This document describes the analysis, design, and prototype test results of the microwave section of a 10- to 19.5-GHz interferometer, aimed at obtaining...
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Publication10- to 19.5-GHz microwave receiver of an electro-optical interferometer for radio astronomy
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Publication10-GHz Tenerife cosmic microwave background observations at 8 deg resolution and their analysis using a new maximum entropy method
The complete set of data from the Tenerife 10-GHz (8-deg FWHM) twin-horn, drift scan experiment is described. These data are affected by both long-term...
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Publication1000 cataclysmic variables from the Catalina Real-time Transient Survey
Over six years of operation, the Catalina Real-time Transient Survey (CRTS) has identified 1043 cataclysmic variable (CV) candidates - the largest sample of CVs...
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Publication12C/13C isotopic ratios in red-giant stars of the open cluster NGC 6791
Carbon isotope ratios, along with carbon and nitrogen abundances, are derived in a sample of 11 red-giant members of one of the most metal-rich clusters in the...
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Publication155-day Periodicity in solar cycles 3 and 4
The near 155 days solar periodicity, so called Rieger periodicity, was first detected in solar flares data and later confirmed with other important solar...
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Publication1RXS J062518.2+733433: A new intermediate polar
We report the identification of the cataclysmic variable 1RXS J062518.2+733433 as an intermediate polar. The orbital period of the system is determined to be...
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Publication1RXS J180408.9-342058: An ultra compact X-ray binary candidate with a transient jet
Aims: We present a detailed near-infrared/optical/UV study of the transient low-mass X-ray binary 1RXS J180408.9-342058 performed during its 2015 outburst...
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Publication2-D Numerical Simulation of the Ambipolar Filamentation of Turbulent Magnetic Fields
Magnetic fields play an important role in astrophysics and they often dominate the behavior of magnetized media. We simulate the mechanism (Tagger et al., 1995)...
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Publication26Al in galaxy regions: massive-star interactions with the ISM
Galactic 26Al is believed to be predominantly injected into the ISM from winds and supernovae of massive stars. These stars are typically born in groups and...