activity
20212026
most citedThe Nineteenth Data Release of the Sloan Digital Sky Survey

8 citations · 23 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2026

Giant Low-Surface Brightness Galaxies in the Global Picture of Galaxy Formation and Evolution

Fedor M. Kolganov, Igor V. Chilingarian, Anna S. Saburova +5

Giant low-surface brightness galaxies (gLSBGs) challenge standard merger-driven galaxy assembly models due to their large, dynamically cold disks, with radii often larger than 100~…

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.IM2026

Website with interactive visualization of multivariate astronomical time series

M. Volkov, M. Demianenko, D. Matveev +2

Light curves represent astronomical time series of flux measured across one or more photometric bands. With the rapid growth of large-scale sky surveys, time-domain astronomy has b…

astro-ph.GA2025★ 1 cited

MUSE Study of Two Giant Low-surface-brightness Galaxies with Compact Satellites

Anna S. Saburova, Damir Gasymov, Ivan S. Gerasimov +7

Giant low-surface-brightness disk galaxies (gLSBGs) are rare objects with disk radii up-to 160 kpc and dynamical masses of an order of up to 10 . Their very exist…

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.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.GA2025

Broad line region echo from highly accreting intermediate-mass black hole candidate SDSS J144850.08+160803.1. The first probe of intra-night variability and reverberation mapping

Mariia Demianenko, Anton Afanasiev, Evgenii Rubtsov +8

Elusive intermediate-mass black holes (IMBHs) can be used as ``time-squeezing'' machines, enabling studies of AGN geometry via reverberation mapping on much shorter timescales than…

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.IM2024★ 1 cited

What is the Role of Large Language Models in the Evolution of Astronomy Research?

Morgan Fouesneau, Ivelina G. Momcheva, Urmila Chadayammuri +10

ChatGPT and other state-of-the-art large language models (LLMs) are rapidly transforming multiple fields, offering powerful tools for a wide range of applications. These models, co…

astro-ph.GA2024

A closer look at the extended edge-on low-surface brightness galaxies

Anna S. Saburova, Damir Gasymov, Evgenii V. Rubtsov +13

To understand the origin of extended disks of low-surface brightness (LSB) galaxies, we studied in detail 4 such systems with large disks seen edge-on. Two of them are edge-on gian…

astro-ph.GA2024

What excites the optical emission in X-ray-selected galaxies?

N. G. Pulatova, H. -W. Rix, A. V. Tugay +3

We present a study of galaxies at with detected nuclear X-ray emission and optical emission line diagnostics in the Baldwin-Phillips-Terlevich (BPT) diagram. This s…

astro-ph.IM2024

PSF quality metrics in the problem of revealing Intermediate-Mass Black Holes using MICADO@ELT

Mariia Demianenko, Joerg-Uwe Pott, Kai Polsterer

Nowadays, astronomers perform point spread function (PSF) fitting for most types of observational data. Interpolation of the PSF is often an intermediate step in such algorithms. I…

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…