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

30 papers

astro-ph.GA2026

CoRGI in MaNGA - II. NGC 5717: cold-gas accretion and disk growth in a BGG

Damir Gasymov, Ivan Yu. Katkov, Eva K. Grebel +6

Large-scale stellar counter-rotation, in which two coplanar stellar components rotate in opposite directions, is usually interpreted as a signature of external gas accretion. Such…

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.GA2026

SDSS-V Local Volume Mapper (LVM): The Integrated Light and Internal Rotation of Omega Centauri

Maximilian Häberle, Dmitry Bizyaev, Alina Boecker +34

The SDSS-V Local Volume Mapper (LVM) is a wide-field integral field spectroscopic survey of the Southern Milky Way plane, the Magellanic Clouds, and nearby Local Group galaxies. We…

astro-ph.GA2026

The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper

SDSS Collaboration, Mojgan Aghakhanloo, David Aguilar +273

This paper presents the twentieth data release (DR20) from the Sloan Digital Sky Survey, the third data release of its fifth generation (SDSS-V). SDSS-V is a panoptic spectroscopy…

astro-ph.GA2026

There is no single density: star-forming regions and galaxies hold more dense ionized gas than long assumed

J. Eduardo Méndez-Delgado, Christophe Morisset, William J. Henney +29

Ionized gas fills star-forming regions and galaxies, and nearly everything we know about its temperature, pressure, mass, and composition is inferred from its emission lines [1-3].…

astro-ph.GA2025★ 2 cited

Optical Emission-Line Properties of eROSITA-selected SDSS-V Galaxies

Nadiia G. Pulatova, Evgenii Rubtsov, Igor V. Chilingarian +21

We present and discuss optical emission line properties obtained from the analysis of Sloan Digital Sky Survey (SDSS) spectra for an X-ray selected sample of 3684 galaxies (0.002 <…

astro-ph.HE2025

SDSS-V LVM: Collisionless Shocks in the Supernova Remnant RCW86

Sumit K. Sarbadhicary, Knox S. Long, John C. Raymond +19

The supernova remnant (SNR) RCW86 is among the few SNRs with Balmer-emission lines containing broad and narrow spectral components that trace fast, non-radiative shocks in partiall…

astro-ph.GA2025★ 8 cited

The Nineteenth Data Release of the Sloan Digital Sky Survey

SDSS Collaboration, Gautham Adamane Pallathadka, Mojgan Aghakhanloo +210

Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial…

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.HE2025

Peering into the heart of darkness with VLBA : Radio Quiet AGN in the JWST North Ecliptic Pole Time-Domain Field

Payaswini Saikia, Ramon Wrzosek, Joseph Gelfand +27

We present initial results from the 4.8 GHz Very Long Baseline Array (VLBA) survey of the JWST North Ecliptic Pole Time-Domain Field (TDF). From 106 radio sources found in the Karl…

astro-ph.GA2024

Optical spectroscopy of host-galaxies of intermediate mass black holes: evolution of central black holes

V. Goradzhanov, I. Chilingarian, M. Demianenko +6

Intermediate-mass black holes (IMBHs) with masses below () are pivotal in understanding the origin and growth mechanisms of supermassive black holes (SMBHs…

astro-ph.GA2022★ 5 cited

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

Abdurro'uf, Katherine Accetta, Conny Aerts +337

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete…

astro-ph.GA2022

Optical Variability of "Light-weight" Supermassive Black Holes at a Few Percent Level from ZTF Forced-Photometry Light Curves

Mariia Demianenko, Kirill Grishin, Victoria Toptun +4

Large time-domain surveys provide a unique opportunity to detect and explore variability of millions of sources on timescales from days to years. Broadband photometric variability…

astro-ph.GA2022★ 2 cited

Optical spectroscopic observations of intermediate-mass black holes and their host galaxies: the relation

Vladimir Goradzhanov, Igor Chilingaryan, Ivan Katkov +4

Intermediate-mass black holes (IMBHs; ) in galaxy centers are cruciel for painting a coherent picture of the formation and growth of supermassive black…

astro-ph.HE2022★ 4 cited

Confirmation of intermediate-mass black holes candidates with X-ray observations

Victoria Toptun, Igor Chilingarian, Kirill Grishin +5

The origin of supermassive black holes (SMBH) in galaxy centers still remains uncertain. There are two possible ways of their formation - from massive () and…

astro-ph.GA2021★ 2 cited

Optical light curves of light-weight supermassive black holes produced by the Zwicky Transient Facility Forced Photometry Service

Mariia Demianenko, Igor Chilingarian, Kirill Grishin +4

In this paper, we present an algorithm to correct optical light curves obtained using The Zwicky Transient Facility Forced Photometry Service and its application to the analysis of…

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…