SFI++. II. A New I-Band Tully-Fisher Catalog, Derivation of Peculiar Velocities, and Data Set Properties

By C. Springob, Karen L. Masters, M. Haynes, R. Giovanelli, C. Marinoni. 2007

199 citations recorded by the source corpus.

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In Astronomy and Astrophysics

Citations in the corpus

The Arecibo Legacy Fast ALFA Survey: The ALFALFA Extragalactic H i Source Catalog (2018, methodology): “…with czcmb < 6000 km s −1, we use the local peculiar velocity model of Masters (2005), which is based in large part on the SFI++ catalog of galaxies (Springob et al. 2007) and results from analysis of the peculiar motions of galaxies, groups, and clusters, using a combination of primary distances…”
Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field (2014, methodology): “For the SFI++ subsets we use the distances as determined in Springob et al. (2007) which have not been corrected for Malmquist bias.”
Consistently large cosmic flows on scales of 100 h−1 Mpc: a challenge for the standard ΛCDM cosmology (2008, background): “The characteristic depth of the survey is 32 h−1 Mpc. (iv) SFI++ (Springob et al. 2007), based on the Tully–Fisher (TF) relation, is the largest and densest peculiar velocity survey considered here.”
THE ARECIBO LEGACY FAST ALFA SURVEY: THE α.40 H i SOURCE CATALOG, ITS CHARACTERISTICS AND THEIR IMPACT ON THE DERIVATION OF THE H i MASS FUNCTION (2011, methodology): “…czcmb < 6000 km s −1, we use the local universe peculiar velocity model of Masters (2005), which is based on data from the SFI++ catalog of galaxies (Springob et al. 2007) and results from analysis of the peculiar motions of galaxies, groups, and clusters, using a combination of primary distances…”
THE 2MASS REDSHIFT SURVEY—DESCRIPTION AND DATA RELEASE (2011, background): “25 to the SFI++ peculiar velocity survey (Masters et al. 2006; Springob et al. 2007a) to place constraints on the bias between galaxies and dark matter halos, as well as β = f(Ω)/b (where f is the rate of growth of structure and b is the bias factor) and σ8 (which measures the amplitude of the…”
A DIRECT MEASUREMENT OF THE BARYONIC MASS FUNCTION OF GALAXIES AND IMPLICATIONS FOR THE GALACTIC BARYON FRACTION (2012, background): “The triangles correspond to disc galaxies for which Mh was determined from their rotation speed (Geha et al. 2006; Pizagno et al. 2007; Springob et al. 2007).”
xCOLD GASS: The Complete IRAM 30 m Legacy Survey of Molecular Gas for Galaxy Evolution Studies (2017, methodology): “Properties of the spectral lines, such as central velocity and width, are measured using a custommade IDL interactive program following the technique described in e.g. Springob et al. (2007), Catinella et al. (2007) and Saintonge et al. (2011a).”
THE EXTRAGALACTIC DISTANCE DATABASE (2009, unknown): “— Photometry of NGC 3223.”
COSMICFLOWS-2: THE DATA (2013, methodology): “Before moving on to other methods we acknowledge and integrate a second important compendium of TFR distances, the SFI++ compilation(Springob et al. 2007).”
Galaxy groups and clouds in the local (z∼ 0.01) Universe (2010, background): “Recently, Abate & Erdoğdu (2009) analysed the peculiar velocity field for the 2MASS galaxies, using the SFI++ survey data (Springob et al. 2007), and concluded that in the Local universe with a characteristic scale of ∼ 6000 km s−1 the density of matter lies within the interval of Ωm = 0.09–0.23.”
GALAXIES IN ΛCDM WITH HALO ABUNDANCE MATCHING: LUMINOSITY–VELOCITY RELATION, BARYONIC MASS–VELOCITY RELATION, VELOCITY FUNCTION, AND CLUSTERING (2010, methodology): “In order to convert the I-band luminosities measured by Springob et al. (2007) to the r band, we cross-referenced their data with the sample of Pizagno et al. (2007) and used the median (r − I ) colors of the galaxies present in both catalogs.”
Local gravity versus local velocity: solutions for β and non-linear bias (2010, methodology): “We begin by drawing the published magnitudes, velocity widths and redshifts from Springob et al. (2007, 2009).”
The Sydney-AAO Multi-object Integral field spectrograph (2011, background): “The largest TFR samples (e.g. Springob et al. 2007) currently contain ≃ 5000 galaxies with either long-slit spectroscopy or spatially unresolved H I velocities.”
Erratum: From dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmology (2010, background): “Observational data for relatively bright galaxies from Springob et al. (2007) and for isolated dwarfs from Blanton et al. (2008) are shown by blue symbols.”
THE ARECIBO LEGACY FAST ALFA SURVEY. X. THE H i MASS FUNCTION AND FROM THE 40% ALFALFA SURVEY (2010, methodology): “This parametric multiattractor model, based on the SFI++ catalog of galaxies with Tully-Fisher distances (Springob et al. 2007), includes two attractors (Virgo and a Great Attractor) along with a dipole and quadrupole component.”
Cosmic flows on 100 h−1 Mpc scales: standardized minimum variance bulk flow, shear and octupole moments (2009, methodology): “Here we use the data from the corrected dataset (Springob et al. 2009) rather than from the erroneous one (Springob et al. 2007).”