Complex phase masks for fabricating OH-suppression filters for astronomy

Abstract

The design of a complex phase mask (CPM) for inscribing aperiodic filters in fibers is presented. The complex structure of the mask surface relief consists of discrete aperiodic phase-steps at periodic intervals. We show that the diffraction of the inscribing laser beam from the phase-step locations of the CPM produces periodically located half phase-steps along the fiber. The accumulated phase, along with controlled index modulation, generates the desired aperiodic reflection spectrum. Compared to a complex 'running-light' interferometry based inscription method, CPM offers the well known convenience and reproducibility of the standard phase mask inscription technique. The complexity of an aperiodic grating is encoded into the structure of the CPM. Complex filters fabricated with CPM can be used for suppressing the near infrared (NIR) OH- emission lines generated in the upper atmosphere, improving the performance of ground based telescopes.

arXiv comment4 Pages, 4 figures, to be submitted to IEEE Photonics Technology Letters

References in corpus (4)

• GNOSIS: the first instrument to use fibre Bragg gratings for OH suppression
• The case for OH suppression at near-infrared wavelengths
• Suppression of the near-infrared OH night sky lines with fibre Bragg gratings - first results
• First demonstration of OH suppression in a high efficiency near-infrared spectrograph