output
20022020
most citedThe ACS Nearby Galaxy Survey Treasury

564 citations

Showing 2016Show all

11 papers · 1 filter

astro-ph.SR20161 cited

Light equation in eclipsing binary CV Boo: third body candidate in elliptical orbit

A. I. Bogomazov, V. S. Kozyreva, B. L. Satovskii +8

A short period eclipsing binary star CV Boo is tested for the possible existence of additional bodies in the system with a help of the light equation method. We use data on the mom…

astro-ph.GA201625 cited

On the influence of the environment on galactic chemical abundances

L. S. Pilyugin, E. K. Grebel, I. A. Zinchenko +2

We examine the influence of the environment on the chemical abundances of late-type galaxies with masses of 10^9.1 M_sun - 10^11 M_sun using data from the Sloan Digital Sky Survey(…

astro-ph.IM20164 cited

A Technique for Simultaneous Measurement of Circular and Linear Polarization with Single-Channel Polarimeter

Sergey V. Kolesnikov, Vitalii V. Breus, Nickolay N. Kiselev +1

The algorithm is described, which have been used for photo-polarimetric monitoring of various astronomical objects - cataclysmic variables, asteroids, comets.

astro-ph.GA201615 cited

MiNDSTEp differential photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756: Microlensing and a new time delay

E. Giannini, R. W. Schmidt, J. Wambsganß +52

We present V and R photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756. The data were taken by the MiNDSTEp collaboration with the 1.54 m Danish telescope…

astro-ph.SR201610 cited

RZ Leonis Minoris Bridging between ER Ursae Majoris-Type Dwarf Nova and Novalike System

Taichi Kato, Ryoko Ishioka, Keisuke Isogai +64

We observed RZ LMi, which is renowned for the extremely (~19d) short supercycle and is a member of a small, unusual class of cataclysmic variables called ER UMa-type dwarf novae, i…

astro-ph.GA201637 cited

Do Some AGN Lack X-ray Emission?

Charlotte Simmonds, Franz E. Bauer, Trinh X. Thuan +3

Intermediate-Mass Black Holes (IMBHs) are thought to be the seeds of early Supermassive Black Holes (SMBHs). While 100 IMBH and small SMBH candidates have been…