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Cataclysmic variables from DESI DR1 sp.
We present a systematic search for cataclysmic variables (CVs) using spectroscopic data from Data Release 1 of the Dark Energy Spectroscopic Instrument. Applying the... -
X-Shooter acc disc properties of Sco-Cen stars
The evolution of protoplanetary discs is intertwined with the process of planet formation, growth and migration. Studies of nearby star-forming regions of different ages and... -
SMaSH+ physical properties of O-Stars pairs
A key property of massive stars is their high degree of multiplicity, which can impact their evolution and end-of-life products. The Southern Massive Stars at High Angular... -
Stellar properties of M3/M13 HB stars with UVIT
We present a far-ultraviolet (FUV) study of hot stellar populations in the second parameter pair globular clusters (GCs) M3 and M13, as a part of the GC UVIT Legacy Survey... -
Kinematic groups in USco with GaiaEDR3
The improved astrometry precision of Gaia-eDR3 allows us to perform a detailed study of the Upper Scorpius OB association and revisit its spatial, kinematic, and age... -
Stellar properties of Sun-like stars SDST III
The Survey for Distant Solar Twins aims to find stars very similar to the Sun at distances of 1-4kpc, several times more distant than any currently known solar twins and... -
Omega/WINGS clusters/fields galaxies
The observed properties of galaxies are strongly dependent on both their total stellar mass and their morphology. Furthermore, the environment is known to play a strong role in... -
HSC gLSB galaxies structures and SB properties
Rare giant low surface brightness galaxies (gLSBGs) act as a stress test for the current galaxy formation paradigm. To answer the question 'How rare are they?', we estimate... -
Radio-loudness stat. of QSOs from Quaia-VLASS
Quasars are objects of high interest in extragalactic astrophysics, cosmology, and astrometry. One of their useful qualities is their potential radio-loudness. However, the... -
Gas content of star-forming galaxies
Stars do not form continuously distributed over star-forming galaxies. They form in star clusters of different masses. This nature of clustered star formation is taken into... -
Carbon star candidates from LAMOST and SDSS
Carbon stars are critical for understanding stellar evolution and exploring cosmic chemistry. This paper provides 7809 carbon star candidates identified from the Large-Area... -
JADES and FRESCO Ha-emitting galaxies at z=5.1-5.5
HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at... -
M dwarfs properties in VVV b294 inner bulge field
M dwarf stars are the dominant stellar population in the Milky Way, and they are important for a wide variety of astrophysical topics. The Gaia mission has delivered a superb... -
ASPIC VIPERS catalogue on W4 field
Photometry, physical parameters and spectral features of VIPERS PDR-2 sources on W4 field. -
ASPIC VIPERS catalogue on W1-VIDEO field
Photometry, physical parameters and spectral features of VIPERS PDR-2 sources on W1-VIDEO field. -
ASPIC GAMA catalogue on G09 G12 G15 fields
ASPIC value-added catalogue on GAMA G09, G12, and G15 fields. -
ASPIC GAMA catalogue on G02 field
ASPIC value-added catalogue on GAMA G02 field. -
ASPIC VUDS-DR1 catalogue on ECDFS field
Photometry, spectral features, and physical parameters of VUDS (DR1) sources on ECDFS field. -
ASPIC VIPERS catalogue on W1 field
Photometry, physical parameters and spectral features of VIPERS PDR-2 sources on W1 field. -
ASPIC MUSE-Wide DR1 catalogue
Photometry, spectral features, and physical parameters of MUSE-Wide sources on GOODS-South field.
