We begin with the UDG catalog from Zaritsky et al. (2019, J/ApJS/240/1) of 275 UDG candidates with half light radii, r_h_>~5.3" that lie within roughly a 10{deg} projected...

Observations were taken during two observing runs in 2014 and 2017. Our strategy consisted of obtaining continuous observations of our field in two bands (g and r) for several...

The polarisation study presented in this paper is based on unpublished data of the radio galaxy B2 0258+35 from the WSRT archive. The data consist of two full 12 h tracks...

The COSMOS field has been observed in a broad range of wavelengths, with imaging data from X-ray to radio and number of spectroscopic campaigns. We have added to the...

Photometric redshifts are calculated using the optical photometry catalogs presented in Kondapally et al. (Paper III. 2020, in prep.), using a hybrid template + machine learning...

In this paper, we present the multi-wavelength counterpart information and source-associated catalogues of the LOFAR-detected sources in the LoTSS Deep Fields Data Release 1. In...

The ELAIS-N1 data presented in this paper were taken in the LOFAR observation cycles 0, 2, and 4 (proposals LC0_019, LC2_024, and, LC4_008 respectively) from May 2013 to August...

The Census of the Local Universe (CLU) emission-line (H{alpha}) galaxy survey (CLU-Ha) is a narrowband survey of the entire northern sky above a decl. of -20{deg}, with the aim...

The observational data set consists of 15GHz VLBA observations of 409 AGNs obtained between 1994 August 31 and 2016 December 26 as part of the 2cm VLBA survey and Monitoring Of...

For our sample selection, we use the multiwavelength photometric catalogs from ZFOURGE (Straatman+ 2016, J/ApJ/830/51), which overlap with the CANDELS survey in the COSMOS,...

We have selected all Alerts appearing in the Gaia Alerts website from the beginning (first one Gaia14aaa, detected on August 30th, 2014), to the end of October 2018 (last one...

The Deep Extragalactic Exploratory Probe (DEEP) is a multiphase research program dedicated to the study of the formation and evolution of galaxies and of large-scale structure...

The sample set is composed of 20 iETGs that are included in the Analysis of the interstellar Medium of Isolated Galaxies sample (AMIGA, Verdes-Montenegro et al. (2005, Cat....

We perform a photometric study on four new fields that complements those carried out in previous surveys on the Antlia cluster of galaxies. These fields were observed with the...

As a step toward investigating the parsec-scale properties of faint extragalactic radio sources, the Very Long Baseline Array (VLBA) was used at 5.0GHz to obtain...

Photometric catalogues of NGC 6822 from PS1, Gaia, LGGS, UKIRT, VHS, IRSF, HAWK-I, Spitzer, and WISE. We also identified 234 RSG candidates. The catalogues mainly provide...

Eight dense galaxy groups in the COSMOS field at intermediate redshifts (z~0.7) were studied using IFU and high resolution photometry data to determine morphological and...

Observations of the ^12^CO(1-0) emission were carried out with the IRAM Plateau de Bure Interferometer (PdBI) in summer 2014 using all six antennas in C and D configuration. The...

Photometric parameters, coordinates, and predicted H{alpha}, H{beta}, [OII]3727AA, and [OIII]5007AA line fluxes from spectral energy distribution modeling are presented....

We present Low-Frequency Array (LOFAR) maps of Canes Venatici I. Data are at full angular resolution, low angular resolution (FWHM=20arcsec), with sources included and...