Data Release 2 of S-PLUS: Accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters

被引：32

作者：

Almeida-Fernandes, F. ^{[1
]}

SamPedro, L. ^{[1
]}

Herpich, F. R. ^{[1
]}

Molino, A. ^{[1
]}

Barbosa, C. E. ^{[1
]}

Buzzo, M. L. ^{[1
]}

Overzier, R. A. ^{[2
]}

de Lima, E. V. R. ^{[1
]}

Nakazono, L. M., I ^{[1
]}

Oliveira Schwarz, G. B. ^{[3
]}

Perottoni, H. D. ^{[1
]}

Bolutavicius, G. F. ^{[1
]}

Gutierrez-Soto, L. A. ^{[1
]}

Santos-Silva, T. ^{[1
]}

Vitorelli, A. Z. ^{[1
]}

Werle, A. ^{[1
,4
,5
]}

Whitten, D. D. ^{[6
,7
]}

Costa Duarte, M., V ^{[1
]}

Bom, C. R. ^{[8
,9
]}

Coelho, P. ^{[1
]}

Sodre Jr, L. ^{[1
]}

Placco, V. M. ^{[10
]}

Teixeira, G. S. M. ^{[8
]}

Alonso-Garcia, J. ^{[11
,12
]}

Barbosa, C. L. ^{[13
]}

Beers, T. C. ^{[6
,7
]}

Bonatto, C. J. ^{[14
]}

Chies-Santos, A. L. ^{[14
,15
]}

Hartmann, E. A. ^{[14
]}

Lopes de Oliveira, R. ^{[2
,16
]}

Navarete, F. ^{[1
,17
]}

Kanaan, A. ^{[5
]}

Ribeiro, T. ^{[18
]}

Schoenell, W. ^{[19
]}

Mendes de Oliveira, C. ^{[1
]}

机构：

[1] Univ Sao Paulo, IAG, Dept Astron, Rua Matao 1226, BR-05509900 Sao Paulo, Brazil

[2] Observat Nacl MCTIC, R Gen Jose Cristino 77, BR-20921400 Rio De Janeiro, Brazil

[3] Univ Presbiteriana Mackenzie, R Consolacao 930, Sao Paulo, Brazil

[4] INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[5] Univ Fed Santa Catarina, Dept Fis, BR-88040900 Florianopolis, SC, Brazil

[6] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA

[7] Univ Notre Dame, JINA Ctr Evolut Elements, Notre Dame, IN 46556 USA

[8] Ctr Brasileir Pesquisas Fis, Rua Dr Xavier Sigaud 150, BR-22290180 Rio De Janeiro, RJ, Brazil

[9] Ctr Fed Educ Tecnol Celso Suckow Fonseca, Rodovia Mario Covas,Lote J2,Quadra J, BR-23810000 Itaguai, RJ, Brazil

[10] NSFs NOIRLab, Community Sci & Data Ctr, 950 N Cherry Ave, Tucson, AZ 85719 USA

[11] Univ Antofagasta, Ctr Astron CITEVA, Av Angamos 601, Antofagasta, Chile

[12] Millennium Inst Astrophys, Nuncio Monsenor Sotero Sanz 100,Of 104, Santiago, Chile

[13] Ctr Univ FEI, Dept Fis, Av Humberto Alencar Castelo Branco 3972, BR-09850901 Sao Bernardo Do Campo, SP, Brazil

[14] Univ Fed Rio Grande do Sul, Inst Fis, Dept Astron, Av Bento Gonalves 9500, Porto Alegre, RS, Brazil

[15] Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China

[16] Univ Fed Sergipe, Dept Fis, Av Marechal Rondon S-N, BR-49000000 Sao Cristovao, SE, Brazil

[17] SOAR Telescope NSFs NOIRLab, Avda Juan Cisternas 1500, La Serena 1700000, Chile

[18] Natl Opt Astron Observ, POB 26732, Tucson, AZ 85726 USA

[19] GMTO Corp, 465 N Halstead St,Suite 250, Pasadena, CA 91107 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2022年 / 511卷 / 03期

基金：

巴西圣保罗研究基金会;

关键词：

techniques: photometric; astronomical data bases: miscellaneous; catalogues; surveys; stars: general; galaxies: general; DIGITAL SKY SURVEY; ALL-SKY; STELLAR SPECTRA; STAR-CATALOG; EVOLUTION; CALIBRATION; SDSS; METALLICITY; !text type='JAVA']JAVA[!/text]LAMBRE; ISOCHRONES;

D O I：

10.1093/mnras/stac284

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing survey of similar to 9300 deg(2) in the southern sky in a 12-band photometric system. This paper presents the second data release (DR2) of S-PLUS, consisting of 514 tiles covering an area of 950 deg(2). The data has been fully calibrated using a new photometric calibration technique suitable for the new generation of wide-field multifilter surveys. This technique consists of a chi(2) minimization to fit synthetic stellar templates to already calibrated data from other surveys, eliminating the need for standard stars and reducing the survey duration by similar to 15 per cent. We compare the template-predicted and S-PLUS instrumental magnitudes to derive the photometric zero-points (ZPs). We show that these ZPs can be further refined by fitting the stellar templates to the 12 S-PLUS magnitudes, which better constrain the models by adding the narrow-band information. We use the STRIPE82 region to estimate ZP errors, which are less than or similar to 10 mmags for filters J0410, J0430, g, J0515, r, J0660, i, J0861 and z; less than or similar to 15 mmags for filter J0378; and less than or similar to 25 mmags for filters u and J0395. We describe the complete data flow of the S-PLUS/DR2 from observations to the final catalogues and present a brief characterization of the data. We show that, for a minimum signal-to-noise threshold of 5, the photometric depths of the DR2 range from 19.1 to 20.5 mag (measured in Petrosian apertures), depending on the filter. The S-PLUS DR2 can be accessed from the website: https://splus.cloud.

引用

页码：4590 / 4618

页数：29

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