Optical Frequency Comb as a general-purpose and wide-band calibration source for astronomical high resolution infrared spectrographs

Autor: Andrea Tozzi, Ernesto Oliva, Carlo Baffa, Elisabetta Giani, Pablo Cancio Pastor, Giulia Schettino, Massimo Inguscio
Rok vydání: 2011
Předmět:
Zdroj: Experimental astronomy
31 (2011): 69–81. doi:10.1007/s10686-011-9232-7
info:cnr-pdr/source/autori:Schettino Giulia [ 1,2 ] ; Oliva Ernesto [ 2 ] ; Inguscio Massimo [ 1,3,4 ] ; Baffa Carlo [ 2 ] ; Giani Elisabetta [ 2 ] ; Tozzi Andrea [ 2 ] ; Cancio Pastor Pablo [ 3,4 ]/titolo:Optical Frequency Comb as a general-purpose and wide-band calibration source for astronomical high resolution infrared spectrographs/doi:10.1007%2Fs10686-011-9232-7/rivista:Experimental astronomy (Print)/anno:2011/pagina_da:69/pagina_a:81/intervallo_pagine:69–81/volume:31
ISSN: 1572-9508
0922-6435
DOI: 10.1007/s10686-011-9232-7
Popis: A spectrally filtered Optical Frequency Comb (OFC) laser is proposed as a versatile calibration source for astronomical spectrometers in the 1-2 mu m spectral range. Such a source overcomes the limitations of current calibration lamps providing a uniform spectrum of equally spaced lines with similar intensity and extremely high long-term frequency stability. We present preliminary studies and results of a system which filters the OFC from a 100 MHz comb spacing to 16 GHz one, an adequate spacing for spectrometers with resolving power Delta lambda/lambda > 30000. The first approach employs two Fabry-Perot cavities in series, made of dielectric coated mirrors, followed by a non-linear optical broadening system. The limitations of such a filtering process are discussed. These can be overcome by the second approach, based on filtering cavities with metallic coated mirrors.
Databáze: OpenAIRE