January 16, 2015: THIS CAMPAIGN HAS BEEN CANCELLED. PLEASE SEE AAVSO SPECIAL NOTICE #395 FOR DETAILS.
December 5, 2014: Drs. Matthew W. Muterspaugh and Gregory W. Henry (Tennessee State University) have requested AAVSO observers' assistance in monitoring the possible Algol-like binary star alpha Com before, during, and after the eclipse they have predicted for mid-to-late January 2015.
Note: A thread for this campaign has been created in the AAVSO Campaigns and Observation Reports discussion forum: https://www.aavso.org/eps-aur-monitoring
CONTINUED AT LEAST THROUGH 2021 - Elizabeth O. Waagen, 17 April 2020
September 17, 2014: Dr. Robert Stencel (University of Denver Astronomy Program) has requested that AAVSO observers monitor epsilon Aurigae from now through the end of the observing season.
Notes: Please continue to monitor RT Cru as it continues to decline slowly from its outburst that began in 2021 and after it returns to minimum. - Elizabeth O. Waagen, April 4, 2023
This campaign has been extended indefinitely. Dr. Karovska requests monitoring of RT Cru until further notice. - Elizabeth O. Waagen, 17 April 2020
July 24, 2014:The eclipse of EE Cep (AAVSO Alert Notice 502) appears to be gradually beginning, according to observations in the AAVSO International Database. Please observe this system according to the instructions given in the Alert Notice.
Out-of-eclipse monitoring requested until further notice to study evolution of disk. - June 2017. Also, Special Notice #387 (20140724) updated this campaign.
June 20, 2014: Kris Z. Stanek (The Ohio State University) et al. reported the discovery during the ongoing All-Sky Automated Survey for SuperNovae (ASAS-SN) of a bright transient (10.66V) on 2014 June 14.52 UT. Data were obtained using the quadruple 14-cm "Brutus" telescope in Haleakala, HI (hosted by Las Cumbres Observatory Global Telescope Network).(ATel #6233, http://www.astronomerstelegram.org/?read=6233)
May 13, 2014: The HST/COS observations of the cataclysmic variable SBS 1108+574 described in AAVSO Alert Notice 501 and Special Notice #384 are scheduled for 2014 May 16 06:19:04 - 15:16:56 UT.
Your observations TONIGHT AND PARTICULARLY TOMORROW NIGHT ARE CRUCIAL!
May 9, 2014: The HST/COS observations of the cataclysmic variable SBS 1108+574 described in AAVSO Alert Notice 501 have been pushed back a few days. The new exact time of the observations is:
SBS 1108+574 2014 May 16 06:19:04 - 15:16:56 UT
April 29, 2014: Dr. Peter Garnavich (University of Notre Dame) and Dr. Paula Szkody (University of Washington) have requested the help of AAVSO observers in monitoring the cataclysmic variable SBS 1108+574 (= CSS 120422:111127+571239) in support of upcoming Hubble Space Telescope observations. The HST COS (Cosmic Origins Spectrograph) will be carrying out far-ultraviolet spectroscopy of this target on 2014 May 12-13 UT.
April 2, 2014
1. Nova Scorpii 2014 = TCP J17154683-3128303 [V1534 Sco]
2. Nova Cygni 2014 = PNV J20214234+3103296 [V2659 Cyg]
1. Nova Scorpii 2014 = TCP J17154683-3128303
Event: Nova Scorpii 2014 = TCP J17154683-3128303
Discovered by: Koichi Nishiyama (Kurume, Japan) and Fujio Kabashima (Miyaki, Japan)
