Low Surface Brightness Galaxy catalogue selected from the alpha.40-SDSS DR7 Survey and Tully-Fisher relation

Abstract

We present a catalogue of an HI-selected sample of 1129 low surface brightness galaxies (LSBGs) searched from the alpha.40-SDSS DR7 survey. This sample, consisting of various types of galaxies in terms of luminosity and morphology, has extended the parameter space covered by the existing LSBG samples. Based on a subsample of 173 LSBGs which are selected from our entire LSBG sample to have the 2-horn shapes of the HI line profiles, minor-to-major axial ratios (b/a) less than 0.6 and signal-to-noise ratio (S/N) of HI detection greater than 6.5, we investigated the Tully-Fisher relation (TFr) of LSBGs in the optical B, g and r bands and near-infrared J, H and K bands as well. In optical bands, the LSBG subsample follows the fundamental TFr which was previously defined for normal spiral galaxies. In NIR bands, the TFrs for our LSBG subsample are slightly different from the TFrs for the normal bright galaxies. This might be due to the internal extinction issue. Furthermore, the mass-to-light ratio (M/L),disk scale length (h) and mass surface density (sigma) for our LSBG subsample were deduced from the optical TFr results. Compared with High Surface Brightness Galaxies(HSBGs), our LSBGs have higher M/L, larger h and lower sigma than HSBGs.

Accepted to be published in MNRAS

References in corpus (16)

• Forty-Seven Milky Way-Sized, Extremely Diffuse Galaxies in the Coma Cluster
• The Arecibo Legacy Fast ALFA Survey: The ALFALFA Extragalactic HI Source Catalog
• The structure of galactic disks: Studying late-type spiral galaxies using SDSS
• Scaling Relations of Spiral Galaxies
• Kinematics of the Local Universe XIII. 21-cm line measurements of 452 galaxies with the Nançay radiotelescope, JHK Tully-Fisher relation and preliminary maps of the peculiar velocity field
• The Tully-Fisher Relation and Its Residuals for a Broadly Selected Sample of Galaxies
• Baryonic Tully-Fisher Relation for Extremely Low Mass Galaxies
• Photometric Properties and Scaling Relations of Early Type Brightest Cluster Galaxies
• The Multi-Wavelength Tully-Fisher relation with spatially resolved HI kinematics
• Low Surface Brightness Galaxies selected from the 40% sky area of the ALFALFA HI survey.I.Sample and statistical properties
• The properties of the Malin 1 galaxy giant disk: A panchromatic view from the NGVS and GUViCS surveys
• The Tully-Fisher Relation of COLD GASS Galaxies
• An optical search for Low Surface Brightness Galaxies in the Arecibo HI Strip Survey
• Galaxy And Mass Assembly (GAMA): detection of low-surface-brightness galaxies from SDSS data
• An H$\alpha$ Imaging Survey of the Low-surface-brightness Galaxies Selected from the Fall Sky Region of the 40$\%$ ALFALFA \ion{H}{1} Survey
• Low Surface Brightness Galaxies around the HDF-S: II. Distances and volume densities

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