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Morphologies in the Cepheus Flare region
These tables contain the data of the cloud sample on which the study of the relationships between cloud morphology, optical and IR properties, and star formation is based. The... -
VEGAS-SSS photometry of NGC3115
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of NGC 3115, observed as part of the ongoing wide-field imaging survey VEGAS,... -
CALIFA DR2
This paper describes the Second Public Data Release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. The data for 200 objects are made public, including the... -
Astrometric Catalogue 5, LQAC-5
In addition to their great astrophysical interest, quasars represent quasi-ideal reference objects in the celestial sphere with, a priori, a lack of significant proper motion.... -
r' magnitudes and sizes of Oph cluster galaxies
Ophiuchus is one of the most massive clusters known, but due to its low Galactic latitude its optical properties remain poorly known. We investigate the optical properties of... -
Disc galaxies baryonic specific ang. mom.
Specific angular momentum (the angular momentum per unit mass, j=J/M) is one of the key parameters that control the evolution of galaxies, and it is closely related with the... -
The OTELO survey as morphological probe
The morphology of galaxies provide us with a unique tool to connect and understand other related physical properties and their changes over the course of cosmic time. Only... -
FR-type radio sources at 3GHz VLA-COSMOS
Radio active galactic nuclei (AGN) are traditionally separated into two Fanaro-Riley (FR) type classes, edge-brightened FRII sources or edge-darkened FRI sources. With the... -
SDSS galaxies morphological classification
Machine learning methods are effective tools in astronomical tasks for classifying objects by their individual features. One of the promising utilities is related to the... -
Star formation quenching stages of galaxies
The mechanisms that bring galaxies to strongly reduce their star formation activity (star-formation quenching) remain poorly understood. To better study galaxy evolution, we... -
Feature-based asteroid taxonomy in 3D color space
The taxonomic classification of asteroids has been mostly based on spectroscopic observations with wavelengths spanning from the visible (VIS) to the near-infrared (NIR).... -
GAMA. MegaMorp/GalfitM profile fits
We present the capabilities of Galapagos-2 and Galfitm in the context of fitting two-component profiles - bulge-disk decompositions - to galaxies, with the ultimate goal of... -
MUSE surveys intermediate-redshift galaxies
We quantify the stellar rotation of galaxies by computing the {lambda}R parameter, a proxy for the stellar angular momentum in a sample of 106 intermediate-redshift galaxies... -
13CO clump properties two 2 W5 bubble regions
The feedback effect of massive stars can either accelerate or inhibit star formation activity within molecular clouds. Studying the morphology of molecular clouds near W5 offers... -
Bar galaxies and their environments
The prints of the Palomar Sky Survey, luminosity classifications, and radial velocities were used to assign all northern Shapley-Ames galaxies to either (1) field, (2) group, or... -
HI 21cm observations of Pegasus galaxies
We present neutral hydrogen observations of 54 galaxies in the Pegasus Cluster. The observations include single-dish HI measurements, obtained with the Arecibo telescope for all... -
Spitzer c2d small clouds and cores
We present the results of a submillimeter survey of 53 low-mass dense cores with the Submillimeter High Angular Resolution Camera II (SHARC-II). The survey is a follow-up... -
Globulettes in four HII regions
Some HII regions surrounding young stellar clusters contain tiny dusty clouds, which on photos look like dark spots or teardrops against a background of nebular emission. From... -
104 large asteroids mass determination studies
The techniques described in an earlier paper were used to determine masses of 104 asteroids by the method of asteroid-asteroid gravitational interaction. For each of the 104... -
A new catalog of HII regions in M31
We present a new catalog of HII regions in M31. The full disk of the galaxy (~24kpc from the galaxy center) is covered in a 2.2deg^2^ mosaic of 10 fields observed with the...
