J/A+A/339/165 J/A+A/339/165 The red spectrum of HD 101065 C R Cowley G Mathys Astron. Astrophys. 339 165 1998 1998A&A...339..165C Abundances, peculiar Spectra, red Stars, peculiar stars: abundances stars: chemically peculiar stars: individual (HD 101065) stars: magnetic fields Wavelength list for Przybylski's star (a rapidly rotation Ap star) including a measurement of the line depths.

HD 101065Przybylski's star11 37 37.2-46 42 37

Lambda Measured wavelength 0.1nm Int Measured central intensity number=1 Central depth of the line, as measured from a convolved and Fourier filtered spectrum (1.00 corresponds to the continuum level). --- Strength Line strength number=2 Estimate of the line strength on an arbitrary scale, derived from the measured line depth. Intensities of lines in the wing of H{alpha} are eye estimates, and not computed from the line depths. They are given with colons --- n_Strength : when eye estimates --- Id1 First identification number=3 Up to 4 possible contributing transitions are identified for the measured lines. The fractional part of the laboratory wavelength of the transition is given, followed by spectrum (e.g. Nd II). For most of the lanthanide spectra, the parenthesized number following the spectrum is the intensity from Meggers, Corliss, and Scribner (NBS Monog. 145, 1975). Iron-group spectra are typically followed by Multiplet numbers (e.g. Fe I-15 is a line from Multiplet 15). Energy levels are sometimes given for third spectra of the lanthanides. These are from Martin, Zalubas, and Hagan (NSRDS-NBS 60, 1978), or unpublished material provided to CRC by Hannah Crosswhite. Lines lacking energy-level classifications are designated "uncl." --- Id2 Second identification number=3 Up to 4 possible contributing transitions are identified for the measured lines. The fractional part of the laboratory wavelength of the transition is given, followed by spectrum (e.g. Nd II). For most of the lanthanide spectra, the parenthesized number following the spectrum is the intensity from Meggers, Corliss, and Scribner (NBS Monog. 145, 1975). Iron-group spectra are typically followed by Multiplet numbers (e.g. Fe I-15 is a line from Multiplet 15). Energy levels are sometimes given for third spectra of the lanthanides. These are from Martin, Zalubas, and Hagan (NSRDS-NBS 60, 1978), or unpublished material provided to CRC by Hannah Crosswhite. Lines lacking energy-level classifications are designated "uncl." --- Id3 Third identification number=3 Up to 4 possible contributing transitions are identified for the measured lines. The fractional part of the laboratory wavelength of the transition is given, followed by spectrum (e.g. Nd II). For most of the lanthanide spectra, the parenthesized number following the spectrum is the intensity from Meggers, Corliss, and Scribner (NBS Monog. 145, 1975). Iron-group spectra are typically followed by Multiplet numbers (e.g. Fe I-15 is a line from Multiplet 15). Energy levels are sometimes given for third spectra of the lanthanides. These are from Martin, Zalubas, and Hagan (NSRDS-NBS 60, 1978), or unpublished material provided to CRC by Hannah Crosswhite. Lines lacking energy-level classifications are designated "uncl." --- Id4 Fourth identification number=3 Up to 4 possible contributing transitions are identified for the measured lines. The fractional part of the laboratory wavelength of the transition is given, followed by spectrum (e.g. Nd II). For most of the lanthanide spectra, the parenthesized number following the spectrum is the intensity from Meggers, Corliss, and Scribner (NBS Monog. 145, 1975). Iron-group spectra are typically followed by Multiplet numbers (e.g. Fe I-15 is a line from Multiplet 15). Energy levels are sometimes given for third spectra of the lanthanides. These are from Martin, Zalubas, and Hagan (NSRDS-NBS 60, 1978), or unpublished material provided to CRC by Hannah Crosswhite. Lines lacking energy-level classifications are designated "uncl." --- G. Mathys (ESO, Santiago, Chile), Patricia Bauer CDS 1998Sep28Gautier Mathys <gmathys@eso.org> J_A+A_339_165.xml