J/A+A/561/A146      SN 2010ae optical spectra             (Stritzinger+, 2014)

Optical and near-IR observations of the faint and fast 2008ha-like supernova 2010ae. Stritzinger M.D., Hsiao E., Valenti S., Taddia F., Rivera-Thorsen T.J., Leloudas G., Maeda K., Pastorello A., Phillips M.M., Pignata G., Baron E., Burns C.R., Contreras C., Folatelli G., Hamuy M., Hoeflich P., Morrell N., Prieto J.L., Benetti S., Campillay A., Haislip J.B., LaClutze A.P., Moore J.P., Reichart D.E. <Astron. Astrophys. 561, A146 (2014)> =2014A&A...561A.146S 2014A&A...561A.146S
ADC_Keywords: Supernovae ; Spectroscopy Keywords: supernovae: general - supernovae: individual: SN 2008ha - supernovae: individual: SN 2010ae Abstract: A comprehensive set of optical and near-infrared (NIR) photometry and spectroscopy is presented for the faint and fast 2008ha-like supernova (SN) 2010ae. Description: With substantial target-of-opportunity (ToO) access on Gemini- South (+GMOS) and the VLT (+X-Shooter), along with visitor nights at the NTT (+EFOSC, SOFI), SOAR (+GOODMAN), and du Pont (+WFCCD) telescopes, a detailed time series of optical and NIR spectroscopy was obtained for SN 2010ae. The resulting early phase time series consists of 21 spectra covering 20 epochs of optical spectroscopy, extending from -2d to +57d relative to T(B)max, as well as eight NIR spectra covering seven epochs ranging from -1d to +18d. Additionally, at late phases a visual-wavelength spectrum was taken with the VLT (+FORS2) on +252d. Objects: -------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------- 07 15 54.65 -57 20 36.9 SN 2010ae = SN 2010ae -------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 140 23 Journal of spectroscopic observations sp/* . 22 Individual spectra as FITS files -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 "date" Date Observation date (YYYY/MMM/DD) 13- 18 F6.2 d JD Julian date (JD-2455000) 20- 25 F6.1 d Phase Days since Bmax (JD-2455252.65) 27- 31 A5 --- Tel Telescope (1) 33- 40 A8 --- Inst Instrument 42- 52 A11 --- Grating Grating 54- 57 I4 0.1nm lam.min Wavelength range (lower value) 58 A1 --- --- [-] 59- 63 I5 0.1nm lam.max Wavelength range (upper value) 65- 68 F4.1 0.1nm Res1 ? First resolution (FWHM) 69 A1 --- --- [,] 70- 73 F4.1 0.1nm Res2 ? Second resolution (FWHM) 74 A1 --- --- [,] 75- 77 F3.1 0.1nm Res3 ? Third resolution (FWHM) 79- 80 I2 --- N1 Number of exposures for first observation 81 A1 --- --- [,] 82- 83 I2 --- N2 ? Number of exposures for second observation 84 A1 --- --- [,] 85- 86 I2 --- N3 ? Number of exposures for third observation 88- 91 I4 s t1 Integration time for first observation 92 A1 --- --- [,] 93- 95 I3 s t2 ? Integration time for second observation 96 A1 --- --- [,] 97- 99 I3 s t3 ? Integration time for third observation 101-140 A40 --- FileName Name of the fits file with spectrum in subdirectory sp -------------------------------------------------------------------------------- Note (1): the telescopes are: DUP = du Pont telescope (Las Campanas) SWO = Swope telescope (Las Campanas) SOAR = Southern Astrophysical Research (SOAR) Telescope (Chile) GEM-S = Gemini South (Chile) VLT = Very Large Telescope, ESO (Chile) -------------------------------------------------------------------------------- Acknowledgements: Maximilian Stritzinger, max(at)phys.au.dk
(End) Patricia Vannier [CDS] 03-Jan-2014
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