast flares in the early light curve seen from days 9-15 (which have no proposed explanation) and the optical dips seen out of eclipse from days 41-61 (likely caused by raised rims of the accretion disk occulting the bright inner regions of the disk as seen over specific orbital phases). The expanding shell and wind cleared enough from days 12-15 so that the inner binary system became visible, resulting in the sudden onset of eclipses and the turn-on of the supersoft X-ray source. On day 15, a strong asymmetry in the out-of-eclipse light points to the existence of the accretion stream. The normal optical flickering restarts on day 24.5. For days 15-26, eclipse mapping shows that the optical source is spherically symmetric with a radius of 4.1 R_sun. For days 26-41, the optical light is coming from a rim-bright disk of radius 3.4 R_sun. For days 41-67, the optical source is a center-bright disk of radius 2.2 R_sun. Throughout the eruption, the colors remain essentially constant. We present 12 eclipse times during eruption plus five just after the eruption.},
note = {arXiv: 1108.1214},
keywords = {},
pubstate = {published},
tppubtype = {article}
}

@article{tan_supernova_2009,
title = {Supernova 2009gg in Pgc 65919},
author = {Tan, T. G. and Jacques, C. and Pimentel, E.},
url = {http://adsabs.harvard.edu/abs/2009CBET.1848....1T},
year = {2009},
date = {2009-01-01},
urldate = {2016-12-24},
journal = {Central Bureau Electronic Telegrams},
volume = {1848},
pages = {1},
abstract = {CBET 1848 available at Central Bureau for Astronomical Telegrams.},
keywords = {},
pubstate = {published},
tppubtype = {article}
}

@article{tan_supernova_2008,
title = {Supernova 2008ff in Pgc 64319},
author = {Tan, T. G.},
url = {http://adsabs.harvard.edu/abs/2008CBET.1488....1T},
year = {2008},
date = {2008-09-01},
urldate = {2016-12-24},
journal = {Central Bureau Electronic Telegrams},
volume = {1488},
pages = {1},
abstract = {CBET 1488 available at Central Bureau for Astronomical Telegrams.},
keywords = {},
pubstate = {published},
tppubtype = {article}
}

@article{tan_supernova_2007,
title = {Supernova 2007rv in NGC 689},
author = {Tan, T. G. and Suzuki, M. and Nakano, S. and Nishiyama, K. and Kabashima, F.},
url = {http://adsabs.harvard.edu/abs/2007CBET.1152....1T},
year = {2007},
date = {2007-12-01},
urldate = {2016-12-24},
journal = {Central Bureau Electronic Telegrams},
volume = {1152},
pages = {1},
abstract = {CBET 1152 available at Central Bureau for Astronomical Telegrams.},
keywords = {},
pubstate = {published},
tppubtype = {article}
}