J/PASP/130/H4203 Newly spectroscopically confirmed DB white dwarfs (Kong+, 2018)

Spectral feature extraction for DB white dwarfs through machine learning applied to new discoveries in the SDSS DR12 and DR14. Kong X., Luo A.-L., Li X.-R., Wang Y.-F., Li Y.-B., Zhao J.-K. <Publ. Astron. Soc. Pac., 130, h4203 (2018)> =2018PASP..130h4203K 2018PASP..130h4203K (SIMBAD/NED BibCode)
ADC_Keywords: Stars, white dwarf ; Radial velocities ; Effective temperatures ; Photometry, ultraviolet Keywords: catalogs - methods: data analysis - surveys - white dwarfs Abstract: Using a machine learning (ML) method, we mine DB white dwarfs (DBWDs) from the Sloan Digital Sky Survey (SDSS) Data Release (DR) 12 and DR14. The ML method consists of two parts: feature extraction and classification. The least absolute shrinkage and selection operator (LASSO) is used for the spectral feature extraction by comparing high quality data of a positive sample group with negative sample groups. In both the training and testing sets, the positive sample group is composed of a selection of 300 known DBWDs, while the negative sample groups are obtained from all types of SDSS spectra. In the space of the LASSO detected features, a support vector machine is then employed to build classifiers that are used to separate the DBWDs from the non-DBWDs for each individual type. Depending on the classifiers, the DBWD candidates are selected from the entire SDSS data set. After visual inspection, 2808 spectra (2029 objects) are spectroscopically confirmed. By checking the samples with the literature, there are 58 objects with 60 spectra that are newly identified, including a newly discovered AM CVn. Finally, we measure their effective temperatures (Teff), surface gravities (log g), and radial velocities, before compiling them into a catalog. Description: We have spectroscopically identified 1999 DBWDs in the SDSS DR12 and DR14, including 58 newly identified objects, using ML, i.e., LASSO and SVM. A total of 176 DB objects from the literature are not included in our catalog, Teff mostly varies around 11000K, and logg is fixed at 8.0. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table6.dat 155 2808 Newly spectroscopically confirmed DBWDs from SDSS DR12 and DR14 -------------------------------------------------------------------------------- See also: https://http://skyserver.sdss.org/DR12 : SDSS DR12 Home Page https://http://skyserver.sdss.org/DR14 : SDSS DR14 Home Page Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- SDSS SDSS object name (JHHMMSS.ss+DDMMSS.s) 21- 35 A15 --- P-M-F SDSS Plate number-Modified Julian date-Fiber 37- 42 A6 --- Type Classification of objects derived from ML method 44- 48 I5 km/s RVDB Radial velocity of each spectrum 50- 53 I4 km/s e_RVDB Radial velocity uncertainty of each spectrum 55- 59 I5 km/s RVM ?=-9999 Radial velocity of M companions 61- 65 I5 km/s e_RVM ?=-9999 Radial velocity uncertainty of M companions 67- 71 I5 K Teff ?=-9999 Effective temperature 73- 77 I5 K e_Teff ?=-9999 Effective temperature 78- 82 F5.2 [cm/s2] logg ?=-9.99 Surface gravity 84- 89 F6.3 [cm/s2] e_logg ?=-9.999 Surface gravity 91- 95 F5.1 mag FUV ?=-99.9 Magnitude of FUV from GALEX 97-100 F4.1 mag e_FUV ?