activity
20102026
most citedThe virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B

57 citations · 109 across the 12 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.IM2024★ 6 cited

DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration

Benjamin M. Boyd, Gautham Narayan, Kaisey S. Mandel +17

We use hierarchical Bayesian modelling to calibrate a network of 32 all-sky faint DA white dwarf (DA WD) spectrophotometric standards () alongside three CALSPEC st…

astro-ph.IM2024

Faint white dwarf flux standards: data and models

Ralph C. Bohlin, Susana Deustua, Gautham Narayan +7

Fainter standard stars are essential for the calibration of larger telescopes. This work adds to the CALSPEC (calibration spectra) database 19 faint white dwarfs (WDs) with all-sky…

astro-ph.SR2024★ 3 cited

Revealing the elusive companion of the red giant binary 2MASSJ05215658+4359220 from UV HST and Astrosat-UVIT data

Luciana Bianchi, John Hutchings, Ralph Bohlin +2

Black hole demographics in different environments is critical in view of recent results on massive-stars binarity, and of the multi-messenger detectability of compact objects merge…

astro-ph.IM2024

The James Webb Space Telescope Absolute Flux Calibration. II. Mid-Infrared Instrument Imaging and Coronagraphy

Karl D. Gordon, G. C. Sloan, Macarena Garcia Marin +11

The absolute flux calibration of the Mid-Infrared Instrument Imaging and Coronagraphy is based on observations of multiple stars taken during the first 2.5 years of JWST operations…

astro-ph.SR2024

The updated BOSZ synthetic stellar spectral library

Szabolcs Mészáros, Ralph Bohlin, Carlos Allende Prieto +9

Context. The modeling of stellar spectra of flux standards observed by the Hubble and James Webb space telescopes requires a large synthetic spectral library that covers a wide atm…

astro-ph.GA2024

Expanded Sample of Small Magellanic Cloud Ultraviolet Dust Extinction Curves: Correlations between the 2175 A bump, q_pah, UV extinction shape, and N(HI)/A(V)

Karl D. Gordon, E. L. Fitzpatrick, Derck Massa +7

The Small Magellanic Cloud (SMC) shows a large variation in ultraviolet (UV) dust extinction curves, ranging from Milky Way-like (MW) to significantly steeper curves with no detect…