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Program

Abstracts for the talks are listed here.

Talks are allocated for 20 minute each, with 15 min for the presentation.

All times are listed local to Green Bank, WV in the Eastern Time Zone (EST).

Session 1: Compact objects and stars at the end of their lifetime Chair: Hendrik
Monday - May 19, 2025
11:00--11:05	Welcome and Introduction	Anna Kapinska, Tony Remijan
11:05--11:25	Looking for imprints of the explosion mechanism of thermonuclear supernovae in their remnants	Soham Mandal
11:25--11:45	An Extreme Scattering Event Towards PSR B2310+42	Jacob Turner
11:45--12:05	The largest* galactic transient search - with CHIME	Fengqiu Adam Dong
12:05--12:25	A New Mass Estimate for PSR J0348+0432	Alexander Saffer
12:25--12:45	Demographics of the Dynamic Radio Sky	Dillon Dong
12:45--13:15	Discussion: Session 1
13:15--15:15	Break
Keynote Talk Chair: David
15:15--16:45	Exploring a Black Hole Explorer - The Science and Technology of Millimeterwave Space/Ground VLBI	Dan Marrone

All times are listed local to Green Bank, WV in the Eastern Time Zone (EST).

Session 2: Protoplanetary disks, planetary objects and AGN Chair: Tao
Tuesday - May 20, 2025
11:00--11:20	Sulfur Chemistry as a Window into Planet Formation	Charles Law
11:20--11:40	The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Dust and Gas Disk Properties in the Ophiuchus Star-forming Region	Dary Ruiz
11:40--12:00	A Radio Recombination Line View of the Orion Proplyds	Ryan Boyden
12:00--12:20	Characterizing the Spectral Variability of the First Directly-Imaged Planetary-Mass Companion	Arthur Adams
12:20--12:40	Obscuration Variability in Nearby AGN	Núria Torres-Albà
12:40--13:15	Discussion: Session 2
13:15--15:00	Break
Session 3: Star Formation Chair: Dillon
15:00--15:20	Phosphorus Chemistry at the Earliest Stage of Low-mass Star Formation	Samantha Scibelli
15:20--15:40	THOR-GC: Characterizing the interstellar medium towards the Galactic Center	Michael Rugel
15:40--16:00	Molecular gas fraction and dynamical equilibrium pressure in local and nearby galaxies	Cosima Eibensteiner
16:00--16:20	Measuring Magnetic Field Strengths in Galactic Star Forming Regions via the Zeeman Effect	Tao-Chung Ching
16:20--17:00	Discussion: Session 3

Career Panel Chair: Alex
Wednesday - May 21, 2025
11:00--13:00	Career Panel (Ricardo Finger Camus, Dan Marrone, Stefanie Milam, Poonam Chandra)
13:00--15:00	Break
Session 4: Instrumentation, tools and techniques Chair: Michael
15:00--15:20	Room Temperature and Cryogenic Measurements of the 3D Printed Orthomode Transducer at Ka-Band	Priyanka Mondal
15:20--15:40	A quasi-linear Harmonic Balance model for studying the performance of 2SB millimeter and submillimeter wave SIS receivers	David Monasterio
15:40--16:00	Tropospheric Phase Correction Using Water Vapor Radiometers	Kyle Massingill
16:00--16:20	Accelerating the major loop and minor loop of radio interferometric imaging	Hendrik Müller
16:20--17:00	Discussion: Session 4

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Founded in 1956, the NSF NRAO provides state-of-the-art radio telescope facilities for use by the international scientific community. NSF NRAO telescopes are open to all astronomers regardless of institutional or national affiliation. Observing time on NSF NRAO telescopes is available on a competitive basis to qualified scientists after evaluation of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time. NSF NRAO also provides both formal and informal programs in education and public outreach for teachers, students, the general public, and the media.