=-9.9 Magnitude uncertainty of FUV from GALEX 103-107 F5.1 mag NUV ?=-99.9 Magnitude of NUV from GALEX 109-112 F4.1 mag e_NUV ?=-9.9 Magnitude uncertainty of NUV from GALEX 116-119 F4.1 --- S/N Median S/N from catalog of SDSS DR14 121-124 F4.2 Msun Mass ?=9.99 Obtained from Bergeron & Gilles Fontaine (2016) (1) 127-132 F6.1 Myr Age ?=-99.9 Obtained from Bergeron & Gilles Fontaine (2016) (1) 134-155 A22 --- Ref ID of the literature (2) -------------------------------------------------------------------------------- Note (1): Bergeron & Gilles Fontaine (2016, Synthetic Colors and Evolutionary Sequences of Hydrogen- and Helium-Atmosphere White Dwarfs http://www.astro.umontreal.ca/~bergeron/CoolingModels/) Note (2): References as follows: 0 = newly identified in this paper 1 = Kleinman et al. (2013ApJS..204....5K 2013ApJS..204....5K, Cat. J/ApJS/204/5) 2 = Koester & Kepler (2005A&A...432.1025K 2005A&A...432.1025K) 3 = Kepler et al. (2015MNRAS.446.3078V 2015MNRAS.446.3078V) 4 = Kepler et al. (2016MNRAS.455.3413K 2016MNRAS.455.3413K, Cat. J/MNRAS/455/3413) 5 = Atlee & Gould (2007ApJ...664...53A 2007ApJ...664...53A, Cat. J/ApJ/664/53) 6 = Eisenstein et al. (2006ApJS..167...40E 2006ApJS..167...40E, Cat. J/ApJS/167/40) 7 = Croom et al. (2004MNRAS.349.1397C 2004MNRAS.349.1397C, Cat. VII/241) 8 = Croom et al. (2001MNRAS.322L..29C 2001MNRAS.322L..29C, Cat. VII/223) 9 = Rebassa-Mansergas et al. (2010MNRAS.402..620R 2010MNRAS.402..620R, Cat. J/MNRAS/402/620) 10 = West et al. (2008AJ....135..785W 2008AJ....135..785W, Cat. J/AJ/135/785) 11 = Girven et al. (2011MNRAS.417.1210G 2011MNRAS.417.1210G, Cat. J/MNRAS/417/1210) 12 = Stepanian (2005RMxAA..41..155S 2005RMxAA..41..155S, Cat. VII/276) 13 = Bicay et al. (2000A&AS..147..169B 2000A&AS..147..169B, Cat. J/A+AS/147/169) 14 = Gentile Fusillo et al. (2015MNRAS.448.2260G 2015MNRAS.448.2260G, Cat. J/MNRAS/448/2260) 15 = Levitan et al. (2015MNRAS.446..391L 2015MNRAS.446..391L) 16 = Drake et al. (2014ApJS..213....9D 2014ApJS..213....9D, Cat. J/ApJS/213/9) 17 = Vennes et al. (2011MNRAS.410.2095V 2011MNRAS.410.2095V) 18 = Rau et al. (2010ApJ...708..456R 2010ApJ...708..456R) 19 = Carter et al. (2013MNRAS.429.2143C 2013MNRAS.429.2143C, Cat. J/MNRAS/429/2143) 20 = Jura & Xu (2012AJ....143....6J 2012AJ....143....6J) 21 = Girven et al. (2012ApJ...749..154G 2012ApJ...749..154G) 22 = Bergeron et al. (2011ApJ...737...28B 2011ApJ...737...28B) 23 = Zuckerman et al. (2010ApJ...722..725Z 2010ApJ...722..725Z) 24 = Voss et al. (2007A&A...470.1079V 2007A&A...470.1079V, Cat. J/A+A/470/1079) 25 = Koester et al. (2005A&A...432.1025K 2005A&A...432.1025K) 26 = McCook & Sion (1999ApJS..121....1M 1999ApJS..121....1M, Cat. B/wd ) 27 = Bradley (2000BaltA...9..485B 2000BaltA...9..485B) 28 = Bradley (1998BaltA...7..355B 1998BaltA...7..355B) 29 = Lepine & Shara (2005AJ....129.1483L 2005AJ....129.1483L, Cat. I/298) 30 = Stepanian et al. (2005RMxAA..41..155S 2005RMxAA..41..155S, Cat. VII/276) 31 = Stark & Wade (2003AJ....126.1455S 2003AJ....126.1455S, Cat. J/AJ/126/1455) 32 = Calcaferro et al. (2017A&A...600A..73C 2017A&A...600A..73C) 33 = Kleinman et al. (2004ApJ...607..426K 2004ApJ...607..426K, Cat. J/ApJ/607/426) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 09-Oct-2020
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line