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Photometry of SN 2015da
In this paper we report the results of the first ~four years of spectroscopic and photometric monitoring of the Type IIn supernova SN 2015da (also known as PSN... -
Spectral log of (i)PTF stripped-envelope SN
We present an analysis of 507 spectra of 173 stripped-envelope (SE) supernovae (SNe) discovered by the untargeted Palomar Transient Factory (PTF) and intermediate PTF (iPTF)... -
NIR K-corrections
Type Ia Supernovae (SNe Ia) have been used as standardizable candles in the optical wavelengths to measure distances with an accuracy of ~7% out to redshift z~1.5. There is... -
SN 2007on and SN 2011iv light curves
We present an analysis of ultraviolet (UV) to near-infrared observations of the fast-declining Type Ia supernovae (SNe Ia) 2007on and 2011iv, hosted by the Fornax cluster member... -
Updated Type II supernova Hubble diagram
We present photometry and spectroscopy of nine Type II-P/L supernovae (SNe) with redshifts in the 0.045~ -
CSP-I photometry for 34 supernovae
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young,... -
PTF11mnb Bgri light curves
We study PTF11mnb, a He-poor supernova (SN) whose light curves resemble those of SN 2005bf, a peculiar double-peaked stripped-envelope (SE) SN, until the declining phase after... -
Photometry of supernova iPTF13z
We present optical photometry of Type IIn SN iPTF13z, obtained by the intermediate Palomar Transient Factory (iPTF) collaboration using the 1.2m Samuel Oschin telescope and the... -
Systematic survey of wind mass loss
Mass loss processes are a key uncertainty in the evolution of massive stars. They determine the amount of mass and angular momentum retained by the star, thus influencing its... -
SN Type Ibn OGLE-2014-SN-131 lightcurves
Type Ibn supernovae (SNe Ibn) are thought to be the core-collapse explosions of massive stars whose ejecta interact with He-rich circumstellar material (CSM). We report the... -
SN 2011dh. The first two years
We present optical and near-infrared (NIR) photometry and spectroscopy as well as modelling of the lightcurves of the Type IIb supernova (SN) 2011dh. Our extensive dataset, for... -
PESSTO catalog
The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. PESSTO classifies transients... -
Light curve templates of SNe Ib/c from SDSS
We present optical (ugriz) light curve templates of supernovae Ib/c from the SDSS II SN survey. Cone search capability for table J/A+A/574/A60/table1 (SDSS sample of 20 SNe Ib,... -
Light curves of 5 type IIn supernovae
We present optical (uBgVri) and near-infrared (YJHKs) photometry of Type IIn Supernovae 2005kj, 2006aa, 2006bo, 2006qq, 2008fq, obtained by the Carnege Supernova Project. We... -
2011fe spectrophotometric time series
We present 32 epochs of optical (3300-9700{AA}) spectrophotometric observations of the nearby quintessential "normal" type Ia supernova (SN Ia) SN 2011fe in the galaxy M101,... -
SNLS and SDSS SN surveys photometric calibration
We present a joined photometric calibration for the SNLS and the SDSS supernova surveys. Our main delivery are catalogs of natural AB magnitudes for a large set of selected... -
SN 1987A images at 350 and 870um
Supernova 1987A (SN 1987A) in the neighbouring Large Magellanic Cloud offers a superb opportunity to follow the evolution of a supernova and its remnant in unprecedented detail.... -
Spectroscopy of SN 2005cf
The ESC-RTN optical spectroscopy data set for SN 2005cf is presented and analyzed. The observations range from -11.6 and +77.3 days with respect to B-band maximum light. The... -
Abundances in the early Galaxy
In the framework of the ESO Large Programme "First Stars", very high-quality spectra of some 70 very metal-poor dwarfs and giants were obtained with the ESO VLT and UVES... -
Revised photometry of SNIa
Re-calibrated B magnitudes and (B-V) colors for the stars of the local sequences used at Asiago in the seventies as reference for the SN photometry are given in table3. For...
