SDSS optical cable and

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The SDSS-V local volume mapper fibre cable assembly and metrology

The fibre cable spans approximately 20 meters from the telescope platform to the spectrograph slits. A sorting hat, located in the spectrograph room, redistributes the 1944 fibres into three 648–element

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The SDSS-V local volume mapper fibre cable assembly and metrology

Request PDF | On Oct 7, 2022, Tobias Feger and others published The SDSS-V local volume mapper fibre cable assembly and metrology | Find, read and cite all the research you need on ResearchGate

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DR18 Open Fiber Programs

The SDSS-V focal plane fiber-positioning hardware and survey strategy were designed around the core science cases, whose target densities — and relative infrared vs optical needs — vary dramatically

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The SDSS-V Local Volume Mapper fiber cable system

Each spectrograph will be fed by 648 fibers, which are reformatted into a linear array, forming the entrance slit. In this paper, we present the opto-mechanical design of the LVM-LCO fiber cable system.

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c089_ANSI

Optical Fiber consists of a thin glass filament in a polymer coating. The polymer coating has a thin outer coating of various colored inks. Glass is a solid material produced by combining various raw

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SDSS-V fiber optic throughput performance evaluation in multi-fiber

In this paper we describe the original SDSS spectrograph design and the upgrades implemented for BOSS, and document the predicted and measured performances.

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The SDSS Instruments

The SDSS Instruments The SDSS Instruments The SDSS survey collects data with modern, digital detectors. An enormous array of CCD detectors takes images, and a pair of spectrographs, fed by

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Understanding SDSS spectroscopic data

Understanding SDSS spectroscopic data In SDSS, spectra for many objects are taken simultaneously. This is possible because the spectrographs are connected

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Understanding the Optical Data | SDSS

In SDSS, spectra for many objects are taken simultaneously. This is possible because the spectrographs are connected by fiber optic cables to an aluminum plate in the telescope''s focal

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The SDSS-V local volume mapper fibre cable assembly and metrology

The Sloan Digital Sky Survey V (SDSS–V) is an all-sky spectroscopic survey of <6 million objects, designed to decode the history of the Milky Way, reveal the inner workings of stars, investigate the

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The SDSS-V local volume mapper fibre cable assembly and metrology

Over a series of discrete filter bands, from 0.4 to 21 microns, J-Black optical and infrared reflectivity performance is compared with other available coatings. Measured total reflectance values...

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Optical Spectra Overview | SDSS

Optical Spectra Overview Single-fiber Optical Spectra Data Release 16 includes the complete dataset of optical single-fibre spectroscopy of the Sloan Digital Sky Survey through February 2019. These data

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SDSS-V fiber optic throughput performance evaluation in multi-fiber

Download Citation | On Aug 29, 2022, Emily Farr and others published SDSS-V fiber optic throughput performance evaluation in multi-fiber termination connectors | Find, read and cite all the

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SDSS Plates – Voyages

SDSS is a multi-object spectroscopic survey, meaning that it can analyze the light of multiple objects simultaneously using its spectrographs. To do that, light from

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The SDSS-V local volume mapper fiber cable system

In this paper, we present the opto-mechanical design of the LVM-LCO fiber cable system. Dive into the research topics of ''The SDSS-V local volume mapper fiber cable system''. Together they form a

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spectrograph parameters

Optical fibers plugged into the holes in the plate carry light from the focal plane to slitheads attached to the cartridge. Each of the two slitheads accept light from

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The SDSS-V local volume mapper fiber cable assembly and

Abstract The Local Volume Mapper (LVM) is a small-telescope facility designed to provide a contiguous 2500 sq degree optical integral-field survey at Las Campanas Observatory (LCO) in Chile. The

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c302_ANSI

Optical fiber consists of a thin glass filament in a polymer coating. Glass is a solid material produced by combining various raw materials (e.g. oxides, carbonates, etc.), melting these components together,

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The SDSS-V local volume mapper fiber cable system

The Sloan Digital Sky Survey V (SDSS-V) is an all-sky spectroscopic survey of >6 million objects, designed to decode the history of the Milky Way, reveal the inner workings of stars, investigate the

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Introduction to SDSS

SDSS I-IV used a fiber plug-plate system for spectroscopic observations. This system consisted of aluminum plates with pre-drilled holes at specific on-sky positions for a pre-selected hour angle.

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Camera | SDSS

The imaging camera collects photometric imaging data using an array of 30 SITe/Tektronix 2048 by 2048 pixel CCDs arranged in six columns of five CCDs

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Focal Plane Systems

To meet SDSS-V''s requirements of rapid cadence and high target densities, we have replaced the iconic SDSS fiber plug-plates with robotic Focal Plane Systems (FPS).

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The Optical Spectroscopy Pipeline | SDSS

Starting with DR13, all SDSS data releases contain both BOSS and eBOSS spectra reprocessed using the latest version of the reduction pipeline. The reprocessing consists of raw CCD count extraction,

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DR16 Optical Spectra Overview | SDSS

SDSS optical spectra, both galactic and extra-galactic, are organized into a number of component surveys. The information boxes below describe the surveys that

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Optical Communication Insights