FRELLED: A realtime volumetric data viewer for astronomers

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00465536" target="_blank" >RIV/67985815:_____/15:00465536 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1016/j.ascom.2015.10.002" target="_blank" >http://dx.doi.org/10.1016/j.ascom.2015.10.002</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.ascom.2015.10.002" target="_blank" >10.1016/j.ascom.2015.10.002</a>

Jazyk výsledku

angličtina

Název v původním jazyce

FRELLED: A realtime volumetric data viewer for astronomers

Popis výsledku v původním jazyce

The author presents a new FITS viewer designed to explore 3D spectral line data (in particular H I) and assist with visual source extraction and analysis. Using the artistic software Blender, FRELLED can visualize even large (similar to 600(3) voxels) data sets at high frame rates (greater than or similar to 10 f.p.s.) in 3D. Blender's interface enables easy navigation within the 3D environment, and the FRELLED scripts support world coordinate systems. A variety of tools are included to aid source extraction and analysis, including interactively masking data (using 3D polyhedra of arbitrary complexity), querying NED, calculating the flux in specified volumes, generating contour plots and overlaying optical data. It includes tools to overlay n-body particle data, and multi-volume rendering is supported. The interface is designed to make cataloguing sources as easy as possible and I show that this can be as much as a factor of 50 times faster than using other viewers

Název v anglickém jazyce

FRELLED: A realtime volumetric data viewer for astronomers

Popis výsledku anglicky

The author presents a new FITS viewer designed to explore 3D spectral line data (in particular H I) and assist with visual source extraction and analysis. Using the artistic software Blender, FRELLED can visualize even large (similar to 600(3) voxels) data sets at high frame rates (greater than or similar to 10 f.p.s.) in 3D. Blender's interface enables easy navigation within the 3D environment, and the FRELLED scripts support world coordinate systems. A variety of tools are included to aid source extraction and analysis, including interactively masking data (using 3D polyhedra of arbitrary complexity), querying NED, calculating the flux in specified volumes, generating contour plots and overlaying optical data. It includes tools to overlay n-body particle data, and multi-volume rendering is supported. The interface is designed to make cataloguing sources as easy as possible and I show that this can be as much as a factor of 50 times faster than using other viewers

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

—

Projekt

<a href="/cs/project/GAP209%2F12%2F1795" target="_blank" >GAP209/12/1795: Tvorba hvězd aktivovaná expandujícími obálkami</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Astronomy and Computing

ISSN

2213-1337

e-ISSN

—

Svazek periodika

13

Číslo periodika v rámci svazku

November

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

13

Strana od-do

67-79

Kód UT WoS článku

000370460200006

EID výsledku v databázi Scopus

2-s2.0-84945589441