most citedRCSEDv2: Open-source web tools for visualization of imaging and spectral data

1 citations · 1 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2021

Fast interactive web-based data visualizer of panoramic spectroscopic surveys

Ivan Katkov, Damir Gasymov, Joseph D. Gelfand +7

Panoramic IFU spectroscopy is a core tool of modern observational astronomy and is especially important for galaxy physics. Many massive IFU surveys, such as SDSS MaNGA (10k target…

astro-ph.IM2021

RCSEDv2: homogenization of multi-wavelength photometric data

Victoria Toptun, Igor Chilingarian, Ivan Katkov +6

RCSEDv2 (https://rcsed2.voxastro.org/), the second Reference Catalog of Spectral Energy Distributions of galaxies includes the largest homogeneously processed photometric dataset f…

astro-ph.IM20211 cited

RCSEDv2: Open-source web tools for visualization of imaging and spectral data

Vladislav Klochkov, Ivan Katkov, Igor Chilingarian +6

We present a set of open-source web tools for visualization of spectral and imaging data, which we use in the second Reference Catalogue of Spectral Energy Distributions of galaxie…

astro-ph.IM2021

RCSEDv2: the largest database of galaxy properties from a homogeneously processed multi-wavelength dataset

Igor Chilingarian, Sviatoslav Borisov, Vladimir Goradzhanov +6

The Reference Catalog of Spectral Energy Distributions of 800,000 galaxies (RCSED) includes the results of uniform re-processing of 800,000 SDSS DR7 galaxies at redshifts $0.007<z<…

astro-ph.IM2021

RCSEDv2: Processing and analysis of 4+ million galaxy spectra

Vladimir Goradzhanov, Igor Chilingarian, Evgenii Rubtsov +6

RCSEDv2 (https://rcsed2.voxastro.org/), the second Reference Catalog of Spectral Energy Distributions of galaxies, provides the largest homogeneously analyzed collection of optical…

astro-ph.IM2021

RCSEDv2: analytic approximations of k-corrections for galaxies out to redshift

Anastasia Kasparova, Igor Chilingarian, Sviatoslav Borisov +6

To compare photometric properties of galaxies at different redshifts, we need to correct fluxes for the change of effective rest-frame wavelengths of filter bandpasses, called -…