SPRITEly: Time-domain Millimeter Interferometry at the Owens Valley Radio Observatory

Abstract 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.

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Publication Details

Journal
The Astronomical Journal
Published
2024-09-20
DOI
https://doi.org/10.3847/1538-3881/ad6cdb
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
0.00

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article

SPRITEly: Time-domain Millimeter Interferometry at the Owens Valley Radio Observatory

Vikram Ravi, Mark Hodges, James W. Lamb, Nitika Yadlapalli Yurk et al.
The Astronomical Journal
Radio Astronomy Observations and Technology
article

SPRITEly: Time-domain Millimeter Interferometry at the Owens Valley Radio Observatory

Vikram Ravi, Mark Hodges, James W. Lamb, Nitika Yadlapalli Yurk, D. P. Woody, R. W. Hobbs, A. C. S. Readhead
article en

Abstract

Abstract 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.

The Astronomical JournalVol. 168(4)
National Science Foundation
Openalex Percentile: Top 88%
Radio Astronomy Observations and Technology
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SPRITEly: Time-domain Millimeter Interferometry at the Owens Valley Radio Observatory — Vikram Ravi, Mark Hodges, et al. · The Astronomical Journal (2024) | TGRS Research Map | TGRS