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101. ASPITZERSURVEY FOR DUST IN TYPE IIn SUPERNOVAE

103. THE MOST SLOWLY DECLINING TYPE Ia SUPERNOVA 2001ay

106. Peculiar Type II supernovae from blue supergiants

107. BROAD-LINE REVERBERATION IN THEKEPLER-FIELD SEYFERT GALAXY Zw 229-015

108. Nearby supernova rates from the Lick Observatory Supernova Search - II. The observed luminosity functions and fractions of supernovae in a complete sample

110. RESULTS OF THE LICK OBSERVATORY SUPERNOVA SEARCH FOLLOW-UP PHOTOMETRY PROGRAM: BVRI LIGHT CURVES OF 165 TYPE Ia SUPERNOVAE

112. NEAR-ULTRAVIOLET PROPERTIES OF A LARGE SAMPLE OF TYPE Ia SUPERNOVAE AS OBSERVED WITH THESwiftUVOT

113. THE MASSIVE PROGENITOR OF THE TYPE II-LINEAR SUPERNOVA 2009kr

114. VARIABLE SODIUM ABSORPTION IN A LOW-EXTINCTION TYPE Ia SUPERNOVA,

116. SN 2008ha: AN EXTREMELY LOW LUMINOSITY AND EXCEPTIONALLY LOW ENERGY SUPERNOVA

117. SN 2008S: A COOL SUPER-EDDINGTON WIND IN A SUPERNOVA IMPOSTOR

121. Optical and Near‐Infrared Observations of the Highly Reddened, Rapidly Expanding Type Ia Supernova SN 2006X in M100

122. Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. III. Optical Variability and X‐Ray/UV/Optical Correlations

123. A non-spherical core in the explosion of supernova SN 2004dj

124. Fourteen months of observations of the possible super-Chandrasekhar mass Type Ia Supernova 2009dc.

125. The Peculiar SN 2005hk: Do Some Type Ia Supernovae Explode as Deflagrations?Based in part on observations taken at the Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., (AURA) under cooperative agreement with the National Science Foundation.Based in part on observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium.Partly based on observations collected at the European Southern Observatory, Chile, in the course of program 076.A-0156.

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