20 datasets found

Keywords: variable stars

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  • Bochum Galactic Disk Survey (BGDS) images

    The Bochum Galactic Disk Survey is an ongoing project to monitor the stellar content of the Galactic disk in a 6 degree wide stripe centered on the Galactic plane. The data has...
  • BGDS Mean Photometry Cone Search

    Extracted sources from the Bochum Galactic Disk Survey. We provide mean photometry in U, B, V, z, r, and i bands. Note that sources in different bands are not matched. Also,...
  • RW Aur spectroscopy and photometry

    RW Aurigae is a young stellar system containing a classical T Tauri star as the primary component. It shows deep, irregular dimmings, first detected in 2010. At the University...
  • Interstellar Polarization Survey. III.

    Optical starlight can be partially polarized while propagating through the dusty, magnetized interstellar medium (ISM). The polarization efficiency describes the polarization...
  • TESS LCs of TTauri star Classification

    We present a variability and morphological classification study of TESS light curves for TTauri star candidates in the Orion, IC348, {gamma}Velorum, Upper Scorpius, Corona...
  • Bochum Galactic Disk Survey (BGDS) light curves

    This service exposes the light curves of stars produced by the Bochum Galactic Disk Survey; several million light curves are provided in the SDSS i and r bands. The lightcurves...
  • AAVSO Photometric All Sky Survey (APASS) DR10

    AAVSO Photometric All-Sky Survey (APASS), underway since 2010, covers the entire sky from 7.5 < V < 16.5 magnitude, and in the BVugrizY bandpasses. A northern and a...
  • Detection of 228 variable stars in NGC 281

    We identify 228 periodic variables in the region of young open cluster NGC 281 using time series photometry carried out from 1 m class ARIES telescopes, Nainital. The cluster...
  • CFHT optical & NIR obs. of RR Lyrae in M15

    Messier 15 (NGC 7078) is an old and metal-poor post core-collapse globular cluster that hosts a rich population of variable stars. We report new optical (gi) and near-infrared...
  • Type II Cepheids in the Magellanic Clouds

    Type II Cepheids (T2Cs) are the less frequently used counterparts of classical or type I Cepheids (CCs) which provide the primary calibration of the distance ladder for...
  • Radial velocities for 7 cataclysmic variables

    We report spectroscopic observations of seven bright southern cataclysmic variable stars, collected on a single two-week observing run using the 1.9m Radcliffe telescope at the...
  • RR Lyrae stars in Galactic Globular Clusters

    We present a comprehensive catalog of 2824 RR Lyrae stars (RRLs) residing in 115 Galactic globular clusters (GCs). Our catalog includes 1594 fundamental- mode (RRab), 824...
  • BL Her stars Gaia PL relation

    In the era of the Hubble tension, it is crucial to obtain a precise calibration of the period-luminosity (PL) relations of classical pulsators. Type II Cepheids (T2Cs; often...
  • Parameteres for 88 giant variable star candidates

    We present the analysis of 510 light curves in V and I bands of 255 giant stars in the globular cluster NGC-3201. Our aim is to expand the sample of new types of variables...
  • Field RR Lyrae stars RV and pulsation models

    The application of the Parallax of Pulsation (PoP) technique to determine the distances of pulsating stars implies the use of a scaling parameter, the projection factor...
  • Infrared LC and spectrum of Scutum X-1 system

    The symbiotic X-ray binary Sct X-1 was suggested to be the first known neutron star accreting from a red supergiant companion. Although known for nearly 50yr, detailed...
  • V838 Cyg; O-C, amplitude & Fourier coeff modulations

    Noting the weakest modulation and relatively high metal abundance of the Ab-type RR-Lyrae star V838Cyg, we collected the photometric data of this star from several sky surveys...
  • Spatiotemporal technosignature candidate targets

    Spatiotemporal techniques for signal coordination with actively transmitting extraterrestrial civilizations, without the need for prior communication, can constrain...
  • Known exoplanet hosts parameters with TESS

    Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of...
  • Spot modeling of V1298 Tau using SpotCCF tool

    The intrinsic variability due to the magnetic activity of young active stars is one of the main challenges in detecting and characterising exoplanets. The stellar activity is...
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