Merging Galaxies in the SDSS EDR
arXiv:astro-ph/0312214 · doi:10.1086/381954
Abstract
We present a new catalog of merging galaxies obtained through an automated systematic search routine. The 1479 new pairs of merging galaxies were found in approximately 462 sq deg of the Sloan Digital Sky Survey Early Data Release (SDSS EDR; Stoughton et al. 2002) photometric data, and the pair catalog is complete for galaxies in the magnitude range 16.0 <= g* <= 20. The selection algorithm, implementing a variation on the original Karachentsev (1972) criteria, proved to be very efficient and fast. Merging galaxies were selected such that the inter-galaxy separations were less than the sum of the component galaxies' radii. We discuss the characteristics of the sample in terms of completeness, pair separation, and the Holmberg effect. We also present an online atlas of images for the SDSS EDR pairs obtained using the corrected frames from the SDSS EDR database. The atlas images also include the relevant data for each pair member. This catalog will be useful for conducting studies of the general characteristics of merging galaxies, their environments, and their component galaxies. The redshifts for a subset of the interacting and merging galaxies and the distribution of angular sizes for these systems indicate the SDSS provides a much deeper sample than almost any other wide-area catalog to date.
58 pages, which includes 15 figures and 6 tables. Figures 2, 8, 9, 10, 11, 13, and 14 are provided as JPEG files. For online atlas, see http://home.fnal.gov/~sallam/MergePair/ . Accepted for publication in AJ
References in corpus (11)
- Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
- Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data
- The u'g'r'i'z' Standard Star Network
- Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
- Astrometric Calibration of the Sloan Digital Sky Survey
- A photometricity and extinction monitor at the Apache Point Observatory
- Estimating Fixed Frame Galaxy Magnitudes in the SDSS
- Galaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data
- Galaxy Pairs in the 2dF Survey I. Effects of Interactions in the Field
- The SDSS Imaging Pipelines
- The Angular Clustering of Galaxy Pairs
Cited by in corpus (23)
- The Fourth Data Release of the Sloan Digital Sky Survey
- The Evolution of Galaxy Mergers and Morphology at z<1.2 in the Extended Groth Strip
- History of Galaxy Interactions and their Impact on Star Formation over the Last 7 Gyr from GEMS
- Early and Rapid Merging as a Formation Mechanism of Massive Galaxies: Empirical Constraints
- Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass
- The Luminosity Dependence of the Galaxy Merger Rate
- Combined Effects of Galaxy Interactions and Large-Scale Environment on Galaxy Properties
- The 8 o'clock Arc: A Serendipitous Discovery of a Strongly Lensed Lyman Break Galaxy in the SDSS DR4 Imaging Data
- The Sloan Bright Arcs Survey: Four Strongly Lensed Galaxies with Redshift >2
- The Sloan Bright Arcs Survey : Six Strongly Lensed Galaxies at z=0.4-1.4
- Infrared Properties of Close Pairs of Galaxies
- The Sloan Bright Arcs Survey : Discovery of Seven New Strongly Lensed Galaxies from z=0.66-2.94
- Spatial and luminosity distributions of galactic satellites
- Galaxy Collisions - Dawn of a New Era
- The DPOSS II compact group survey: first spectroscopically confirmed candidates
- LBT/ARGOS adaptive optics observations of z lensed galaxies
- The Differences of Star Formation History Between Merging Galaxies and Field Galaxies in the EDR of the SDSS
- Stellar populations of galaxies in the LAMOST spectral survey
- Very Large Array observations of the 8 o'clock arc lens system: Radio emission and a limit on the star-formation rate
- Evolution of the Frequency of Luminous (\geq L_V*) Close Galaxy Pairs at z < 1.2 in the COSMOS Field
- The Ly and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape
- A Search for Spectral Galaxy Pairs of Overlapping Galaxies based on Fuzzy Recognition
- Understanding the large inferred Einstein radii of observed low-mass galaxy clusters