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Data publication: Let's get cyclic – Influence of Head-to-Tail Cyclisation of...
The dataset comprises the experimental data that form the basis of the conclusions presented in the paper, including spectroscopic, calorimetric, and microscopic data. This... -
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... -
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... -
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). -
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... -
Early phot. and spectroscopic obs. of SN 2023bee
We present high-cadence ultraviolet through near-infrared observations of the Type Ia supernova (SN Ia) 2023bee at D=32+/-3Mpc, finding excess flux in the first days after... -
QSOs at z~4 from Subaru/HSC wide field & BH masses
We investigate the black hole mass function (BHMF) and Eddington-ratio distribution function (ERDF) of broad-line active galactic nuclei (AGNs) at z=4, based on a sample of 52... -
Classifying intermediate-z galaxies in SDSS
We select a sample of 1437 active galactic nuclei (AGN) from the catalog of the Sloan Digital Sky Survey galaxy properties from the Portsmouth group by detection of the... -
ACO 746 analysis with Subaru & MMT spectra data
The galaxy cluster A746 (z=0.214), featuring a double radio relic system, two isolated radio relics, a possible radio halo, disturbed V-shaped X-ray emission, and intricate... -
Optical spectra of 14 planetary nebula candidates
The Gaia DR3, released in June 2022, included low-resolution BP/RP (XP) spectra that have been exploited for the classification of various types of emission-line objects using... -
Gaia20fnr reduced spectra
The microlensing event Gaia20fnr is a long-duration, non-caustic-crossing binary-lens event located at high Galactic latitude. Triggered by a photometric rise detected by the...
