activity
19982025
most citedThe Rotational Excitation Temperature of the 6614 Diffuse Interstellar Band Carrier

56 citations · 532 across the 35 of their papers we have counts for

collaborators

38 papers

astro-ph.IM2025★ 27 cited

DECH: Software Package for Astronomical Spectral Data Processing and Analysis

G. A. Galazutdinov

The article provides a brief description of the software package DECH for processing and analysis of astronomical spectra. DECH supports all stages of processing and analysis of sp…

astro-ph.GA2024★ 2 cited

On the intrinsic rest wavelengths of diffuse interstellar bands

G. A. Galazutdinov, E. Babina

The rest wavelengths of DIBs are of fundamental importance owing to the lack of unambiguous identification for these mysterious features. Usually the wavelengths of DIBs are estima…

astro-ph.GA2024★ 6 cited

Position displacement of diffuse interstellar bands

G. Galazutdinov, J. Krełowski, Y. Beletsky +1

We re-consider the already published phenomenon: the blue shift of diffuse interstellar bands, observed in spectra of HD34078 (AE Aur) and members of the Sco OB1 association, in pa…

astro-ph.SR2024★ 1 cited

Catalog of variable stars in the WD 0009+501 and GRW +708247 fields based on photometric survey data on transiting exoplanets

O. Ya. Yakovlev, A. F. Valeev, G. G. Valyavin +15

We present a catalog of 150 variable stars, including 13 stars with exoplanet candidates. 37 stars were identified as variables for the first time. As a result of a 2.5-year photom…

astro-ph.EP2023★ 8 cited

Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit

G. A. Galazutdinov, R. V. Baluev, G. Valyavin +16

We report an independent Doppler confirmation of the TESS planet candidate orbiting an F-type main sequence star TOI-1408 located 140 pc away. We present a set of radial velocities…

astro-ph.EP2023★ 5 cited

Eight exoplanet candidates in SAO survey

O. Ya. Yakovlev, A. F. Valeev, G. G. Valyavin +15

Here we present eight new candidates for exoplanets detected by the transit method at the Special Astrophysical Observatory of the Russian Academy of Sciences. Photometric observat…