photometry of SN 2013gh and iPTF13dge (Ferretti+, 2016)
R. Ferretti (Author), T. Petrushevska (Author)

Abstract

Measured photometry of type Ia supernovae 2013gh and iPTF13dge are presented. Furthermore, the effective light-curve-width-corrected phase and the natural magnitude in specified filters have been computed. Thereby, the corresponding Galactic absorption (Ax_MW) and the filter corrections (Kx) to the corresponding rest-frame filter for SN 2011fe as described by Amanullah et al. (2015MNRAS.453.3300A) are presented. The corrected magnitude can be obtained as X-AXMW-KX. All corrections have been calculated after the SN 2011fe template has been reddened with the best-fit Fitzpatrick (1999PASP..111...63F) law, for each SN. Furthermore, the V magnitude and corrections for each phase phase are included. The V magnitude was either measured (M) or calculated (D) using the SNooPy model. The V magnitude is only shown for data points used in the colour analysis, with phases between -10 and +35-days. The corrected colour can be obtained as (X-AXMW-KX)-(V-AVMW-KV) and can be compared with the corresponding colour of SN 2011fe in order to study the reddening laws of the SNe.

Keywords

supernovae;photometry;UBV;catalogs;

Data

Language: English
Year of publishing:
Typology: 2.20 - Research Data
Organization: UNG - University of Nova Gorica
Publisher: UDS/CNRS
UDC: 52
COBISS: 4997371 Link will open in a new window
Views: 3006
Downloads: 0
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Other data

URN: URN:SI:UNG
Type (COBISS): Not categorized
ID: 10900337
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