Journal: Monthly Notices of the Royal Astronomical Society
Publication
SY Cnc, a case for unstable mass transfer?
Intermediate-resolution (0.5-1 Å) optical spectroscopy of the cataclysmic variable (CV) SY Cnc reveals the spectrum of the donor star. Our data enable us to...
Synchrotron emission from the blazar PG 1553+113. An analysis of its flux and polarization variability
In 2015 July 29-September 1, the satellite XMM-Newton pointed at the BL Lac object PG 1553+133 six times, collecting data for 218 h. During one of these epochs...
Synthesis of infrared Stokes spectra in an evolving solar chromospheric jet
Chromospheric jets are plausible agents of energy and mass transport in the solar chromosphere, although their driving mechanisms have not yet been elucidated...
Synthetic galaxy clusters and observations based on Dark Energy Survey Year 3 Data
We develop a novel data-driven method for generating synthetic optical observations of galaxy clusters. In cluster weak lensing, the interplay between analysis...
Synthetic polarimetric spectra from stellar prominences
Stellar prominences detected in rapidly rotating stars serve as probes of the magnetism in the corona of cool stars. We have synthesized the temporal evolution...
System initial mass function of the 25 Ori group from planetary-mass objects to intermediate/high-mass stars
The stellar initial mass function (IMF) is an essential input for many astrophysical studies but only in a few cases has it been determined over the whole...
System mass constraints for the accreting millisecond pulsar XTE J1814-338 using Bowen fluorescence
We present phase-resolved spectroscopy of the millisecond X-ray pulsar XTE J1814-338 obtained during its 2003 outburst. The spectra are dominated by high...
System parameters of three short-period cataclysmic variable stars
Using photometric ULTRACAM observations of three new short-period cataclysmic variables (CVs), we model the primary eclipse light curves to extract the orbital...
Systematic analysis of jellyfish galaxy candidates in Fornax, Antlia, and Hydra from the S-PLUS survey: a self-supervised visual identification aid
We study 51 jellyfish galaxy candidates in the Fornax, Antlia, and Hydra clusters. These candidates are identified using the JClass scheme based on the visual...