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J/A+A/534/A133   Proxima Cen chromospheric emission lines   (Fuhrmeister+, 2011)

Multi-wavelength observations of Proxima Centauri. Fuhrmeister B., Lalitha S., Poppenhaeger K., Rudolf N., Liefke C., Reiners A., Schmitt J.H.M.M., Ness J.-U. <Astron. Astrophys. 534, A133 (2011)> =2011A&A...534A.133F
ADC_Keywords: Stars, variable ; Stars, late-type ; Spectroscopy Keywords: stars: activity - stars: magnetic fields - stars: chromospheres - stars: coronae - stars: late-type - stars: individual: Proxima Centauri Abstract: We present an extensive identification catalog of chromospheric emission lines in the optical range for a flare on Proxima Centauri. The data were obtained with ESO's Kueyen telescope equipped with the UVES spectrograph on March 9/10, 11/12, 13/14 in 2009. The instrument was operated in dichroic mode (spectral coverage from 3290 to 4500 and from 6400 to 10080Å). We tabulate measured wavelength, line flux and FWHM for every line and also provide the rest wavelength from the Moore catalog which was used for identification (Moore, 1972, Nat. Stand. Ref. Data. Ser., 40). Few lines were identified with the NIST database. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 14 29 42.9 -62 40 46 Proxima Centaurus = V* V645 Cen ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table6.dat 93 474 Catalogue of chromospheric emission lines
See also: J/A+A/415/331 : HST/STIS spectra of alpha Cen A (Pagano+, 2004) J/A+A/459/669 : JHKs photometry around α Cen (Kervella+, 2006) J/A+A/464/373 : VRIZJHK photometry around Alpha Cen (Kervella+, 2007) Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 7 F7.2 0.1nm lambda1 Measured wavelength 9- 12 F4.2 0.1nm sigma Line width sigma 14- 21 E8.3 mW/m2 Flux Line flux (in erg/cm^2^/s) (1) 23- 33 F11.5 0.1nm lambda2 Catalogued wavelength 35- 38 A4 --- Ion Ion name 40- 43 I4 --- Mult Multiplet number 45 I1 --- q_Mult [0/2] Identification status flag (2) 47- 93 A47 --- Rem Remarks (3)
Note (1): Absolute errors are about a factor of 2, differential errors are much smaller Note (2): Line identification status as follows: 0 = secure line identification 1 = unsecure line identification (mostly due to single line out of multiplet) 2 = single line out of multiplet but secure identification, since line was secure identified in the megaflare of CN Leo Note (3): Abbreviations used: em = emission line core in absorption line NIST = line was identified using NIST no gaussian = line is fitted poorly by a Gaussian, flux has large errors
Acknowledgements: Birgit Fuhrmeister, bfuhrmeister(at)hs.uni-hamburg.de
(End) Birgit Fuhrmeister [Univ. Hamburg], Patricia Vannier [CDS] 25-Aug-2011
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

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