ON-SKY SILICON PHOTOMULTIPLIER DETECTOR PERFORMANCE MEASUREMENTS FOR MILLISECOND TO SUB-MICROSECOND OPTICAL SOURCE VARIABILITY STUDIES

Loading...
Thumbnail Image

Date

2020

Authors

Lau, Albert Wai Kit
Shafiee, Mehdi
Smoot, George F.
Grossan, Bruce
Li, Siyang
Maksut, Zhanat

Journal Title

Journal ISSN

Volume Title

Publisher

arxiv

Abstract

In our Ultra-Fast Astronomy (UFA) program, we aim to improve measurements of variability of astro nomical targets on millisecond and shorter time scales. In this work, we present initial on-sky measurements of the performance of silicon photomultiplier detectors (SiPMs) for UFA. We mounted two different SiPMs at the focal plane of the 0.7-meter aperture Nazarbayev University Transient Telescope at the Assy-Turgen Astrophysical Observatory (NUTTelA-TAO), with no filter in front of the detector. The 3mm × 3mm SiPM single-channel detectors have a field of view of 2.27160 × 2.27160 . During the nights of 2019 October 28-29, we measured sky background, bright stars, and an artificial source with a 100Hz flashing frequency. We compared detected SiPM counts with Gaia satellite G-band flux values to show that our SiPMs have a linear response. With our two SiPMs (models S14520-3050VS and S14160-3050HS), we measured a dark current of ∼130 and ∼85 kilo counts per second (kcps), and a sky background of ∼201 and ∼203 kcps, respectively. We measured an intrinsic crosstalk of 10.34% and 10.52% and derived a 5σ sensitivity of 13.9 and 14.0 Gaia G-band magnitude for 200ms exposures, for the two detectors respectively. For a 10 µs window, and allowing a false alarm rate of once per 100 nights, we derived a sensitivity of 22 detected photons, or 6 Gaia G-band magnitudes. For nanosecond timescales, our detection is limited by crosstalk to 12 detected photons, which corresponds to a fluence of ∼155 photons per square meter

Description

Keywords

Type of access: Open Access, Ultra Fast Astronomy, Silicon photomultiplier, Millisecond optical variability

Citation

Lau, A. W. K., Shafiee, M., Smoot, G. F., Grossan, B., Li, S., & Maksut, Z. (2020). On-sky silicon photomultiplier detector performance measurements for millisecond to sub-microsecond optical source variability studies. Journal of Astronomical Telescopes, Instruments, and Systems, 6(04). https://doi.org/10.1117/1.jatis.6.4.046002

Collections