J/A+A/459/875     Early spectral evolution of Nova Sgr 2004  (Ederoclite+, 2006)

Early spectral evolution of Nova Sgr 2004 (V5114 Sgr). Ederoclite A., Mason E., Della Valle M., Gilmozzi R., Williams R.E., Germany L., Saviane I., Matteucci F., Schaefer B.E., Walter F., Rudy R.J., Lynch D., Mazuk S., Venturini C.C., Puetter R.C., Perry R.B., Liller W., Rotter A. <Astron. Astrophys. 459, 875 (2006)> =2006A&A...459..875E 2006A&A...459..875E
ADC_Keywords: Binaries, cataclysmic ; Novae ; Spectroscopy Keywords: stars: novae, cataclysmic variables - stars: individual: V5114 Sgr Abstract: We present optical and near-infrared spectral evolution of the Galactic nova V5114 Sgr (2004) during few months after the outburst. We use multi-band photometry and line intensities derived from spectroscopy to put constrains on the distance and the physical conditions of the ejecta of V5114 Sgr. Description: Data files of FEROS observations are given with four digits (referring to month and day of observation) and an "f" indicating that that is a FEROS observation. Data files of observations carried out at Cerro Tololo are named with four digits (referring to month and day of observation) and a "t" indicating that these are CTIO observations. Observations carried out with the NIRIS instrument are given in three dat files. Although they were carried out on a single night, for uniformity with the rest of the files, these data files are named with four digits (referring to month and day of observation), an "n" indicating that is a NIRIS observation and a letter indicating the wavelength range ("o" for 500-1000nm , "b" for 800-1400nm and "r" for 1400-2500nm) Objects: ------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------ 18 19 32.3 -28 36 36 V5114 Sgr = NOVA Sgr 2004 ------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file obs.dat 29 35 List of spectroscopic observations sp/0622n*.dat . 3 NIRIS observations sp/*f.dat . 7 FEROS observations sp/*t.dat . 25 CTIO observations -------------------------------------------------------------------------------- Byte-by-byte Description of file: obs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 "YYYY/MM/DD" Date Observation date 12- 16 A5 --- Inst Instrument 18 A1 --- n_Inst [bor] Note on NIRIS instrument (1) 20- 29 A10 --- FileName Name of the file containing the spectrum, in "sp" subdirectory -------------------------------------------------------------------------------- Note (1): NIRIS wavelength ranges as follows: o = 500-1000nm b = 800-1400nm r = 1400-2500nm -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/*[ft].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.4 0.1nm lambda Wavelength 12- 24 E13.8 10mW/m2/nm Flux Flux (in mW/m2/Å) -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/0622n*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 6- 13 F8.6 um lambda Wavelength 14- 26 E13.7 mW/cm2/um Flux Flux -------------------------------------------------------------------------------- Acknowledgements: Alessandro Ederoclite, aederocl(at)vub.ac.be
(End) Patricia Vannier [CDS] 30-Nov-2006
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