activity
20112026
most citedThe portrait of Malin 2: a case study of a giant low surface brightness galaxy

28 citations · 69 across the 29 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

16 papers · 1 filter

astro-ph.IM2026

The SDSS-V Local Volume Mapper (LVM): Technical Overview

Guillermo A. Blanc, Niv Drory, Sebastián F. Sánchez +59

The Sloan Digital Sky Survey V (SDSS-V) Local Volume Mapper (LVM) is an ultra-wide integral field spectroscopic survey of the Milky Way, the Magellanic Clouds, and a sample of gala…

astro-ph.IM2026

SDSS-V Local Volume Mapper (LVM): Dithered Data Cube Reconstruction with 3dcubegen

H. J. Ibarra-Medel, A. Z. Lugo-Aranda, R. de J. Zermeño +16

The Sloan Digital Sky Survey V (SDSS-V) Local Volume Mapper (LVM) is conducting an unprecedented wide-field integral field spectroscopic survey of the Milky Way, the Magellanic Clo…

astro-ph.IM2025★ 3 cited

Sloan Digital Sky Survey-V: Pioneering Panoptic Spectroscopy

Juna A. Kollmeier, Hans-Walter Rix, Conny Aerts +217

The Sloan Digital Sky Survey-V (SDSS-V) is pioneering panoptic spectroscopy: it is the first all-sky, multi-epoch, optical-to-infrared spectroscopic survey. SDSS-V is mapping the s…

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.IM2021★ 1 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 -…

astro-ph.IM2021

Hybrid minimization algorithm for computationally expensive multi-dimensional fitting

Evgenii Rubtsov, Igor Chilingarian, Ivan Katkov +3

Multi-dimensional optimization is widely used in virtually all areas of modern astrophysics. However, it is often too computationally expensive to evaluate a model on-the-fly. Typi…

astro-ph.IM2021

Multi-segment and Echelle stellar spectra processing issues and how to solve them

Sviatoslav Borisov, Igor Chilingarian, Evgenii Rubtsov +7

High-quality stellar spectra are in great demand now - they are the most important ingredient in the stellar population synthesis to study galaxies and star clusters. Here we descr…

astro-ph.IM2015

Stellar atmosphere interpolator for empirical and synthetic spectra

Nikolay Podorvanyuk, Igor Chilingarian, Ivan Katkov

We present a new stellar atmosphere interpolator which we will use to compute stellar population models based on empirical and/or synthetic spectra. We combined observed and synthe…

astro-ph.IM2013★ 5 cited

A new technique for the determination of the initial mass function in unresolved stellar populations

Nikolay Podorvanyuk, Igor Chilingarian, Ivan Katkov

We present a new technique for the determination of the low-mass slope (; ) of the present day stellar mass function (PDMF) using the pixel space fitting…

astro-ph.IM2013

The new technique for the determination of the stellar initial mass function of unresolved stellar populations

N. Podorvanyuk, I. Chilingarian, I. Katkov

We present the new technique for the determination of the low-mass slope of the stellar mass function from the pixel-space fitting of integrated light spectra. This technique is th…

astro-ph.IM2011★ 7 cited

NBursts+phot: parametric recovery of galaxy star formation histories from the simultaneous fitting of spectra and broad-band spectral energy distributions

Igor Chilingarian, Ivan Katkov

We present NBursts+phot, a novel technique for the parametric inversion of spectrophotometric data for unresolved stellar populations where high-resolution spectra and broadband SE…

astro-ph.IM2011★ 2 cited

Multi-component parametric inversion of galaxy kinematics and stellar populations using full spectral fitting

Ivan Yu. Katkov, Igor V. Chilingarian

The stellar line-of-sight velocity distribution (LOSVD) can be strongly asymmetric in regions where the light contributions of both disc and bulge in spiral and lenticular galaxies…