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IGM metal enrichment with UVES deep spectrum
The distribution and the abundance of metals in the intergalactic medium (IGM) have strong implications for galaxy formation and evolution models. The ionic transitions of heavy... -
Interstellar medium in early-type gal. V. GAMA DR4
Quenching of star formation plays a fundamental role in galaxy evolution. This process occurs due to the removal of the cold interstellar medium (ISM) or stabilization against... -
Bent-tail radio galaxies from FIRST and hosts
Bent-tail radio galaxies (BTRGs) are characterized by bent radio lobes. This unique shape is mainly caused by the movement of the galaxy within a cluster, during which the radio... -
Beyond ultra-diffuse galaxies. I. HSC PDR2 MW analogs
Large diffuse galaxies are hard to find, but understanding the environments where they live, their numbers, and ultimately their origins, is of intense interest and importance... -
Properties of type 1 AGNs
We examine the connection between galaxy mergers and the triggering of active galactic nuclei (AGNs) using a sample of 614 type 1 AGNs at z<0.07, along with a control sample... -
DESI DR1 redshift catalog
In 2021 May the Dark Energy Spectroscopic Instrument (DESI) collaboration began a 5-year spectroscopic redshift survey to produce a detailed map of the evolving... -
Finding galaxy clusters with machine learning
Building a comprehensive catalog of galaxy clusters is a fundamental task for studies on structure formation and galaxy evolution. In this paper, we present Cluster Optical... -
LOFAR 58MHz Legacy Survey of 3CRR catalog
The Low Frequency Array (LOFAR) is uniquely able to perform deep, high- resolution imaging at frequencies below 100MHz. Observations in this regime, using the Low Band Antenna... -
ALMA obs. of HCN and HCO+ for 12 (U)LIRGs
We present the results of our ALMA<~0.5kpc resolution dense molecular line (HCN and HCO^+^J=2-1, J=3-2, and J=4-3) observations of 12 nearby (ultra)luminous infrared galaxies... -
ASAS-SN core-collapse supernova with MUSE
The analysis of core-collapse supernova (CCSN) environments can provide important information on the life cycle of massive stars and constrain the progenitor properties of these... -
Bright gamma-ray blazars among the 4LAC
Gamma-ray flares of blazars may be accompanied by high-energy neutrinos due to interactions of high-energy cosmic rays in the jet with photons, as suggested by the detection of... -
TOPz photo-z for the GAMA sample
Accurate photometric redshift (photo-z) estimation is crucial for cosmological and galaxy evolution studies, especially with the advent of large-scale photometric surveys. We... -
The SDSS Photometric Catalog, Release 9
The Sloan Digital Sky Survey III (SDSS-III) presents the first spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS). This ninth data release (DR9) of the... -
UVCANDELS: phot. redshifts & galaxy physical param.
The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep Hubble Space Telescope (HST) F275W and... -
Keck/DEIMOS redshifts for galaxies in ACO 56
We report the discovery of a binary galaxy cluster merger via a search of the redMaPPer optical cluster catalog, with a projected separation of 535kpc between the brightest... -
COSMOS-Web Brightest Group Galaxy (BGG) Cat.
We present the first comprehensive study of the structural evolution of Brightest Group Galaxies (BGGs) from redshift z~0.08 to z=3.7 using the James Webb Space Telescope's... -
The SDSS Photometric Catalog, Release 8
Cone search capability for table II/306/sdss8 (* output of the SDSS photometric catalog) -
JADES NIRCam & NIRSpec phot. & line fluxes cat. (DR1-DR3)
JWST has revolutionized the field of extragalactic astronomy with its sensitive and high-resolution infrared view of the distant Universe. Adding to the new legacy of JWST... -
Gamma-ray burst redshifts
We here propose a new model-independent technique to overcome the circularity problem affecting the use of gamma-ray bursts (GRBs) as distance indicators through the use of... -
Hubble Frontier Fields clusters lensing
We present free-form gravitational lensing models derived with the WSLAP+ code for the six Hubble Frontier Fields clusters using the latest data available from the Frontier...
