On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2

被引:18
作者
Nakazono, L. [1 ]
de Oliveira, C. Mendes [1 ]
Hirata, N. S. T. [2 ]
Jeram, S. [3 ]
Queiroz, C. [4 ]
Eikenberry, Stephen S. [3 ]
Gonzalez, A. H. [3 ]
Abramo, R. [4 ]
Overzier, R. [5 ]
Espadoto, M. [2 ]
Martinazzo, A. [2 ]
Sampedro, L. [1 ]
Herpich, F. R. [1 ]
Almeida-Fernandes, F. [1 ]
Werle, A. [1 ,6 ]
Barbosa, C. E. [1 ]
Sodre Jr, L. [1 ]
Lima, E., V [1 ]
Buzzo, M. L. [1 ]
Cortesi, A. [7 ]
Menendez-Delmestre, K. [7 ]
Akras, S. [8 ]
Alvarez-Candal, Alvaro [5 ,9 ,10 ]
Lopes, A. R. [5 ]
Telles, E. [5 ]
Schoenell, W. [11 ]
Kanaan, A. [12 ]
Ribeiro, T. [13 ]
机构
[1] U Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508900 Sao Paulo, SP, Brazil
[2] Inst Matemat & Estat USP, Dept Ciencia Comp, BR-05508090 Sao Paulo, SP, Brazil
[3] Univ Florida, Dept Astron, 211 Bryant Space Ctr, Gainesville, FL 32611 USA
[4] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, Rua Matao 1371, Sao Paulo, SP, Brazil
[5] Observatorio Nacl MCTIC, Rua Gen Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil
[6] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
[7] Univ Fed Rio de Janeiro, Observatorio Valongo, Ladeira Pedro Antonio 43, BR-20080090 Rio De Janeiro, RJ, Brazil
[8] Natl Observ Athens, Inst Astron Astrophys Space Applicat & Remote Sen, GR-15236 Penteli, Greece
[9] CSIC, Inst Astrofis Andalucia, Apt 3004, E-18080 Granada, Spain
[10] Univ Alicante, IUFACyT, E-03080 Alicante, Spain
[11] GMTO Corp, 465 N Halstead St,Suite 250, Pasadena, CA 91107 USA
[12] Univ Fed Santa Catarina, Dept Fis, BR-88040900 Florianopolis, SC, Brazil
[13] Natl Opt Astron Observ, POB 26732, Tucson, AZ 85726 USA
基金
巴西圣保罗研究基金会; 美国国家航空航天局; 美国安德鲁·梅隆基金会;
关键词
methods: data analysis; catalogues; surveys; stars: general; galaxies: general; quasars: general; DIGITAL-SKY-SURVEY; OSCILLATION SPECTROSCOPIC SURVEY; LUMINOSITY FUNCTION; CLASSIFICATION; SDSS; SELECTION; COLOR;
D O I
10.1093/mnras/stab1835
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that a 12-band filter system (5 Sloan-like and 7 narrow bands) allows better performance for object classification than the usual analysis based solely on broad bands (regardless of infrared information). Moreover, we show that our classification is robust against missing values. Using spectroscopically confirmed sources retrieved from the Sloan Digital Sky Survey DR16 and DR14Q, we train a random forest classifier with the 12 S-PLUS magnitudes + 4 morphological features. A second random forest classifier is trained with the addition of the W1 (3.4) and W2 (4.6) magnitudes from the Wide-field Infrared Survey Explorer (WISE). Forty-four percent of our catalogue have WISE counterparts and are provided with classification from both models. We achieve 95.76 percent (52.47 percent) of quasar purity, 95.88 percent (92.24 percent) of quasar completeness, 99.44 percent (98.17 percent) of star purity, 98.22 percent (78.56 percent) of star completeness, 98.04 percent (81.39 percent) of galaxy purity, and 98.8 percent (85.37 percent) of galaxy completeness for the first (second) classifier, for which the metrics were calculated on objects with (without) WISE counterpart. A total of 2926 787 objects that are not in our spectroscopic sample were labelled, obtaining 335 956 quasars, 1347 340 stars, and 1243 391 galaxies. From those, 7.4 percent, 76.0 percent, and 58.4 percent were classified with probabilities above 80 percent. The catalogue with classification and probabilities for Stripe 82 S-PLUS DR2 is available for download.
引用
收藏
页码:5847 / 5868
页数:22
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