Hyperleda. I. Identification and designation of galaxies

By G. Paturel, C. Petit, P. Prugniel, G. Theureau, J. Rousseau, M. Brouty, P. Dubois, L. Cambrésy. 2003

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In Astronomy and Astrophysics

Citations in the corpus

On the correlations between galaxy properties and supermassive black hole mass (2011, background): “( 14 ): to ta lm ag ni tu de of th e bu lg e. (Paturel et al. 2003).”
BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics (2017, methodology): “We used the data from the Hyperleda catalogue (Paturel et al. 2003) and literature references (Cid Fernandes et al. 2004; GarciaRissmann et al. 2005; Ho et al. 2009; van den Bosch et al. 2015).”
Metallicity gradients in local field star-forming galaxies: insights on inflows, outflows, and the coevolution of gas, stars and metals (2015, background): “Inclination angles of WiFeS galaxies are dr wn from Hyperleda (Paturel et al. 2003), which assumes the classical Hubble formula (Hubble 1926).”
What is a cool-core cluster? a detailed analysis of the cores of the X-ray flux-limited HIFLUGCS cluster sample (2009, methodology): “We identified the BCGs from visual inspection of the R-band images of the Second-Epoch Digitized Sky survey (DSS2, see e.g.http://archive.stsci.edu/dss) and then extracted magnitudes and redshifts from NED, HyperLeda19 (Paturel et al. 2003) or the compilation by Andernach & Tago (s e Andernach et al”
The ATLAS3D project – III. A census of the stellar angular momentum within the effective radius of early‐type galaxies: unveiling the distribution of fast and slow rotators (2011, methodology): “8, we show the distribution of galaxies in the λR– diagram using the two main classes of Es (T < −3.5) and S0s (T ≥ −3.5, as defined in Paturel et al. 2003).”
Nearby supernova rates from the Lick Observatory Supernova Search – I. The methods and data base (2010, methodology): “Although on average the classifications from NED and HyperLeda are consistent with each other (the difference, using the numbering scheme in Table 1, is 0.15±0.69 for 11,754 galaxies that have classifications in both databases), there is a tendency for HyperLeda to put galaxies having an Scd classif”
Low luminosity Type II supernovae - II. Pointing towards moderate mass precursors (2014, methodology): “…which a Tully–Fisher distance is adopted, in all other cases the SN distances are estimated using the recessional velocity corrected for Local Group infall into the Virgo Cluster (vVir parameter from the HYPERLEDA data base,1 Paturel et al. 2003) assuming an Hubble constant H0 = 72 km s−1 Mpc−1.”
The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria (2010, methodology): “The few disagreements with HyperLeda could all be easily explained by the high quality of the multi-colour SDSS images, which allowed for a better detection of faint spiral structures.”
The Tully-Fisher relations of early-type spiral and S0 galaxies (2010, methodology): “We apply corrections for Galactic (AG) and internal (Ai) extinction in both bands using the Galactic dust maps of Schlegel et al. (1998) and the internal extinction correction presented in Bottinelli et al. (1995), as tabulated in HYPERLEDA (Paturel et al. 2003), both of which we transform to the ap”
A z = 0 Multiwavelength Galaxy Synthesis. I. A WISE and GALEX Atlas of Local Galaxies (2019, methodology): “This database is built around the Lyon/Meudon Extragalactic Database (LEDA, Paturel et al. 2003a,b; Makarov et al. 2014).”
Masses and scaling relations for nuclear star clusters, and their co-existence with central black holes (2016, neutral): “5 http://leda.univ-lyon1.fr (Paturel et al. 2003) We have therefore calculate M?,gal using the empirically calibrated M/L-galaxy colour relations of Bell et al. (2003).”
HyperLEDA. III. The catalogue of extragalactic distances (2014, background): “HyperLEDA (Paturel et al. 2003a,b) takes its roots in the LyonMeudon Extragalactic database (Paturel et al. 1988, LEDA), which was created in 1983, and in Hypercat, which started as the observational catalogue on kinematics of early-type galaxies (Prugniel & Simien 1996).”
X-ray coronae in simulations of disc galaxy formation (2010, methodology): “The obser- c© 2009 RAS, MNRAS 000, 1–21 vational data are the same in both panels; rotation velocities are inclination-corrected 21-cm measurements extracted from the HYPERLEDA database3 (Paturel et al. 2003).”
CALIFA : a diameter-selected sample for an integral field spectroscopy galaxy survey (2014, methodology): “Hyperleda makes available distance moduli which are corrected for Virgo-centric infall and we also derived distances from pure Hubble flow for comparison.”
Galaxy groups and clouds in the local (z∼ 0.01) Universe (2010, methodology): “We use the HyperLEDA1 (Paturel et al. 2003) and the NED2 databases as main sources of data on radial velocities, apparent magnitudes, morphological types and other parameters 1 http://leda.univ-lyon1.fr 2 http://nedwww.ipac.caltech.edu of galaxies.”