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 Publish in OALib Journal ISSN: 2333-9721 APC: Only $99  Views Downloads  Relative Articles The Remarkable Central Structure of the Barred Galaxy NGC 1415 Photometric and proper motion study of neglected open cluster NGC 2215 The young age of the extremely metal-deficient blue compact dwarf galaxy SBS 1415+437 The Canada-UK Deep Submillimeter Survey VII: Optical and near-infrared identifications for the 14h field Optical identifications of High Frequency Peakers VSOP observation of the quasar PKS 2215+020: a new laboratory for core-jet physics at z=3.572 分子动力学模拟组分对Co1415-xAlx团簇结构特征的影响Composition dependence of the structure characteristics in Co1415-xAlx clusters from molecular dynamics simulations Spectroscopic and photometric studies of low-metallicity star-forming dwarf galaxies. III. SBS 1415+437 Keck Spectroscopy of Millisecond Pulsar J2215+5135: a Moderate-M_NS, High-Inclination Binary Multiple Identifications in Multi-Armed Bandits More... Physics 1995 # THE CANADA-FRANCE REDSHIFT SURVEY III: "Single Emission Line" Objects, Analysis of Repeat Observations, and Spectroscopic Identifications in the 1415+52 and 2215+00 Fields DOI: 10.1086/176557  Full-Text Cite this paper Abstract: This paper is one of a series describing the Canada-France Redshift Survey (CFRS). It is shown how the shape of the continuum around the emission line can be used to distinguish between [OII] 3727 at z > 0.76 and H$\alpha\$ at low redshift in spectra for which only a single isolated emission line is visible. Based on this, [OII] 3727 is most likely to be the emission line in most of the single emission line galaxies in the CFRS. The statistics of the repeated observations are analyzed to derive an empirical calibration of the reliability of the spectroscopic identifications in the CFRS, to determine how often additional observations could lead to the identification of an initially unidentified object and to provide an estimate of the internal velocity accuracy. Finally, the results of spectroscopic observations of 413 objects in the 1415+52 and 2215+00 CFRS survey fields are presented.

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