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Environmental correction in supernovae standardization |
Anastasia Baluta (SAI MSU) |
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Pitfall of FFP parallax parameter accuracy between Euclid and Roman |
Makiko Ban (OAUW) |
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Enhancing Time-Domain Astronomy Through Joint Survey Processing |
Ranga Chary (Caltech/IPAC) |
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Classification conundrum in Gamma Ray Bursts: Signatures of collapsars in high redshift short GRBs |
Dimple Dimple (ARIES, India) |
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Finding Missing Supernovae with Roman |
Ori Fox (STScI) |
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Constraining the Size of the Torus of NGC 6418 |
Ashley Lynn Frank (RIT) |
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The Wide-Field Infrared Transient Explorer (WINTER) |
Danielle Frostig (MIT) |
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From short GRBs to neutron star natal kicks |
Nicola Gaspari (Radboud U.) |
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Search for merger ejecta emission in Short Gamma Ray Bursts from very late time radio observations |
Ankur Ghosh (SRF, ARIES) |
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Probing into emission mechanisms of GRB 190530A using time-resolved spectra and polarization studies: Synchrotron Origin? |
Rahul Gupta (Aryabhatta Res. Inst. Obs. Sci.) |
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Classifying Transients and Variable Objects with SCONE |
Erin Elizabeth Hayes (U. Pennsylvania) |
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The multiband evolution of novae |
Yael Hillman (Ariel U., Israel) |
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Millimeter to đ-Ray Variability of AGN found in the SPTpol 500 degree2 field |
John Calven Hood (Vanderbilt U.) |
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Parameterizing Type Ia Supernovae for Roman Space Telescope Cosmology |
Mitchell Karmen (LBNL) |
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FUV Variable Stars in M31 |
Denis Leahy (U. Calgary) |
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What can we learn about transients from 21 cm line emission in their environments? |
MichaĆ Jerzy MichaĆowski (AMU Poznan) |
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The Astronomical Event Observatory Network (AEON) and Time Domain Follow-up from the Ground and Space |
Bryan Miller (Gemini/NOIRLab) |
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The Transient UV Object (TUVO) Project |
David Modiano (U. Amsterdam) |
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The SALVATION Project: A Red Nova in M31 and Other Highlights |
Rafael Nunez (UCSC) |
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Primordial Black Hole Microlensing Predictions for Roman |
Kerianne Pruett (LLNL) |
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Novel polarimetric technique to constrain the magnetic field structure and strength of Gamma-ray burst jets |
Manisha Shrestha (Astr. Res. Lab, Liverpool) |
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PGIR 20eid (SN2020qmp): A Type IIP Supernova at 15.6 Mpc discovered by the Palomar Gattini-IR survey |
Gokul Prem Srinivasaragavan (U. Maryland) |
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Modeling the Diversity of Transient Light Curves through PCA (principal component analysis) |
Nao Suzuki (Kavli IPMU/U. Tokyo) |