Tracing Galaxy Evolution by Their Present-Day Luminosity Function

Articles in the same Issue

1. Preface
2. Star Classification Possibilities with the Gaia Spectrophotometers. III. The Classification Accuracy with Decontaminated BP/RP Spectra
3. Towards the Automatic Estimation of Time Delays of Gravitational Lenses
4. Some Pages of History of the Specula Dorpatensis, the Elder Sister of Pulkovo Observatory
5. How Struve and Tenner Started the Work of Their Life
6. Anders Celsius’ Contributions to Meridian Arc Measurements and the Establishment of an Astronomical Observatory in Uppsala
7. Bernhard Schmidt and the Schmidt Telescope for Mapping the Sky
8. Ernst Julius Öpik, Solar Variability and Climate Change
9. Recent Advances in Solar Physics at VIRAC: Analysis of Solar Active Regions in Microwaves
10. Grigori Kuzmin and Stellar Dynamics
11. Astrometry Lost and Regained
12. Dark Matter
13. Tracing Galaxy Evolution by Their Present-Day Luminosity Function
14. Some Properties of Galaxy Structures
15. Measuring the Cosmic Web
16. Cosmological Neutrino Background and Connected Problems
17. High-Quality Fast QPOs from Magnetars: An Electric Circuit Model
18. Transfer Equation in General Curvilinear Coordinates
19. Some Studies of Terrestrial Impact Cratering Rate
20. Some Relations Between the Stockholm and Tartu Observatories During the 19th Century
21. Extinction of Radiation in the Universe: from F. G. W. Struve Up to Now
22. Tadeusz Banachiewicz in Tartu (1915 to 1918)
23. Studying the Patterns of the Universe
24. Galaxy Superclusters Detected in the Modified PF-Catalog Using the FOF Method