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J/A+A/545/A68    Optical spectrum of the blazar PKS 0447-439  (Fumagalli+, 2012)

On the redshift of the blazar PKS 0447-439. Fumagalli M., Furniss A., O'Meara J., Prochaska J.X., Williams D., Farina E. <Astron. Astrophys. 545, A68 (2012)> =2012A&A...545A..68F
ADC_Keywords: BL Lac objects ; Spectroscopy Keywords: galaxies: active - BL Lacertae objects: individual: PKS 0447-439 - galaxies: distances and redshifts Abstract: PKS 0447-439 is one of the BL Lacertae objects that have been detected at very high energy. There has been a recent report of a lower limit of z≥1.246 for the redshift of this blazar, challenging the current paradigm in which very high-energy γ-rays cannot freely propagate in the z≳1 universe. In this research note, we present a new MagE/Magellan spectrum of PKS 0447-439 with exquisite signal-to-noise (S/N>150 at 6500Å). Our analysis confirms the presence of the previously-reported absorption line at 6280Å, which we identify, however, with a known telluric absorption, invalidating the claim that this blazar lies at z>1. Since no other extragalactic spectral features are detected, we cannot establish a redshift based on our spectrum. Description: MagE/Magellan optical spectrum of the blazar PKS 0447-439 (see Fig. 1 of the paper). Objects: ----------------------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------------------- 04 49 24.88 -43 50 09.7 PKS 0447-439 = CRATES J044924-435004 ----------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file spectrum.dat 35 11435 Optical spectrum of the blazar PKS 0447-439
Byte-by-byte Description of file: spectrum.dat
Bytes Format Units Label Explanations
1- 9 F9.4 0.1nm lambda [3500.1/8101] Observed wavelength 15- 22 F8.4 aW/m2/nm Flux Flux (10-16erg/cm2/s/Å) 29- 35 F7.5 aW/m2/nm e_Flux 1 sigma error on Flux (10-16erg/cm2/s/Å)
Acknowledgements: Michele Fumagalli, miki(at)ucolick.org
(End) Michele Fumagalli [UCSC], Patricia Vannier [CDS] 11-Aug-2012
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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