collaborators

18 papers

math.NA2026

Identifying changing partial differential equations using Sampled Local WeakIdent

Wenbo Hao, Mengyi Tang, Sung Ha Kang

We propose Sampled Local WeakIdent (SLW-Ident), a framework for identifying changing governing equations from a single set of given data. Different from a typical approach of using…

astro-ph.IM2026

Wavelength Calibration Accuracy Across the STIS CCD: Pipeline Update and User Guidance

Matilde Mingozzi, Robert Jedrzejewski, Matthew Siebert +3

We investigate the wavelength calibration accuracy of STIS CCD spectra as a function of detector position, focusing on the E1/E2 pseudo-apertures. Comparison between measured lamp…

astro-ph.IM2026

CCD Rotation Rates From Regular Dispersion Solution Monitoring

Matilde Mingozzi, Matthew Siebert

It has been previously studied that the STIS CCD exhibits a slow rotation, evident from changes in spectral traces and flat-field evolution. In this Instrument Science Report, we p…

astro-ph.IM2026

Astronomical Advantages of a Boost Mission to Facilitate HST Science into the 2030s: Imaging the Circumgalactic Medium of Galaxies

Matthew J. Hayes, Kate H. R. Rubin, Michelle A. Berg +20

We present the case for imaging ultraviolet line emission from highly ionized metals and HI Lya in the circumgalactic medium of galaxies, should the Hubble Space Telescope receive…

astro-ph.GA2026

High-S/N Quasar Observations with HST/COS: Deep Fields for Spectroscopy

Andrew J. Fox, Jerry Kriss, Philipp Richter +49

Hubble is still in prime observing condition for making transformative discoveries in UV astronomy. In this white paper we describe the science case for a deep (S/N>30) UV spectros…

astro-ph.GA2026

The First Empirical Calibration of the MIR Abundance Diagnostic Ne with JWST

Noah S. J. Rogers, Evan D. Skillman, Danielle A. Berg +10

Large surveys of galaxies in the local and high-redshift Universe have, traditionally, relied on the intensity of rest-optical emission lines from metal ions in the Interstellar Me…