activity
20092026
most citedCharacterization and on-sky demonstration of an integrated photonic spectrograph for astronomy

87 citations · 284 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2026

Modeling the technical specifications for future multi-object spectroscopy instrumentation

Ummee Tania Ahmed, Andrew Hopkins, Simon Ellis

We investigate a proof-of-concept code designed to model the functionality of current generation astronomical fiber positioner instruments. This code accommodates an arbitrary numb…

astro-ph.IM2024★ 1 cited

Astrophotonics: recent and future developments

Simon Charles Ellis, Joss Bland-Hawthorn

Astrophotonics is a burgeoning field that lies at the interface of photonics and modern astronomical instrumentation. Here we provide a pedagogical review of basic photonic functio…

astro-ph.IM2017★ 21 cited

Photonic ring resonator filters for astronomical OH suppression

S. C. Ellis, S. Kuhlmann, K. Kuehn +9

Ring resonators provide a means of filtering specific wavelengths from a waveguide, and optionally dropping the filtered wavelengths into a second waveguide. Both of these features…

astro-ph.GA2012★ 42 cited

First Science with SAMI: A Serendipitously Discovered Galactic Wind in ESO 185-G031

Lisa M. R. Fogarty, Joss Bland-Hawthorn, Scott M. Croom +27

We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fibre bundles (hexabu…

astro-ph.IM2012★ 63 cited

First starlight spectrum captured using an integrated photonic micro-spectrograph

N. Cvetojevic, N. Jovanovic, C. Betters +4

Photonic technologies have received growing consideration for incorporation into next-generation astronomical instrumentation, owing to their miniature footprint and inherent robus…

astro-ph.IM2012★ 57 cited

Suppression of the near-infrared OH night sky lines with fibre Bragg gratings - first results

S. C. Ellis, J. Bland-Hawthorn, J. Lawrence +20

The background noise between 1 and 1.8 microns in ground-based instruments is dominated by atmospheric emission from hydroxyl molecules. We have built and commissioned a new instru…