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EXOSAT TGS Spectra and Lightcurves
Spectra obtained using the EXOSAT transmission grating spectrometer, TGS. There are two databases TGS and TGS2 as follows: <pre> * TGS - the grating spectra averaged over... -
EXOSAT TGS L and R Orders
Spectra obtained using the EXOSAT transmission grating spectrometer, TGS. There are two databases TGS and TGS2 as follows: <pre> * TGS - the grating spectra averaged over... -
Data Central TAP
TAP service for surveys hosted by Data Central -
Galaxy Zoo barred galaxies properties with MaNGA
We study the bar pattern speeds and corotation radii of 225 barred galaxies, using integral field unit data from MaNGA and the Tremaine-Weinberg method. Our sample, which is... -
The X-ray ExSeSS source sample from 2SXPS
We present the Extragalactic Serendipitous Swift Survey (ExSeSS), providing a new well-defined sample constructed from the observations performed using the Swift X-ray... -
PNe using Gaia DR3 and O/H gradient
The spatial distribution of chemical elements in the Galactic disk provides key constraints on models of galaxy evolution. However, studies using planetary nebulae (PNe) as... -
APO ACCELS. Ages, Li EW, & Prot for 166 accel. stars
Directly imaged substellar companions with well-constrained ages and masses serve as vital empirical benchmarks for planet formation and evolution models. Potential benchmark... -
EGPM. III. HPF RVs & activity of young giant planets
We present statistical results from the Epoch of Giant Planet Migration RV planet search program. This survey was designed to measure the occurrence rate of giant planets... -
Starless and pre-stellar cores sulfur depletion
Sulfur is one of the most abundant elements in the Universe, yet the sulfur budget inferred from the observed sulfur-bearing molecules in dense cores is significantly lower than... -
[M/H] of K/M dwarfs in SN kinematic structures
We combine photometric metallicities with astrometry from Gaia DR3 to examine the chemodynamic structure of ~250000 K dwarfs in the solar neighbourhood (SN). In kinematics, we... -
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... -
Spectrophotometric magnetic study of MWD stars
We present a homogeneous analysis of all DA stars labelled as magnetic in the Montreal White Dwarf Database. Our sample is restricted to almost all known magnetic white dwarf... -
n-catpure abundances in NGC 6752
Globular clusters have been widely studied in terms of light element variations present in their different stellar populations. However, the nature of the polluter(s)... -
PN K4-47 spectra
The object K4-47 is a young planetary nebula that exhibits low-ionisation structures in the form of two "lobes". The unusual chemistry of the nebula has raised questions about... -
Data Central SSA
Spectra from surveys hosted by Data Central. Most spectra were taken with the multi-object spectroscopy facilities 2dF (Anglo-Australian Telescope) and 6dF (UK Schmidt Telescope). -
ESO TAP_OBS: a TAP service to browse and access raw and reduced data, and to ...
TAP_OBS is the ESO Science Archive TAP endpoint for observations (raw and reduced data) and ambient measurements (atmospheric seeing, turbulence, water vapour, relative... -
Pavol Jozef Šafárik University Archive TAP service
The Pavol Jozef Šafárik University Archive's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and... -
CEERS Key Paper. VIII. NIRSpec & NIRCam sp.
We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early... -
3D kinematics in the ONC. II. Mass-dependent results
We present the kinematic analysis of 246 stars within 4' from the center of Orion Nebula Cluster (ONC), the closest massive star cluster with active star formation across the...
