An innovative integral field unit upgrade with 3D-printed micro-lenses for the RHEA at Subaru

In the new era of Extremely Large Telescopes (ELTs) currently under construction, challenging requirements drive spectrograph designs towards techniques that efficiently use a facility's light collection power. Operating in the single-mode (SM) regime, close to the diffraction limit, reduces the footprint of the instrument compared to a conventional high-resolving power spectrograph. The custom built injection fiber system with 3D-printed microlenses on top of it for the replicable high-resolution exoplanet and asteroseismology spectrograph (RHEA) at Subaru in combination with extreme adaptive optics of SCExAO, proved its high efficiency in a lab environment, manifesting up to ~77% of the theoretical predicted performance.

[1]  Shane Jacobson,et al.  Extra-solar planets exploration using frequency comb: Infrared Doppler instrument for the Subaru telescope (IRD) , 2012, 2015 Optical Fiber Communications Conference and Exhibition (OFC).

[2]  Robert J. Harris,et al.  Micro-lens arrays as tip-tilt sensor for single mode fiber coupling , 2018, Astronomical Telescopes + Instrumentation.

[3]  Miguel de Val-Borro,et al.  The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package , 2018, The Astronomical Journal.

[4]  Olivier Guyon,et al.  Performance of Subaru adaptive optics system AO188 , 2010, Astronomical Telescopes + Instrumentation.

[5]  Frantz Martinache,et al.  Wavefront Sensing and Control R&D on the SCExAO Testbed , 2020 .

[6]  John D. Hunter,et al.  Matplotlib: A 2D Graphics Environment , 2007, Computing in Science & Engineering.

[7]  E. N. Hubbard,et al.  Operation of a long fused silica fiber as a link between telescope and spectrograph. , 1979 .

[8]  J. Allington-Smith Basic principles of integral field spectroscopy , 2006 .

[9]  Wolfgang Freude,et al.  Printed freeform lens arrays on multi-core fibers for highly efficient coupling in astrophotonic systems. , 2017, Optics express.

[10]  Olivier Guyon,et al.  Precision single mode fibre integral field spectroscopy with the RHEA spectrograph , 2016, Astronomical Telescopes + Instrumentation.

[11]  Olivier Guyon,et al.  Commissioning status of Subaru laser guide star adaptive optics system , 2010, Astronomical Telescopes + Instrumentation.

[12]  J. L. E. DREYER,et al.  Astronomical Spectroscopy , 1894, Nature.

[13]  Olivier Guyon,et al.  Current status of the laser guide star adaptive optics system for Subaru Telescope , 2008, Astronomical Telescopes + Instrumentation.

[14]  G. Perrin,et al.  The Subaru Coronagraphic Extreme Adaptive Optics System: Enabling High-Contrast Imaging on Solar-System Scales , 2015, 1507.00017.

[15]  O. Guyon,et al.  Efficient injection from large telescopes into single-mode fibres: Enabling the era of ultra-precision astronomy , 2017, 1706.08821.

[16]  Gaël Varoquaux,et al.  The NumPy Array: A Structure for Efficient Numerical Computation , 2011, Computing in Science & Engineering.

[17]  Prasanth H. Nair,et al.  Astropy: A community Python package for astronomy , 2013, 1307.6212.

[18]  A. Hopkins,et al.  The Sydney-AAO Multi-object Integral field spectrograph , 2011, 1112.3367.

[19]  W. Freude,et al.  In situ 3D nanoprinting of free-form coupling elements for hybrid photonic integration , 2018 .

[20]  J R. Powell Application Of Optical Fibres To Astronomical Instrumentation , 1984, Astronomical Telescopes and Instrumentation.

[21]  Michael J. Ireland,et al.  RHEA: the ultra-compact replicable high-resolution exoplanet and Asteroseismology spectrograph , 2014, Astronomical Telescopes and Instrumentation.

[22]  Joss Bland-Hawthorn,et al.  The Photonic TIGER: a multicore fiber-fed spectrograph , 2012, Other Conferences.

[23]  James Roger P. Angel,et al.  Optical spectroscopy with a near-single-mode fiber-feed and adaptive optics , 1998, Astronomical Telescopes and Instrumentation.