activity
20182026
most citedA giant shell of ionized gas discovered near M82 with the Dragonfly Spectral Line Mapper pathfinder

21 citations · 40 across the 14 of their papers we have counts for

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10 papers · 1 filter

astro-ph.IM2026

dfcosmic: A Python package for cosmic ray removal

Carter Lee Rhea, Pieter van Dokkum, Steven R. Janssens +5

Astronomical images often show sharp features that are caused by cosmic ray (CR) hits, hot pixels, or non-Gaussian noise. L.A.Cosmic (van Dokkum 2001) is a widely used edge detecti…

astro-ph.IM2025

dfreproject: A Python package for astronomical reprojection

Carter Lee Rhea, Pieter Van Dokkum, Steven R. Janssens +5

Deep astronomical images are often constructed by digitially stacking many individual sub-exposures. Each sub-exposure is expected to show small differences in the positions of sta…

astro-ph.IM2024

Realizing the potential of the Dragonfly Spectral Line Mapper: Calibration methods and on-sky performance

Deborah M. Lokhorst, Seery Chen, Imad Pasha +8

The Dragonfly Spectral Line Mapper is an innovative all-refracting telescope designed to carry out ultra-low surface brightness wide-field mapping of visible wavelength line emissi…

astro-ph.IM2024

Software infrastructure for the highly-distributed semi-autonomous Dragonfly Spectral Line Mapper

Imad Pasha, Seery Chen, Deborah Lokhorst +6

The Dragonfly Spectral Line Mapper (DSLM) is a semi-autonomous, distributed-aperture based telescope design, featuring a modular setup of 120 Canon telephoto lenses, and equal numb…

astro-ph.IM2024

The Dragonfly Spectral Line Mapper: Completion of the 120-lens array

Seery Chen, Deborah M. Lokhorst, Imad Pasha +7

The Dragonfly Spectral Line Mapper is a mosaic telescope comprising 120 Canon telephoto lenses, based on the design of the Dragonfly Telephoto Array. With a wide field of view, and…

astro-ph.IM202311 cited

A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images

Qing Liu, Roberto G. Abraham, Peter G. Martin +9

Unbiased sky background modeling is crucial for the analysis of deep wide-field images, but it remains a major challenge in low surface brightness astronomy. Traditional image proc…