Early spectral evolution of Nova Sgr 2004 (Ederoclite+, 2006)

Details Early spectral evolution of Nova Sgr 2004 (Ederoclite+, 2006) Early spectral evolution of Nova Sgr 2004 (Ederoclite+, 2006)

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34590875e&link_type=abstract

VizieR On-line Data Catalog: J/A+A/459/875. Originally published in: 2006A&A...459..875E

Physics

Binaries: Cataclysmic, Novae, Spectroscopy

Scientific paper

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)
(4 data files).

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