Corpus ID: 45388149

The LSST Data Management System

@article{Juric2015TheLD,
  title={The LSST Data Management System},
  author={Mario Juri'c and J. Kantor and K. Lim and R. Lupton and G. Dubois-Felsmann and T. Jenness and T. Axelrod and J. Aleksic and R. Allsman and Y. AlSayyad and J. Alt and R. Armstrong and J. Basney and A. Becker and J. Becla and S. Bickerton and R. Biswas and J. Bosch and D. Boutigny and M. Kind and D. Ciardi and A. Connolly and S. Daniel and G. Daues and F. Economou and Hsin-Fang Chiang and A. Fausti and M. Fisher-Levine and D. M. Freemon and P. Gee and P. Gris and Fabio Hernandez and J. Hoblitt and vZeljko Ivezi'c and Fabrice Jammes and Darko Jevremovi'c and R. Jones and J. Kalmbach and V. Kasliwal and K. Krughoff and D. Lang and John C. Lurie and N. Lust and F. Mullally and L. MacArthur and Peter Melchior and Joachim Moeyens and D. Nidever and R. Owen and J. Parejko and J. Peterson and D. Petravick and Stephen Pietrowicz and P. Price and D. Reiss and R. Shaw and J. Sick and C. Slater and M. Strauss and I. Sullivan and J. Swinbank and S. V. Dyk and Veljko Vujvci'c and A. Withers and P. Yoachim and for the Supernova Cosmology Project},
  journal={arXiv: Instrumentation and Methods for Astrophysics},
  year={2015}
}
The Large Synoptic Survey Telescope (LSST) is a large-aperture, wide-field, ground-based survey system that will image the sky in six optical bands from 320 to 1050 nm, uniformly covering approximately $18,000$deg$^2$ of the sky over 800 times. The LSST is currently under construction on Cerro Pach\'on in Chile, and expected to enter operations in 2022. Once operational, the LSST will explore a wide range of astrophysical questions, from discovering "killer" asteroids to examining the nature of… Expand
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The overlap between the LSst science pipeline software and Astropy software is described and areas where the LSST software provides new functionality are investigated, including the possibilities of re-engineering the LS ST science pipelineSoftware to build upon Astropy, includingThe option of contributing affliated packages. Expand
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A number of astro-statistical challenges that need to be overcome to extract maximum information and science results from LSST dataset are discussed. Expand
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The design and implementation of the LSST Active Optics System as well as its calibration are described, which will correct in real time the system aberrations mostly introduced by gravity, temperature gradients and other system distortions. Expand
Active Optics System Software Architecture
The Large Synoptic Survey Telescope (LSST) is an 8-meter class wide-field telescope now under construction on Cerro Pachón, near La Serena, Chile. This ground-based telescope is designed to conduct aExpand
LSST active optics system software architecture
The Large Synoptic Survey Telescope (LSST) is an 8-meter class wide-field telescope now under construction on Cerro Pachon, near La Serena, Chile. This ground-based telescope is designed to conduct aExpand
Large Synoptic Survey Telescope Solar System Science Roadmap
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The LSST Solar System Science Collaboration has identified and prioritized key Solar System research areas for investigation with LSST in this roadmap and ranked science priorities highlighted in this living document will inform LSST survey cadence decisions and aid in identifying software tools and pipelines needed to be developed by the planetary community as added value products and resources. Expand
Monitoring LSST system performance during construction
TLDR
This paper describes the latest updates to the comprehensive tool set developed for evaluating the LSST system performance, and introduces an integrated-étendue-based metrics framework, useful for not just system verification, but also mitigation and optimization. Expand
Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
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This paper presents the second data release of the Hyper Suprime-Cam Subaru Strategic Program, a wide-field optical imaging survey on the 8.2 meter Subaru Telescope, including a major update to the processing pipeline, including improved sky subtraction, PSF modeling, object detection, and artifact rejection. Expand
Characterization of LSST CCDs using realistic images, before first light
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This work investigates CCD systematics using both simulations of charge transport as well as with a unique bench-top optical system matched to the LSST’s fast f/1.2 beam to correct for systematic biases imprinted during shift-and-stare CCD observation. Expand
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The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the solar system, exploring the transient optical sky, and mapping the Milky Way. Expand
The LSST Data Processing Software Stack: Summer 2015 Release
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The current status of the data processing software is presented, and how to obtain it is described, to help improve the quality of data releases from LSST. Expand
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A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade. The Large SynopticExpand
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The Dark Energy Survey (DES) collaboration will study cosmic acceleration with a 5000 deg2 griZY survey in the southern sky over 525 nights from 2011-2016. The DES data management (DESDM) system willExpand
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We present the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS) that accurately determines a weak gravitational lensing signal from the full 154 deg^2 of deep multicolour data obtained by theExpand
Simulation of Astronomical Images from Optical Survey Telescopes using a Comprehensive Photon Monte Carlo Approach
We present a comprehensive methodology for the simulation of astronomical images from optical survey telescopes. We use a photon Monte Carlo approach to construct images by sampling photons fromExpand
Bayesian galaxy shape measurement for weak lensing surveys – III. Application to the Canada–France–Hawaii Telescope Lensing Survey
A likelihood-based method for measuring weak gravitational lensing shear in deep galaxy surveys is described and applied to the Canada–France–Hawaii Telescope (CFHT) Lensing Survey (CFHTLenS).Expand
2013a, Level 2 Photometric Calibration for the LSST Survey
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