A Catalog of Neighboring Galaxies

By I. Karachentsev, V. Karachentseva, W. Huchtmeier, Dmitry I. Makarov. 2004

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Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/eec554e3c22e6a956c42eb9ad2772ca6dbac9da3

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Citations in the corpus

Galaxy groups and clouds in the local (z∼ 0.01) Universe (2010, methodology): “Using the data of ‘A Catalog of Neighboring Galaxies’ (CNG) (Karachentsev et al. 2004), which presents individual distances to many galaxies with D < 10 Mpc, and indicates Galaxy groups in the Local universe 15 in the comments their membership in the nearby groups, we compared the populations of…”
Associations of Dwarf Galaxies (2006, background): “…galaxies that are beyond the traditional Local Group (taken to include Tucana and SagDIG at the periphery) but within 3 Mpc in the compilation by Karachentsev et al. (2004) or as updated by a few new objects and improved TRGB detection algorithms (Makarov et al. 2006; Karachentsev et al. 2006a).”
An Hα Imaging Survey of Galaxies in the Local 11 Mpc Volume (2004, background): “…(HST ) and groundbased telescopes, direct stellar distances are being obtained for large numbers of galaxies with distances within 5 Mpc (e.g., Karachentsev et al. 2004 and references therein; Tully et al. 2006), but they are available for only a handful of objects near the survey distance…”
THE NGC 404 NUCLEUS: STAR CLUSTER AND POSSIBLE INTERMEDIATE-MASS BLACK HOLE (2010, methodology): “— (a) TRGB measurement from Karachentsev et al. (2004), (b) at r < 200′′ from Tikhonov et al. (2003) corrected for foreground reddening, (c) for r < 200′′ from Baggett et al. (1998), (d) combining above values; we derive a slightly brighter bulge MI,0 = −18.20 in §3, (e) using M/LI = 1.28 from…”
The Masses of the Milky Way and Andromeda galaxies (2010, positive): “The distances of the M31 satellites are determined by the tip of the red giant branch method and have errors of ±30 kpc (see, e.g. McConnachie et al. 2005).”
Cosmic Dawn (CoDa): the first radiation-hydrodynamics simulation of reionization and galaxy formation in the Local Universe (2015, methodology): “In essence, the method takes as its input, galaxy observations of the local universe today: galaxy catalogs with distances and peculiar velocities, galaxy group catalogs, such as the MARKIII (Willick et al. 1997), SBF (Tonry et al. 2001) and the Karachentsev catalog (Karachentsev et al. 2004).”
GHASP: an Hα kinematic survey of spiral and irregular galaxies – V. Dark matter distribution in 36 nearby spiral galaxies (2007, neutral): “Jam04=James et al. 2004 ; Kar04=Karachentsev et al. 2004 ; Koo06=Koopmann et al. 2006 ; Mou06=Moustakas & Kennicutt 2006 ; Saha06=Saha et al. 2006 ; Sha01=Shapley et al.2001 ; Sw02=Swaters & Balcells 2002.”
Molecular Hydrogen and Global Star Formation Relations in Galaxies (2007, background): “…for DDO 154 and, combined with the dark matter virial velocityV200 = 50km s−1 and concentrationc = 6, produce a rotational velocity of vcirc ≈ 50km s−1 (wherevcirc is defined as the maximum of rotation velocity profile) similar to the value ofvcirc ≈ 54km s−1 reported by Karachentsev et al. (2004).”
Advanced Camera for Surveys Imaging of 25 Galaxies in Nearby Groups and in the Field (2005, background): “By the definition of TI (Karachentsev et al. 2004), such a galaxy has a crossing Fig.”
GLADE: A galaxy catalogue for multimessenger searches in the advanced gravitational-wave detector era (2018, background): “GWGC is a catalogue of ∼50,000 galaxies and ∼150 globular clusters, that is a result of merging three existing catalogues: the Tully Nearby Galaxy Catalog (Tully 1987), the Catalog of Neighboring Galaxies (Karachentsev et al. 2004), and the V8k catalogue (Tully et al. 2009).”
UPDATED NEARBY GALAXY CATALOG (2013, methodology): “The summary of these data, increasing the number of galaxies in the LV up to N = 450 is reflected in the CNG catalog (Karachentsev et al. 2004).”
The Baryon Content of Extremely Low Mass Dwarf Galaxies (2006, background): “Using criteria such as surface brightness and irregularity, several authors have assembled large catalogs of nearby dwarf galaxies (Impey et al. 1996; Schombert et al. 2001; Hunter & Elmegreen 2004; Karachentsev et al. 2004).”
The Local Group and Other Neighboring Galaxy Groups (2005, methodology): “Basic observational data on 450 Local volume galaxies with distances less than 10 Mpc are presented in the Catalog of Neighboring Galaxies (Karachentsev et al. 2004).”
HyperLEDA. III. The catalogue of extragalactic distances (2014, background): “One of them is the Catalogue of the Local Volume galaxies2 (Karachentsev et al. 2004, 2013, hereafter LVG), which gives distances, velocities, and physical characteristics for galaxies within 11 Mpc (at present 869 galaxies).”
A NEW CLASS OF LUMINOUS TRANSIENTS AND A FIRST CENSUS OF THEIR MASSIVE STELLAR PROGENITORS (2008, background): “There is also an asymmetry between the rate of discovery in the northern and the southern sky in excess of a simple extrapolation of star formation from the catalog of Karachentsev et al. (2004).”
On Extending the Mass-Metallicity Relation of Galaxies by 2.5 Decades in Stellar Mass (2006, methodology): “A comparison between B and 4.5 m luminosities is shown in Figure 4, where B luminosities corrected for Galactic extinction are taken from Karachentsev et al. (2004).”
NGC 3741: the dark halo profile from the most extended rotation curve (2006, methodology): “Its distance (Karachentsev et al. 2004), estimated through the tip of the red giant branch, is 3.0 ± 0.3 Mpc, while Georgiev, Karachentsev & Tikhonov (1997) find a slightly higher value (3.5 ± 0.7 Mpc) from the brightest blue stars; unless stated otherwise, in this paper we adopt a distance of 3…”