Received: 2015-1-29
Revised: 2015-5-28
Revised: 2015-6-10
Accepted: 2015-6-11
Published Online: 2017-2-18
Published in Print: 2015-9-1
© 2015 Vladimír Tichý et al., published by De Gruyter Open
Articles in the same Issue
- Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
- Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3
- Optics for Nano-Satellite X-Ray Monitor
- Observational Data and Orbits of the Asteroids Discovered at the Baldone Observatory in 2008–2013
- On the Pseudo Phase-space Density of Dark Matter Haloes and the Universality of Density Profiles
- Baryon Physics and the Missing Satellites Problem
- A Young Star Cluster in the Leo a Galaxy
- Supershells in the M33 Galaxy
- Structural Parameters of Star Clusters: Signal to Noise Effects
- Artificial Star Test for Crowded Field CCD Photometry
- Ultraviolet and Infrared Correlation Studies in Orion
- Ultraviolet Spectroscopic Investigation of HU Aqr and AN UMa with the Data from HST and IUE
Keywords for this article
instrumentation: detectors;
space vehicles: instruments;
telescopes
Creative Commons
BY-NC-ND 3.0
Articles in the same Issue
- Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
- Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3
- Optics for Nano-Satellite X-Ray Monitor
- Observational Data and Orbits of the Asteroids Discovered at the Baldone Observatory in 2008–2013
- On the Pseudo Phase-space Density of Dark Matter Haloes and the Universality of Density Profiles
- Baryon Physics and the Missing Satellites Problem
- A Young Star Cluster in the Leo a Galaxy
- Supershells in the M33 Galaxy
- Structural Parameters of Star Clusters: Signal to Noise Effects
- Artificial Star Test for Crowded Field CCD Photometry
- Ultraviolet and Infrared Correlation Studies in Orion
- Ultraviolet Spectroscopic Investigation of HU Aqr and AN UMa with the Data from HST and IUE