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161. Catalogue of features in the S4G
ID:
ivo://CDS.VizieR/J/A+A/582/A86
Title:
Catalogue of features in the S4G
Short Name:
J/A+A/582/A86
Date:
21 Oct 2021
Publisher:
CDS
Description:
A catalogue of the features for the complete Spitzer Survey of Stellar Structure in Galaxies (S4G), including 2352 nearby galaxies, is presented. The measurements are made using 3.6um images, largely tracing the old stellar population; at this wavelength the effects of dust are also minimal. The measured features are the sizes, ellipticities, and orientations of bars, rings, ringlenses, and lenses. Measured in a similar manner are also barlenses (lens-like structures embedded in the bars), which are not lenses in the usual sense, being rather the more face-on counterparts of the boxy/peanut structures in the edge-on view. In addition, pitch angles of spiral arm segments are measured for those galaxies where they can be reliably traced. More than one pitch angle may appear for a single galaxy. All measurements are made in a human- supervised manner so that attention is paid to each galaxy. We create a catalogue of morphological features in the complete S4G. We used isophotal analysis, unsharp masking, and fitting ellipses to measured structures. We find that the sizes of the inner rings and lenses normalized to barlength correlate with the galaxy mass: the normalized sizes increase toward the less massive galaxies; it has been suggested that this is related to the larger dark matter content in the bar region in these systems. Bars in the low mass galaxies are also less concentrated, likely to be connected to the mass cut-off in the appearance of the nuclear rings and lenses. We also show observational evidence that barlenses indeed form part of the bar, and that a large fraction of the inner lenses in the non-barred galaxies could be former barlenses in which the thin outer bar component has dissolved.
162. Catalogue of galaxies observed with Hectospec
ID:
ivo://CDS.VizieR/J/ApJS/256/4
Title:
Catalogue of galaxies observed with Hectospec
Short Name:
J/ApJS/256/4
Date:
03 Dec 2021 00:37:37
Publisher:
CDS
Description:
We present redshifts for 2753 low-redshift (0.05~<z_spec_~<0.5) galaxies with 18<=r<=22 obtained with Hectospec at the Multi-Mirror Telescope (MMT). The observations targeted the XMM-LSS, ELAIS-N1 and DEEP2-3 fields, each of which covers ~1deg^2^. These fields are also part of the recently completed CFHT Large Area U-band Deep Survey (CLAUDS) and on-going Hyper Suprime-Cam deep fields surveys. The efficiency of our technique for selecting low-redshift galaxies is confirmed by the redshift distribution of our sources. In addition to redshifts, these high S/N spectra are used to measure ages, metallicities, and nuclear activity levels. In combination with the photometric catalogue in u, g, r, i, z, y down to 27 AB mag, we are able to study the galaxy population down to stellar masses of ~10^8^M_{sun}_ . This paper presents the observation strategy, the reduction procedure and properties of the galaxy sample. The catalog can be accessed through the webpage of this survey http://mips.as.arizona.edu/~cnaw/Faint_Low_z/.
163. Catalogue of HI maps of galaxies. I.
ID:
ivo://CDS.VizieR/J/A+AS/131/73
Title:
Catalogue of HI maps of galaxies. I.
Short Name:
J/A+AS/131/73
Date:
21 Oct 2021
Publisher:
CDS
Description:
A catalogue is presented of galaxies having large-scale observations in the HI line. This catalogue collects from the literature the information that characterizes the observations in the 21-cm line and the way that these data were presented by means of maps, graphics and tables, for showing the distribution and kinematics of the gas. It contains furthermore a measure of the HI extension that is detected at the level of the maximum sensitivity reached in the observations. This catalogue is intended as a guide for references on the HI maps published in the literature from 1953 to 1995 and is the basis for the analysis of the data presented in Paper II (Cat. <J/A+AS/131/77>).
164. Catalogue of HI maps of galaxies. II.
ID:
ivo://CDS.VizieR/J/A+AS/131/77
Title:
Catalogue of HI maps of galaxies. II.
Short Name:
J/A+AS/131/77
Date:
21 Oct 2021
Publisher:
CDS
Description:
We use some of the maps of the catalogue presented in Paper I (Cat. <J/A+AS/131/73>) to provide some evidence for global conditions that must be fulfilled by the galaxies to have extended hydrogen. For this purpose, we tried to find possible connections between the HI gas extension and other properties of the galaxies (morphological type, surface brightness, gas density, etc.). With isophotal hydrogen diameters of a large sample, we could observe that optically smaller galaxies seem to have greater relative HI extensions. By means of the relation with the apparent HI surface density, we found an expression that should provide a rough estimate of the gas extension. With respect to the dependence on morphological type, we could not find any significant correlation either for the real HI surface density or the relative gas extension. Nevertheless, whereas for spiral and irregular galaxies the real HI surface density exhibits a broad range of values, the values are rather lower for elliptical and S0 galaxies.
