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Data Management Software

SAS data management solutions allow you to take your AI ambitions to the next level with seamless data connectivity, enhanced transformations and robust governance, enabling you to build, manage an...

‘SAS 데이터플럭스 ESP’ 솔루션 국내 출시 - BI KOREA

SAS코리아(대표 조성식)는 대량의 스트리밍 데이터를 즉각적으로 분석, 실시간 의사결정을 지원하는 ‘SAS 데이터플럭스 이벤트 스트림 프로세싱 엔진(SAS Data Flux Event Stream Processing Engine, 이하...

P-20 Data Systems

SAS provides software and services to create a robust and modernized Statewide Longitudinal Data System (SLDS) helping education leaders move from assumption-based decisions to data driven, analyti...

The SAS: A collection of substation diagrams | Edvard Csanyi님이 토픽에 대해 올림

관련성이 더 높은 업데이트 ; The Brain of a Gas-Insulated Switchgear (GIS): The Bay Local Control Cabinet (LCC) | EEP ; Automatic transfer switch between three power sources (analysis of schemes) | EEP ; Eight substation equipment needed to power up data center | EEP

HDD specs: Assess SATA vs SAS, sustained data rates and block size

In part two of a two-part series, we look at sustained data rates in hard disk drive (HDD) specs, SATA versus SAS, drive security, and how HDD makers pack density into products by shingling.

Available spectroscopic data - SDSS-III

SAS location, CAS table, Description ; plates-dr9.fits (3.7 Mb) (in SPECTRO_REDUX ; see datamodel ), plateX, List of all DR9 plates (available as Yanny file too) ; specObj-dr9.fits (2.9 Gb) (in SPECTRO_REDUX ;(see datamodel ), specObj (only primaries), Redshifts and classifications of all SDSS spectra (also available in BOSS-only and SDSS-only versions) ; ssppOut-dr9.fits (1.8 Gb) (in SSPP_REDUX ; see datamodel ), sppParams, Stellar parameters from SSPP ; ssppOut-dr9.lineindex.fits (2.3 Gb) (in SSPP_REDUX ; see datamodel ), sppLines, Stellar line indices from SSPP ; photoPlate-dr9.fits (7.9 Gb) (in SPECTRO_REDUX ; see datamodel ), join on photoObj, Photometric flux-based matches ; photoPosPlate-dr9.fits (7.5 Gb) (in SPECTRO_REDUX ; see datamodel ), join on photoObj, Photometric position-based matches ; photoMatchPlate-dr9.fits (370 Mb) (in SPECTRO_REDUX ; see datamodel ), , details of match results ; galSpecInfo-dr9.fits (364 Mb) (in SPECTRO_REDUX ; see datamodel ), galSpecInfo, Information for each galaxy processed by Garching group ; galSpecIndx-dr9.fits (1.9 Gb) (in SPECTRO_REDUX ; see datamodel ), galSpecIndx, Index measurements for each galaxy ; galSpecLine-dr9.fits (1.7 Gb) (in SPECTRO_REDUX ; see datamodel ), galSpecLine, Line measurements for each galaxy ; galSpecExtra-dr9.fits (339 Mb) (in SPECTRO_REDUX ; see datamodel ), galSpecExtra, Extra physical parameters for each galaxy ; SAS location, CAS table, Description ; spPlate-PLATE-MJD.fits (in SPECTRO_REDUX/[RUN2D]/[PLATE]; see datamodel ), , Coadded spectra grouped by plate ; spec-PLATE-MJD-FIBER.fits (in BOSS_SPECTRO_REDUX/[RUN2D]/spectra/[PLATE]; see datamodel ), , Individual spectra, one file per PLATE-MJD-FIBER ; spec-image-PLATE-MJD-FIBER.png (in SPECTRO_REDUX/images/[RUN2D]/[PLATE]), specObjAll, PNG images of each spectrum

HEASARC: XMM-Newton Data Analysis

THE XMM-NEWTON ABC GUIDE, STREAMLINED · EPIC (IMAGING mode), SAS Command Line ; Prepare the Data · Reprocess the Data · Apply Standard Filters · Make a Light Curve · Apply Time Filters · Making an Image and Source Detection · Make an Exposure Map · Extract the Source and Background Spectra · Check for Pile Up · My Observation is Piled Up! Now What? · Determine the Spectrum Extraction Areas · Create the Photon Redistribution Matrix (RMF) and Ancillary File (ARF)

Sas Jobs In Gurgaon - 2442 Sas Job Vacancies In Gurgaon - Naukri.com

MNC IT Consulting Firm · Posted by Metaphor Infotech ; 5-10 Yrs · 20-27.5 Lacs PA · Pune, Gurugram, Bengaluru

Available Spectroscopic Data - SDSS-III

SAS location, CAS table, Description ; (in SPECTRO_REDUX ; see datamodel ), plateX, List of all DR10 plates (available as Yanny file too) ; specObj-dr10.fits (2.9 Gb), specObj (only primaries), Redshifts and classifications of all SDSS spectra (also available in BOSS-only and SDSS-only versions) ; ssppOut-dr10.fits (1.8 Gb), sppParams, Stellar parameters from SSPP ; ssppOut-dr10.lineindex.fits (2.3 Gb), sppLines, Stellar line indices from SSPP ; photoPlate-dr10.fits (7.9 Gb), join on photoObj, Photometric flux-based matches ; photoPosPlate-dr10.fits (7.5 Gb), join on photoObj, Photometric position-based matches ; photoMatchPlate-dr10.fits (370 Mb), , details of match results ; galSpecInfo-dr8.fits (364 Mb), galSpecInfo, Information for each galaxy processed by Garching group ( deprecated in DR10 ) ; galSpecIndx-dr8.fits (1.9 Gb), galSpecIndx, Index measurements for each galaxy ( deprecated in DR10 ) ; galSpecLine-dr8.fits (1.7 Gb), galSpecLine, Line measurements for each galaxy ( deprecated in DR10 ) ; galSpecExtra-dr8.fits (339 Mb), galSpecExtra, Extra physical parameters for each galaxy ( deprecated in DR10 ) ; SAS location, CAS table, Description ; (in SPECTRO_REDUX/[RUN2D]/[PLATE];, , Coadded spectra grouped by plate ; (in BOSS_SPECTRO_REDUX/[RUN2D]/spectra/[PLATE];, , Individual spectra, one file per PLATE-MJD-FIBER ; (in SPECTRO_REDUX/images/[RUN2D]/[PLATE]), specObjAll, PNG images of each spectrum

SAS Visual Statistics Software

With SAS Visual Statistics, multiple users can explore data, then interactively create and refine predictive models. Uncover opportunities faster than your competitors. Put better models into action faster. Boost analytical productivity. Gain the freedom to experiment.

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