Though the time-domain millimeter sky is yet to be well characterized, the scarcity of millimeter observing resources in the world at present hampers progress toward it. In efforts to bolster the exploration of millimeter transients, we present the Stokes Polarization Radio Interferometer for Time-Domain Experiments (SPRITEly). Located at the Owens Valley Radio Observatory, SPRITEly is currently deployed as a two-element short-baseline 90 GHz interferometer uniquely focused on monitoring bright variable millimeter-continuum sources. We leverage two existing 10.4 m antennas and their existing receiver systems to begin, but we make significant upgrades to the back-end system during the commissioning process. With the ability to achieve rms noise of a few mJy, we plan to monitor known variable sources along with new nearby transients detected from optical surveys at high cadence, with the goal of producing well-sampled light curves. Interpreting these data in conjunction with multiwavelength observations stands to provide insight into the physical properties of the sources that produce transient millimeter emission. We present commissioning and early-science observations that demonstrate the performance of the instrument, including observations of the flaring BL Lac object S2 0109+22 and a periastron passage of the binary T Tauri system DQ Tau.
SPRITEly: Time-domain Millimeter Interferometry at the Owens Valley Radio Observatory
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© 2024. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Acknowledgement
The Owens Valley Radio Observatory is located on the ancestral homelands of the Big Pine Paiute Tribe of the Owens Valley. We recognize and acknowledge the historical and cultural significance of these lands to members of the Tribe. The authors thank staff members of the Owens Valley Radio Observatory and the Caltech radio group, including Kristen Bernasconi, Stephanie Cha-Ramos, Charlie Harnach, Sarah Harnach, Lori McGraw, Paul Rasmussen, Andres Rizo, and Michael Virgin. Their tireless efforts were instrumental to the success of SPRITEly.
This material is based on work supported by the National Science Foundation under grant No. 1935980. We acknowledge funding from the Mt. Cuba Astronomical Foundation under a grant titled "SPRITEly: A New Window into the Explosive, Dark Universe." We would like to thank the director of OVRO, G. Hallinan, for access to the Alan Moffet Funds.
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Additional details
Funding
- National Science Foundation
- 1935980
- Mt. Cuba Astronomical Foundation
Dates
- Accepted
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2024-08-06
- Available
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2024-09-20Published