Pith. sign in

REVIEW 1 cited by

From Data to Software to Science with the Rubin Observatory LSST

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2208.02781 v1 pith:PNY73L2N submitted 2022-08-04 astro-ph.IM

Katelyn Breivik , Andrew J. Connolly , K. E. Saavik Ford , Mario Jurić , Rachel Mandelbaum , Adam A. Miller , Dara Norman , Knut Olsen
show 92 more authors
William O'Mullane Adrian Price-Whelan Timothy Sacco J. L. Sokoloski Ashley Villar Viviana Acquaviva Tomas Ahumada Yusra AlSayyad Catarina S. Alves Igor Andreoni Timo Anguita Henry J. Best Federica B. Bianco Rosaria Bonito Andrew Bradshaw Colin J. Burke Andresa Rodrigues de Campos Matteo Cantiello Neven Caplar Colin Orion Chandler James Chan Luiz Nicolaci da Costa Shany Danieli James R. A. Davenport Giulio Fabbian Joshua Fagin Alexander Gagliano Christa Gall Nicolás Garavito Camargo Eric Gawiser Suvi Gezari Andreja Gomboc Alma X. Gonzalez-Morales Matthew J. Graham Julia Gschwend Leanne P. Guy Matthew J. Holman Henry H. Hsieh Markus Hundertmark Dragana Ilić Emille E. O. Ishida Tomislav Jurkić Arun Kannawadi Alekzander Kosakowski Andjelka B. Kovačević Jeremy Kubica François Lanusse Ilin Lazar W. Garrett Levine Xiaolong Li Jing Lu Gerardo Juan Manuel Luna Ashish A. Mahabal Alex I. Malz Yao-Yuan Mao Ilija Medan Joachim Moeyens Mladen Nikolić Robert Nikutta Matt O'Dowd Charlotte Olsen Sarah Pearson Ilhuiyolitzin Villicana Pedraza Mark Popinchalk Luka C. Popović Tyler A. Pritchard Bruno C. Quint Viktor Radović Fabio Ragosta Gabriele Riccio Alexander H. Riley Agata Rożek Paula Sánchez-Sáez Luis M. Sarro Clare Saunders {DJ}or{j̣e V. Savić Samuel Schmidt Adam Scott Raphael Shirley Hayden R. Smotherman Steven Stetzler Kate Storey-Fisher Rachel A. Street David E. Trilling Yiannis Tsapras Sabina Ustamujic Sjoert van Velzen José Antonio Vázquez-Mata Laura Venuti Samuel Wyatt Weixiang Yu Ann Zabludoff
This is my paper · ORCID
classification astro-ph.IM
keywords lsstsoftwaresciencescalablecollaborationobservatoryrubinservices
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) dataset will dramatically alter our understanding of the Universe, from the origins of the Solar System to the nature of dark matter and dark energy. Much of this research will depend on the existence of robust, tested, and scalable algorithms, software, and services. Identifying and developing such tools ahead of time has the potential to significantly accelerate the delivery of early science from LSST. Developing these collaboratively, and making them broadly available, can enable more inclusive and equitable collaboration on LSST science. To facilitate such opportunities, a community workshop entitled "From Data to Software to Science with the Rubin Observatory LSST" was organized by the LSST Interdisciplinary Network for Collaboration and Computing (LINCC) and partners, and held at the Flatiron Institute in New York, March 28-30th 2022. The workshop included over 50 in-person attendees invited from over 300 applications. It identified seven key software areas of need: (i) scalable cross-matching and distributed joining of catalogs, (ii) robust photometric redshift determination, (iii) software for determination of selection functions, (iv) frameworks for scalable time-series analyses, (v) services for image access and reprocessing at scale, (vi) object image access (cutouts) and analysis at scale, and (vii) scalable job execution systems. This white paper summarizes the discussions of this workshop. It considers the motivating science use cases, identified cross-cutting algorithms, software, and services, their high-level technical specifications, and the principles of inclusive collaborations needed to develop them. We provide it as a useful roadmap of needs, as well as to spur action and collaboration between groups and individuals looking to develop reusable software for early LSST science.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Searching for Nearby Diffuse Dwarf Galaxies in the COSMOS Field

    astro-ph.GA 2025-02 conditional novelty 4.0 of 10

    Three nearby low-surface-brightness dwarf galaxies, two of them ultra-diffuse galaxies, are identified in the COSMOS field and characterized with multiwavelength SED fitting.

Pith tools