The LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap I. The Spectroscopic Redshift Catalog
arXiv:1710.04301 · doi:10.3847/1538-4365/aa921e
Abstract
We present a spectroscopic redshift catalog from the LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap (SGC), which is designed to observe all sources (Galactic and extra-galactic) by using repeating observations with a limiting magnitude of in two fields. The project is mainly focusing on the completeness of LAMOST ExtraGAlactic Surveys (LEGAS) in the SGC, the deficiencies of source selection methods and the basic performance parameters of LAMOST telescope. In both fields, more than 95% of galaxies have been observed. A post-processing has been applied to LAMOST 1D spectrum to remove the majority of remaining sky background residuals. More than 10,000 spectra have been visually inspected to measure the redshift by using combinations of different emission/absorption features with uncertainty of . In total, there are 1528 redshifts (623 absorption and 905 emission line galaxies) in Field A and 1570 redshifts (569 absorption and 1001 emission line galaxies) in Field B have been measured. The results show that it is possible to derive redshift from low SNR galaxies with our post-processing and visual inspection. Our analysis also indicates that up to 1/4 of the input targets for a typical extra-galactic spectroscopic survey might be unreliable. The multi-wavelength data analysis shows that the majority of mid-infrared-detected absorption (91.3%) and emission line galaxies (93.3%) can be well separated by an empirical criterion of . Meanwhile, a fainter sequence paralleled to the main population of galaxies has been witnessed both in / and / diagrams, which could be the population of luminous dwarf galaxies but contaminated by the edge-on/highly inclined galaxies ().
19 pages, 14 figures, 2 MRT, accepted by ApJS
References in corpus (8)
- The Host Galaxies and Classification of Active Galactic Nuclei
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- A calibration of the relation between the abundance of close galaxy pairs and the rate of galaxy mergers
- Galaxy and Mass Assembly (GAMA): Exploring the WISE Cosmic Web in G12
- Catching Quenching Galaxies: The Nature of the WISE Infrared Transition Zone
- Morphological Dependence of MIR Properties of SDSS Galaxies in the Spitzer SWIRE Survey
- Clusters of galaxies: setting the stage
Cited by in corpus (4)
- Central velocity dispersion catalog of LAMOST-DR7 galaxies
- Two Portions of Sagittarius Stream in the LAMOST Complete Spectroscopic Survey of Pointing Area at Southern Galactic Cap
- Stellar populations of galaxies in the LAMOST spectral survey
- Applying Vision Transformers on Spectral Analysis of Astronomical Objects