Assessing the Suitability of H4RG Near Infrared Detectors for Precise Doppler Radial Velocity Measurements. (arXiv:1908.11429v1 [astro-ph.IM])

Assessing the Suitability of H4RG Near Infrared Detectors for Precise Doppler Radial Velocity Measurements. (arXiv:1908.11429v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Bechter_E/0/1/0/all/0/1">Eric B. Bechter</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bechter_A/0/1/0/all/0/1">Andrew J. Bechter</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Crepp_J/0/1/0/all/0/1">Justin R. Crepp</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Crass_J/0/1/0/all/0/1">Jonathan Crass</a>

At wavelengths longwards of the sensitivity of silicon, hybrid structured
mercury-cadmium-telluride (HgCdTe) detectors show promise to enable extremely
precise radial velocity (RV) measurements of late-type stars. The most advanced
near infrared (NIR) detector commercially available is the HAWAII series (HxRG)
of NIR detectors. While the quantum efficiency of such devices has been shown
to be approx ninety percent, the noise characteristics of these devices, and
how they relate to RV measurements, have yet to be quantified. We characterize
the various noise sources generated by H4RG arrays using numerical simulations.
We present recent results using our end-to-end spectrograph simulator in
combination with the HxRG Noise Generator, which emulates the effects of read
noise, parameterized by white noise, correlated and uncorrelated pink noise,
alternating column noise, and picture frame noise. The effects of nonlinear
pixel response, dark current, persistence, and interpixel capacitance (IPC) on
RV precision are also considered. Our results have implications for RV error
budgets and instrument noise floors that can be achieved with NIR Doppler
spectrographs that utilize this kind of detector.

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