© 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim Mini-MegaTORTORA is a nine-channel wide-field camera that continuously monitors the sky looking for rapid optical transients since mid-2014. It is also performing a regular sky survey, and has already acquired nearly half a million images covering every point of Northern Sky hundreds to thousands of times. Photometric analysis of these data may provide a huge amount of information useful for the detection and characterization of different types of variable objects. Here we present a brief description of our activities related to the acquisition, processing, and calibration of these data, as well as examples of uncataloged variable stars of various types detected during the analysis
Having a need to perform differential photometry for tens of thousands stars in a several square deg...
Two fully automatic Pi of the Sky detectors with a large field of view, located in Spain (INTA) and ...
peer reviewedPhotometric measurements are prone to systematic errors presenting a challenge to lowam...
© 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim Mini-MegaTORTORA is a nine-channel wide-field ca...
© 2017, Pleiades Publishing, Ltd.We describe the properties of Mini-MegaTORTORA (MMT-9) nine-channel...
Here we present the summary of first years of operation and the first results of a novel 9-channel w...
A set of 64 simultaneous optical and near-infrared photometric observations of 17 late-type giants i...
The Chinese Small Telescope Array (CSTAR) is the first telescope facility built at Dome A, Antarctic...
We describe photometric recalibration of data obtained by the asteroid survey LINEAR. Although LINEA...
Pi of the Sky is a system of two wide field of view robotic telescopes, which search for short times...
We present variability analysis of data from the Northern Sky Variability Survey (NSVS). Using the c...
We present variability analysis of data from the Northern Sky Variability Survey (NSVS). Using the c...
Abstract. Measuring magnitudes from astronomical images can be slow and difficult when done by hand,...
© 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim We briefly present the status of digitization an...
Sky surveys represent a fundamental data basis for astronomy. We use them to map in a systematic way...
Having a need to perform differential photometry for tens of thousands stars in a several square deg...
Two fully automatic Pi of the Sky detectors with a large field of view, located in Spain (INTA) and ...
peer reviewedPhotometric measurements are prone to systematic errors presenting a challenge to lowam...
© 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim Mini-MegaTORTORA is a nine-channel wide-field ca...
© 2017, Pleiades Publishing, Ltd.We describe the properties of Mini-MegaTORTORA (MMT-9) nine-channel...
Here we present the summary of first years of operation and the first results of a novel 9-channel w...
A set of 64 simultaneous optical and near-infrared photometric observations of 17 late-type giants i...
The Chinese Small Telescope Array (CSTAR) is the first telescope facility built at Dome A, Antarctic...
We describe photometric recalibration of data obtained by the asteroid survey LINEAR. Although LINEA...
Pi of the Sky is a system of two wide field of view robotic telescopes, which search for short times...
We present variability analysis of data from the Northern Sky Variability Survey (NSVS). Using the c...
We present variability analysis of data from the Northern Sky Variability Survey (NSVS). Using the c...
Abstract. Measuring magnitudes from astronomical images can be slow and difficult when done by hand,...
© 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim We briefly present the status of digitization an...
Sky surveys represent a fundamental data basis for astronomy. We use them to map in a systematic way...
Having a need to perform differential photometry for tens of thousands stars in a several square deg...
Two fully automatic Pi of the Sky detectors with a large field of view, located in Spain (INTA) and ...
peer reviewedPhotometric measurements are prone to systematic errors presenting a challenge to lowam...