ML-Enhanced GCVS: Variable Stars with Gaia DR3 and TESS
Short Name:
KazVO Variable Stars
Date:
13 Mar 2025 08:45:50
Publisher:
Fesenkov Astrophysical Institute
Description:
This catalog combines photometric and astrometric data from three
major sources: the General Catalogue of Variable Stars (GCVS,
2017ARep...61...80S), Gaia DR3, and TESS. It provides detailed
information on variable stars, including their coordinates,
magnitudes, variability periods, parallaxes, proper motions, spectral
classifications, and other physical characteristics. Additionally, the
catalog includes computed parameters such as galactocentric distances
and model-predicted values for spectral types and variability types
for stars with incomplete observational data. The catalog aims to
facilitate studies of stellar variability, galactic structure, and
stellar evolution.
This service queries the unified source catalogue of radio sources
from the Multifrequency Snapshot Sky Survey (MSSS) Verification Field.
This survey is the first major observing program to be carried out
with LOFAR during its ongoing commissioning phase. This service
queries the unified source catalogue database for the MSSS survey. The
Verification Field is a region of 100 square degrees centered at
(15h,69◦).
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Description:
MUDEHaR DR1 (March, 2025). MUDEHaR (MUlti-epoch Disparity Examination of H-Alpha and infraRed) is a multi-epoch photometric survey of two narrow filters: Hα and the calcium triplet window. Using the JAST telescope and T80Cam instrument at the Observatorio Astrofísico de Javalambre (OAJ, Teruel, Spain) is studying 40 square degrees of star forming fields in the Galactic disk. It will detect all kind of variable Hα stars on a days-months-years scale. . Please include the following in any published material that makes use of this data: "Based on observations made with the JAST80 telescope for the MUDEHaR project at the Observatorio Astrofísico de Javalambre, in Teruel, owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón."
MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found
in the 2MAst (2MASS with Astrometry) catalogue. The target list was
compiled on the basis of present-day lists of open, globular and
candidate clusters. For confirmed clusters we determined a homogeneous
set of astrophysical parameters such as membership, angular radii of
the main morphological parts, mean cluster proper motions, distances,
reddenings, ages, tidal parameters, and sometimes radial velocities.
MWSC-e14a ("MWSC extension 2014a") is a catalogue of
139 new open clusters at high Galactic latitudes
(\|b\|>20 deg) including lists of candidate members. It extends the
Kharchenko et al. 'Catalog of Milky Way Star Clusters'.
The target list was compiled as density enhancements found in the 2MASS
point source catalogue. For confirmed clusters we determined a homogeneous
set of astrophysical parameters such as membership, angular radii of the
main morphological parts, proper motion, distance, reddening, age, and
tidal parameters.
.. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/form
MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found
in the 2MAst (2MASS with Astrometry) catalogue. The target list was
compiled on the basis of present-day lists of open, globular and
candidate clusters. For confirmed clusters we determined a homogeneous
set of astrophysical parameters such as membership, angular radii of
the main morphological parts, mean cluster proper motions, distances,
reddenings, ages, tidal parameters, and sometimes radial velocities.
NED's implementation of the VO Table Access Protocol, or TAP.
The results include main information from NED about the objects:
Preferred name for the object, Position, Redshift, Type of the Object, and numbers
of main results for the object.