165. Catalogue of ISM content of normal galaxies
ID:
ivo://CDS.VizieR/J/A+A/405/5
Title:
Catalogue of ISM content of normal galaxies
Short Name:
J/A+A/405/5
Date:
21 Oct 2021
Publisher:
CDS
Description:
We have compiled a catalogue of the gas content for a sample of 1916 galaxies, considered to be a fair representation of normality. The definition of a normal galaxy adopted in this work implies that we have purposely excluded from the catalogue galaxies having distorted morphology (such as interaction bridges, tails or lopsidedness) and/or any signature of peculiar kinematics (such as polar rings, counterrotating disks or other decoupled components). In contrast, we have included systems hosting active galactic nuclei (AGN) in the catalogue. This catalogue revises previous compendia on the ISM content of galaxies published by Bregman et al. (1992ApJ...387..484B) and Casoli et al. (1998A&A...331..451C), and compiles data available in the literature from several small samples of galaxies. Masses for warm dust, atomic and molecular gas, as well as X-ray luminosities have been converted to a uniform distance scale taken from the Catalogue of Principal Galaxies (PGC). We have used two different normalization factors to explore the variation of the gas content along the Hubble sequence: the blue luminosity (LB) and the square of linear diameter (D_25_^2^). Our catalogue significantly improves the statistics of previous reference catalogues and can be used in future studies to define a template ISM content for normal galaxies along the Hubble sequence.
166. Catalogue of Isolated Galaxies
ID:
ivo://CDS.VizieR/VII/82A
Title:
Catalogue of Isolated Galaxies
Short Name:
VII/82A
Date:
21 Oct 2021
Publisher:
CDS
Description:
The catalog of isolated galaxies is defined on the basis of the Palomar Sky Survey. It contains 1051 isolated galaxies with apparent magnitudes brighter than 15.7 and north of declination -3{deg}. Compared to the original version published in 1973 (Comm. Special Astrophys. Obs. of USSR, No. 8), new data about the morphological types, the isolation class, and the radial velocities have been added. The catalog includes running numbers for the galaxies, equatorial coordinates, isolation classes, apparent magnitudes, morphological types, major axes, axial ratios, and radial velocities.
167. Catalogue of Markarian Galaxies
ID:
ivo://CDS.VizieR/VII/61A
Title:
Catalogue of Markarian Galaxies
Short Name:
VII/61A
Date:
21 Oct 2021
Publisher:
CDS
Description:
Markarian galaxies have a moderate to strong ultraviolet continuum as detected by an objective-prism survey at Byurakan Observatory from 1965 to 1978. The survey was done with a 40-inch Schmidt telescope with a dispersion of 2500 angstroms/millimeter at H-alpha. The catalog contains no galaxies brighter than mag 13.0 or fainter than mag 17.5. The catalog fields are Markarian Identification number; S(eyfert) or Q(uasar) flag; cross identifications to other catalogs; B1950 positions; major and minor axis (arcsec); magnitude and spectral types, including a code for the strength of the UV continuum. This catalogue is superseded by the First Byurakan Survey (see the "See Also" section below) The original documentation was by Robert S. Hill and Lee E. Brotzman in the "adc.doc" file (From the CD-ROM "Selected Astronomical Catalogs" Vol. 1 (1992), directory "nonstell/galaxies/mkn")
168. Catalogue of 2810 nearby galaxies
ID:
ivo://CDS.VizieR/VII/98A
Title:
Catalogue of 2810 nearby galaxies
Short Name:
VII/98A
Date:
21 Oct 2021
Publisher:
CDS
Description:
(no description available)
169. Catalogue of Principal Galaxies (PGC)
ID:
ivo://CDS.VizieR/VII/119
Title:
Catalogue of Principal Galaxies (PGC)
Short Name:
VII/119
Date:
21 Oct 2021
Publisher:
CDS
Description:
This "catalog of principal galaxies" constitutes the basis of the "Third Reference Catalogue of Bright Galaxies" (RC3). It lists equatorial coordinates for the equinoxes 1950 and 2000 and cross identifications for 73197 galaxies. Of the 73197 galaxies, 40932 have coordinates with standard deviations of less than ten arcsec. Listed are 131,601 names from the 38 most common sources. These data are given when available: morphological descriptions, apparent major and minor axes, apparent magnitudes, radial velocities, and position angles.
170. Catalogue of Southern Peculiar Galaxies and Associations
ID:
ivo://CDS.VizieR/VII/170
Title:
Catalogue of Southern Peculiar Galaxies and Associations
Short Name:
VII/170
Date:
21 Oct 2021
Publisher:
CDS
Description:
This "Catalogue of Southern Peculiar Galaxies and Associations" is a complete and detailed catalogue of all the most interesting galaxies and most striking apparent associations of galaxies in the Southern sky. The printed catalogue is made of two volumes: Volume I which lists the Peculiar Galaxies, and Volume II which contains photographs of galaxies which are representative of the various Categories used in the Classification scheme presented in Volume I.

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