activity
19972026
most citedQuantitative Spectroscopy of O Stars at Low Metallicity. O Dwarfs in NGC 346

311 citations · 2k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.SR2026

Carbon in J0815+4729: Casting a shadow of doubt on the interpretation of CH absorption in the most primitive stars

Junbo Zhang, Carlos Allende Prieto, Yeisson Osorio +7

Aims. We revisit the carbon abundance in the primitive iron-poor star J0815+4729 ([Fe/H] = -5.49). J0815+4729 is so carbon-enhanced and oxygen-rich that, in addition to CH and C2 m…

astro-ph.SR2026

WISE J005128.08+645651.7: An enigmatic R Coronae Borealis star

J. Budaj, K. Bernhard, I. Hubeny

Context. R Coronae Borealis (RCB) stars are hydrogen-deficient and carbon-rich (HdC) supergiants that likely originate from a merger of two white dwarfs. As such they are not expec…

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

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.SR2017★ 99 cited

Effective Temperatures of Cataclysmic Variable White Dwarfs as a Probe of their Evolution

A. F. Pala, B. T. Gänsicke, D. Townsley +29

We present HST spectroscopy for 45 cataclysmic variables (CVs), observed with HST/COS and HST/STIS. For 36 CVs, the white dwarf is recognisable through its broad Ly absorption p…