Non-detections of expected third flares in TDE 2022dbl and TDE 2020vdq support rpTDE interpretation over independent events, with modeling favoring bound main-sequence star orbits and deep initial encounters.
and Corbett, Hank and Galliher, Nathan W
9 Pith papers cite this work, alongside 38 external citations. Polarity classification is still indexing.
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ORACLE-2 multimodal classifiers raise macro F1 from 0.52-0.66 (light-curve only) to 0.73 on ZTF Bright Transient Survey data and reach 0.88 on simulated ELAsTiCC data.
GOATS integrates ANTARES, Gemini triggering, archive access, DRAGONS, and Astro Data Lab into one platform for LSST alert follow-up, demonstrated by triggering observations and classifying supernovae within minutes of detection.
Modeling indicates arrays of small seeing-limited telescopes are more cost-effective than single large seeing-limited ones for single-object observations, with single diffraction-limited telescopes preferred only below 20-28 magnitudes depending on architecture.
No kilonova detected from sub-solar GW candidate S251112cm, but coincident IIb supernova SN 2025adtq yields suggestive evidence for the superkilonova channel, though inconclusive after accounting for chance coincidence.
CASM-256 is a new 256-antenna radio array at Owens Valley that uses real-time digital beamforming to search for fast radio bursts and galactic transients over a huge sky area.
Simulations predict Argus and DSA will serendipitously catch GRB afterglows at rates of ~47/yr (Argus, reliable-fade metric) and ~82/yr (DSA) for Fermi/GBM LGRBs, with ~116 optical and ~217 radio orphan afterglows per year.
Lazuli is proposed as a space observatory combining flagship sensitivity with response times one to two orders of magnitude faster than current large facilities to enable new time-domain and multi-messenger science.
TESS and ZTF observations of 12 LFBOTs yield no late-time flares after SSO attribution, constraining central engine lifetimes to hundreds of days or less.
citing papers explorer
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A Disappearing Act: Constraints From "Missing" Flares of Repeating Partial TDE Candidates
Non-detections of expected third flares in TDE 2022dbl and TDE 2020vdq support rpTDE interpretation over independent events, with modeling favoring bound main-sequence star orbits and deep initial encounters.
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Leveraging Multimodality for Real-Time Classification of Transients and Variables found by the Zwicky Transient Facility
ORACLE-2 multimodal classifiers raise macro F1 from 0.52-0.66 (light-curve only) to 0.73 on ZTF Bright Transient Survey data and reach 0.88 on simulated ELAsTiCC data.
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GOATS: The next generation software infrastructure for time-domain astronomy at Gemini/NOIRLab. Application to alerts from Vera C. Rubin Observatory's Legacy Survey of Space and Time
GOATS integrates ANTARES, Gemini triggering, archive access, DRAGONS, and Astro Data Lab into one platform for LSST alert follow-up, demonstrated by triggering observations and classifying supernovae within minutes of detection.
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Single object observations: Large telescopes vs. multiple small telescopes
Modeling indicates arrays of small seeing-limited telescopes are more cost-effective than single large seeing-limited ones for single-object observations, with single diffraction-limited telescopes preferred only below 20-28 magnitudes depending on architecture.
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Electromagnetic Follow-up of the Sub-Solar Mass Gravitational Wave Candidate S251112cm: Kilonova Constraints and a Coincident IIb Supernova
No kilonova detected from sub-solar GW candidate S251112cm, but coincident IIb supernova SN 2025adtq yields suggestive evidence for the superkilonova channel, though inconclusive after accounting for chance coincidence.
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The 256-antenna Coherent All-Sky Monitor
CASM-256 is a new 256-antenna radio array at Owens Valley that uses real-time digital beamforming to search for fast radio bursts and galactic transients over a huge sky area.
-
Prospects for GRB Afterglow Discovery with the Eric and Wendy Schmidt Observatory System
Simulations predict Argus and DSA will serendipitously catch GRB afterglows at rates of ~47/yr (Argus, reliable-fade metric) and ~82/yr (DSA) for Fermi/GBM LGRBs, with ~116 optical and ~217 radio orphan afterglows per year.
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The Lazuli Space Observatory: Opportunities for time-domain and multi-messenger astronomy
Lazuli is proposed as a space observatory combining flagship sensitivity with response times one to two orders of magnitude faster than current large facilities to enable new time-domain and multi-messenger science.
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Constraints on Late-Time Flaring from Luminous Fast Blue Optical Transients using the Transiting Exoplanet Survey Satellite and the Zwicky Transient Facility
TESS and ZTF observations of 12 LFBOTs yield no late-time flares after SSO attribution, constraining central engine lifetimes to hundreds of days or less.