J/A+A/573/A2        SN 2012Z spectra                        (Stritzinger+, 2015)

Comprehensive observations of the bright and energetic Type Iax SN 2012Z: Interpretation as a Chandrasekhar mass white dwarf explosion. Stritzinger M., Valenti S., Hoeflich P., Baron E., Phillips M.M., Taddia F., Foley R.J., Hsiao E.Y., Jha S.W., McCully C., Pandya V., Simon J.D., Benetti S., Brown P.J., Burns C.R., Campillay A., Contreras C., Forster F., Holmbo S., Marion G.H., Morrell N., Pignata G. <Astron. Astrophys. 573, A2 (2015)> =2015A&A...573A...2S 2015A&A...573A...2S
ADC_Keywords: Supernovae ; Spectroscopy ; Spectra, infrared Keywords: supernovae: individual: SN 2012Z - supernovae: individual: SN 2005hk - supernovae: general Description: We present 8 unpublished low-resolution visual-wavelength spectra of the Type Iax supernova 2012Z ranging from +1.8d to +248.1d relative to B-band maximum. In addition a high-resolution spectrum is presented obtained on -6.4d. Accompanying these data are 7 low-resolution spectra ranging from -9.2d to +33.8d, which were previously published by Foley et al. (2013ApJ...767...57F 2013ApJ...767...57F). The Foley et al. spectra were provided in normalized ascii format, which we have convert to fits format. Finally, we present the most comprehensive set of near-infrared spectra yet obtained for a Type Ia supernova. This includes 10 epochs ranging from -7.3d to +268.8d relative to B-band maximum. For spectra taken with ESO facilities a single fits file is present for each instrumental setup, i.e., each grating has its own fits file. For the FIRE spectra the one-dimensional spectra are stored in fits files as 2048x3 arrays, corresponding to the wavelength, flux and error values for each of the 2048 pixels across the detector. The wavelength and flux are as observed. Objects: ---------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------- 03 22 05.40 -15 23 14.9 SN 2012Z = SN 2012Z ---------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 129 34 List of FITS spectra fits/* . 34 Individual FITS spectra -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 6 I4 --- Nx ? Number of pixels along X-axis 8 I1 --- Nsp ? Number of spectra in the file 9 I1 --- Par ? Number of "sets" (first axis is wavelength) 11- 18 F8.3 nm lam.min [203/1500] Lower value of wavelength interval 19 A1 --- --- [/] 20- 27 F8.3 nm lam.max [506/2750] Upper value of wavelength interval 29- 37 F9.6 0.1nm dlam [0.05/11]? Spectral resolution 40- 49 A10 "date" Obs.Date Observation date 51- 54 I4 Kibyte size Size of FITS file 56- 85 A30 --- FileName Name of FITS file, in subdirectory fits 87- 91 F5.1 d Phase [-9.2/269] Phase (days since explosion) 93-129 A37 --- Title Title of the file -------------------------------------------------------------------------------- Acknowledgements: Maximilian Stritzinger, max(at)phys.au.dk
(End) Patricia Vannier [CDS] 14-Oct-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line