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20062026
most citedGalaxy and Mass Assembly (GAMA): survey diagnostics and core data release

1.1k citations · 20.7k across the 326 of their papers we have counts for

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21 papers · 1 filter

astro-ph.IM2026

SM-Net: Learning a Continuous Spectral Manifold from Multiple Stellar Libraries

Omar Anwar, Aaron S. G. Robotham, Luca Cortese +1

We present SM-Net, a machine-learning model that learns a continuous spectral manifold from multiple high-resolution stellar libraries. SM-Net generates stellar spectra directly fr…

astro-ph.IM2025★ 1 cited

SKYSURF. X. A Novel Method for Measuring Integrated Galaxy Light

Delondrae D. Carter, Timothy Carleton, Daniel J. Henningsen +19

We describe the drizzling pipeline and contents of the drizzled database for Hubble Space Telescope Cycle 27-29 Archival Legacy project "SKYSURF," the largest archival project ever…

astro-ph.IM2023

JWST's PEARLS: Improved Flux Calibration for NIRCam

Zhiyuan Ma, Haojing Yan, Bangzheng Sun +23

The Prime Extragalactic Areas for Reionization and Lensing Science (PEARLS), a JWST GTO program, obtained a set of unique NIRCam observations that have enabled us to significantly…

astro-ph.IM2023

ProPane: Image Warping with Fire

A. S. G. Robotham, R. Tobar, S. Bellstedt +7

In this paper we introduce the software package ProPane, written for the R data analysis language. ProPane combines the full range of wcslib projections with the C++ image manipula…

astro-ph.IM2023★ 1 cited

Dynamic Wisp Removal in JWST NIRCam Images

A. S. G. Robotham, J. C. J. D'Silva, R. A. Windhorst +5

The James Webb Space Telescope (JWST) near-infrared camera (NIRCam) has been found to exhibit serious wisp-like structures in four of its eight short-wavelength detectors. The exac…

astro-ph.IM2023★ 7 cited

Hydra II: Characterisation of Aegean, Caesar, ProFound, PyBDSF, and Selavy source finders

M. M. Boyce, A. M. Hopkins, S. Riggi +24

We present a comparison between the performance of a selection of source finders using a new software tool called Hydra. The companion paper, Paper~I, introduced the Hydra tool and…

astro-ph.IM2023★ 5 cited

Hydra I: An extensible multi-source-finder comparison and cataloguing tool

M. M. Boyce, A. M. Hopkins, S. Riggi +24

The latest generation of radio surveys are now producing sky survey images containing many millions of radio sources. In this context it is highly desirable to understand the perfo…

astro-ph.IM2022★ 11 cited

SKYSURF-4: Panchromatic HST All-Sky Surface-Brightness Measurement Methods and Results

Rosalia O'Brien, Timothy Carleton, Rogier A. Windhorst +22

The diffuse, unresolved sky provides most of the photons that the Hubble Space Telescope (HST) receives, yet remains poorly understood. HST Archival Legacy program SKYSURF aims to…

astro-ph.IM2020

Current and Next Generation Survey Filter Conversions with ProSpect

Aaron S. G. Robotham

In this work we compute a reasonably comprehensive set of tables for current and next generation survey facility filter conversions. Almost all useful transforms are included with…

astro-ph.IM2019★ 37 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.IM2019★ 8 cited

4MOST Survey Strategy Plan

G. Guiglion, C. Battistini, C. P. M. Bell +30

The current status of and motivation for the 4MOST Survey Strategy, as developed by the Consortium science team, are presented here. Key elements of the strategy are described, suc…

astro-ph.IM2019★ 7 cited

4MOST Scientific Operations

C. J. Walcher, M. Banerji, C. Battistini +65

The 4MOST instrument is a multi-object spectrograph that will address Galactic and extragalactic science cases simultaneously by observing targets from a large number of different…

astro-ph.IM2019★ 311 cited

4MOST: Project overview and information for the First Call for Proposals

R. S. de Jong, O. Agertz, A. Agudo Berbel +335

We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey facility under development for the four-metre-class Vis…

astro-ph.IM2019★ 39 cited

Climbing Halo Merger Trees with TreeFrog

Pascal J. Elahi, Rhys J. J. Poulton, Rodrigo J. Tobar +4

We present TreeFrog, a massively parallel halo merger tree builder that is capable comparing different halo catalogues and producing halo merger trees. The code is written in c++11…

astro-ph.IM2018★ 187 cited

ProFound: Source Extraction and Application to Modern Survey Data

A. S. G. Robotham, L. J. M. Davies, S. P. Driver +4

We introduce ProFound, a source finding and image analysis package. ProFound provides methods to detect sources in noisy images, generate segmentation maps identifying the pixels b…

astro-ph.IM2016★ 119 cited

ProFit: Bayesian Profile Fitting of Galaxy Images

A. S. G. Robotham, D. S. Taranu, R. Tobar +2

We present ProFit, a new code for Bayesian two-dimensional photometric galaxy profile modelling. ProFit consists of a low-level C++ library (libprofit), accessible via a command-li…

astro-ph.IM2016★ 7 cited

A concise overview of the Maunakea Spectroscopic Explorer

Alan W. McConnachie, Carine Babusiaux, Michael Balogh +19

This short document is intended as a companion and introduction to the Detailed Science Case (DSC) for the Maunakea Spectroscopic Explorer. It provides a concise summary of the ess…

astro-ph.IM2016★ 31 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe

Alan McConnachie, Carine Babusiaux, Michael Balogh +173

MSE is an 11.25m aperture observatory with a 1.5 square degree field of view that will be fully dedicated to multi-object spectroscopy. More than 3200 fibres will feed spectrograph…

astro-ph.IM2015★ 107 cited

Hyper-Fit: Fitting Linear Models to Multidimensional Data with Multivariate Gaussian Uncertainties

A. S. G. Robotham, D. Obreschkow

Astronomical data is often uncertain with errors that are heteroscedastic (different for each data point) and covariant between different dimensions. Assuming that a set of D-dimen…

astro-ph.IM2014★ 8 cited

4MOST - 4m Multi Object Spectroscopic Telescope

Eric Depagne, the 4MOST consortium

4MOST (4m Multi Object Spectroscopic Telescope) is a spectroscopic facility that will be installed on ESO's VISTA around 2020. The science rationale of this facility are to be foun…

astro-ph.IM2014★ 142 cited

Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors

I. K. Baldry, M. Alpaslan, A. E. Bauer +17

The Galaxy And Mass Assembly (GAMA) survey has obtained spectra of over 230000 targets using the Anglo-Australian Telescope. To homogenise the redshift measurements and improve the…