WISE/DEIMOS Redshift Catalog, Version 2
收藏Mendeley Data2024-01-31 更新2024-06-27 收录
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https://figshare.com/articles/dataset/WISE_DEIMOS_Redshift_Catalog_Version_2/3860016
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Reanalysis of spectra used to generate the redshift catalog originally published in 2012 under DOI:10.1088/0004-6256/143/1/7, as described in a paper under DOI(to be added after paper passes peer review). Designation has ``NA" for serendipitous sources. ID is a unique integer assigned to each source in the catalog. Ra and Dec are the J2000 right ascension and declination of the primary target on the slit. W1targ is the W1 Vega magnitude used for target selection (``nan" if unavailable). TG is the target group (explained in the text). mask is the mask number, and it corresponds to the Field Number of Table 4. SlitNum is the slit number in the mask the source fell on. z is the Earth-centric redshift of the source (``nan" if no valid redshift could be determined); no correction for the motion of the sun, Earth's orbital motion, or the CMB dipole was made, but all redshifts were gathered on a single night, Universal Time 2010 September 14, using the Keck 2 telescope on Mauna Kea, Hawaii. z_err is the uncertainty in the redshift, as ascertained by the template correlation performed by SpecPro (``nan" if redshift invalid or a star). q_z is the quality code of the spectrum, explained in the text. class is the spectroscopic classification assigned to the source, one of: ``Star" for stars, ``Gal" for galaxy, ``QSO" for broad line quasar, ``Indet" for a source that had an indeterminate spectrum, ``Unseen" for sources that didn't produce an observable spectrum, and ``Lost" for sources that were lost to instrument constraints. SpecProTemplate is the name of the SpecPro template that matches the spectrum closest (``NA" for invalid sources). R is a flag for whether the source was ``real," that is, it corresponds to a non-artifact AllWISE source. SpecFeatures is a list of spectroscopic features listed in the specPro software that were identified, in increasing wavelength order (no distinction is made between emission and absorption features).
创建时间:
2024-01-31



