Optimisation of the WEAVE target assignment algorithm

Ground-based and Airborne Instrumentation for Astronomy IX Proc. SPIE 12184 (2022) 121846J

Authors:

Sarah Hughes, Gavin Dalton, Daniel Smith, Kenneth Duncan, David Terrett, Don Carlos Abrams, J. Alfonso Aguerri, Marc Balcells, Georgia Bishop, Piercarlo Bonifacio, Esperansa Carrasco, Shoko Jin, Ian Lewis, Scott Trager, Antonella Vallenari

Abstract:

WEAVE is the new wide-field spectroscopic facility for the prime focus of the William Herschel Telescope in La Palma, Spain. Its fibre positioner is essential for the accurate placement of the spectrograph's ~960-fibre multiplex. To maximise the assignment of its optical fibres, WEAVE uses a simulated annealing algorithm called Configure, which allocates the fibres to targets in the field of view. We have conducted an analysis of the algorithm's behaviour using a subset of mid-tier WEAVE LOFAR fields, and adjusted the priority assignment algorithm to optimise the total fibres assigned per field, and the assignment of fibres to the higher priority science targets. The output distributions have been examined, to investigate the implications for the WEAVE science teams.

Results of the Gemini Deep Planet Survey -- Constraints on the Existence of Planets on Wide Orbits

Proceedings of the conference In the Spirit of Bernard Lyot, UCB

Authors:

D Lafreniere, R Doyon, C Marois, D Nadeau, BR Oppenheimer, PF Roche, F Rigaut

Silicon Monoxide in Supernova SN1987A

Proceedings of the 150th IAU Symposium

Authors:

PF Roche, CH Smith, DK Aitken

Spatially resolved observations of the unidentified dust features in BD +30°3639

IAU Symposium No. 131

Authors:

PF Roche, CH Smith, DK Aitken

Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). VI. Crowdsourced lens finding with Space Warps

Authors:

Alessandro Sonnenfeld, Aprajita Verma, Anupreeta More, Campbell Allen, Elisabeth Baeten, James HH Chan, Roger Hutchings, Anton T Jaelani, Chien-Hsiu Lee, Christine Macmillan, Philip J Marshall, James O' Donnell, Masamune Oguri, Cristian E Rusu, Marten Veldthuis, Kenneth C Wong, Claude Cornen, Christopher Davis, Adam McMaster, Laura Trouille, Chris Lintott, Grant Miller

Abstract:

Strong lenses are extremely useful probes of the distribution of matter on galaxy and cluster scales at cosmological distances, but are rare and difficult to find. The number of currently known lenses is on the order of 1,000. We wish to use crowdsourcing to carry out a lens search targeting massive galaxies selected from over 442 square degrees of photometric data from the Hyper Suprime-Cam (HSC) survey. We selected a sample of $\sim300,000$ galaxies with photometric redshifts in the range $0.2 < z_{phot} < 1.2$ and photometrically inferred stellar masses $\log{M_*} > 11.2$. We crowdsourced lens finding on this sample of galaxies on the Zooniverse platform, as part of the Space Warps project. The sample was complemented by a large set of simulated lenses and visually selected non-lenses, for training purposes. Nearly 6,000 citizen volunteers participated in the experiment. In parallel, we used YattaLens, an automated lens finding algorithm, to look for lenses in the same sample of galaxies. Based on a statistical analysis of classification data from the volunteers, we selected a sample of the most promising $\sim1,500$ candidates which we then visually inspected: half of them turned out to be possible (grade C) lenses or better. Including lenses found by YattaLens or serendipitously noticed in the discussion section of the Space Warps website, we were able to find 14 definite lenses, 129 probable lenses and 581 possible lenses. YattaLens found half the number of lenses discovered via crowdsourcing. Crowdsourcing is able to produce samples of lens candidates with high completeness and purity, compared to currently available automated algorithms. A hybrid approach, in which the visual inspection of samples of lens candidates pre-selected by discovery algorithms and/or coupled to machine learning is crowdsourced, will be a viable option for lens finding in the 2020s.