CANDELS multi-wavelength catalogs : source detection and photometry in the Goods-South field
- Author
- Yicheng Guo, Henry C Ferguson, Mauro Giavalisco, Guillermo Barro, SP Willner, Matthew LN Ashby, Tomas Dahlen, Jennifer L Donley, Sandra M Faber, Adriano Fontana, Audrey Galametz, Andrea Grazian, Kuang-Han Huang, Dale D Kocevski, Anton M Koekemoer, David C Koo, Elizabeth J McGrath, Michael Peth, Mara Salvato, Stijn Wuyts, Marco Castellano, Asantha R Cooray, Mark E Dickinson, James S Dunlop, GG Fazio, Jonathan P Gardner, Eric Gawiser, Norman A Grogin, Nimish P Hathi, Li-Ting Hsu, Kyoung-Soo Lee, Ray A Lucas, Bahram Mobasher, Kirpal Nandra, Jeffery A Newman and Arjen van der Wel (UGent)
- Organization
- Abstract
- We present a UV to mid-infrared multi-wavelength catalog in the CANDELS/GOODS-S field, combining the newly obtained CANDELS HST/WFC3 F105W, F125W, and F160W data with existing public data. The catalog is based on source detection in the WFC3 F160W band. The F160W mosaic includes the data from CANDELS deep and wide observations as well as previous ERS and HUDF09 programs. The mosaic reaches a 5 sigma limiting depth (within an aperture of radius 0 ''.17) of 27.4, 28.2, and 29.7 AB for CANDELS wide, deep, and HUDF regions, respectively. The catalog contains 34,930 sources with the representative 50% completeness reaching 25.9, 26.6, and 28.1 AB in the F160W band for the three regions. In addition to WFC3 bands, the catalog also includes data from UV (U band from both CTIO/MOSAIC and VLT/VIMOS), optical (HST/ACS F435W, F606W, F775W, F814W, and F850LP), and infrared (HST/WFC3 F098M, VLT/ISAAC K s, VLT/HAWK-I K s, and Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 mu m) observations. The catalog is validated via stellar colors, comparison with other published catalogs, zero-point offsets determined from the best-fit templates of the spectral energy distribution of spectroscopically observed objects, and the accuracy of photometric redshifts. The catalog is able to detect unreddened star-forming (passive) galaxies with stellar mass of 10(10) M-circle dot at a 50% completeness level to z similar to 3.4 (2.8), 4.6 (3.2), and 7.0 (4.2) in the three regions. As an example of application, the catalog is used to select both star-forming and passive galaxies at z similar to 2-4 via the Balmer break. It is also used to study the color-magnitude diagram of galaxies at 0 < z < 4.
- Keywords
- ORIGINS DEEP SURVEY, SPECTRAL ENERGY-DISTRIBUTIONS, STAR-FORMATION, HISTORY, SIMILAR-TO 2, GMASS ULTRADEEP SPECTROSCOPY, EXTRAGALACTIC, LEGACY SURVEY, REST-FRAME ULTRAVIOLET, UV LUMINOSITY FUNCTION, HIGH-REDSHIFT GALAXIES, SPACE-TELESCOPE, catalogs, galaxies: high-redshift, galaxies: photometry, methods: data, analysis, techniques: image processing
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Citation
Please use this url to cite or link to this publication: http://hdl.handle.net/1854/LU-8572983
- MLA
- Guo, Yicheng, et al. “CANDELS Multi-Wavelength Catalogs : Source Detection and Photometry in the Goods-South Field.” ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, vol. 207, no. 2, 2013, doi:10.1088/0067-0049/207/2/24.
- APA
- Guo, Y., Ferguson, H. C., Giavalisco, M., Barro, G., Willner, S., Ashby, M. L., … van der Wel, A. (2013). CANDELS multi-wavelength catalogs : source detection and photometry in the Goods-South field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 207(2). https://doi.org/10.1088/0067-0049/207/2/24
- Chicago author-date
- Guo, Yicheng, Henry C Ferguson, Mauro Giavalisco, Guillermo Barro, SP Willner, Matthew LN Ashby, Tomas Dahlen, et al. 2013. “CANDELS Multi-Wavelength Catalogs : Source Detection and Photometry in the Goods-South Field.” ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 207 (2). https://doi.org/10.1088/0067-0049/207/2/24.
- Chicago author-date (all authors)
- Guo, Yicheng, Henry C Ferguson, Mauro Giavalisco, Guillermo Barro, SP Willner, Matthew LN Ashby, Tomas Dahlen, Jennifer L Donley, Sandra M Faber, Adriano Fontana, Audrey Galametz, Andrea Grazian, Kuang-Han Huang, Dale D Kocevski, Anton M Koekemoer, David C Koo, Elizabeth J McGrath, Michael Peth, Mara Salvato, Stijn Wuyts, Marco Castellano, Asantha R Cooray, Mark E Dickinson, James S Dunlop, GG Fazio, Jonathan P Gardner, Eric Gawiser, Norman A Grogin, Nimish P Hathi, Li-Ting Hsu, Kyoung-Soo Lee, Ray A Lucas, Bahram Mobasher, Kirpal Nandra, Jeffery A Newman, and Arjen van der Wel. 2013. “CANDELS Multi-Wavelength Catalogs : Source Detection and Photometry in the Goods-South Field.” ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 207 (2). doi:10.1088/0067-0049/207/2/24.
- Vancouver
- 1.Guo Y, Ferguson HC, Giavalisco M, Barro G, Willner S, Ashby ML, et al. CANDELS multi-wavelength catalogs : source detection and photometry in the Goods-South field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2013;207(2).
- IEEE
- [1]Y. Guo et al., “CANDELS multi-wavelength catalogs : source detection and photometry in the Goods-South field,” ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, vol. 207, no. 2, 2013.
@article{8572983, abstract = {{We present a UV to mid-infrared multi-wavelength catalog in the CANDELS/GOODS-S field, combining the newly obtained CANDELS HST/WFC3 F105W, F125W, and F160W data with existing public data. The catalog is based on source detection in the WFC3 F160W band. The F160W mosaic includes the data from CANDELS deep and wide observations as well as previous ERS and HUDF09 programs. The mosaic reaches a 5 sigma limiting depth (within an aperture of radius 0 ''.17) of 27.4, 28.2, and 29.7 AB for CANDELS wide, deep, and HUDF regions, respectively. The catalog contains 34,930 sources with the representative 50% completeness reaching 25.9, 26.6, and 28.1 AB in the F160W band for the three regions. In addition to WFC3 bands, the catalog also includes data from UV (U band from both CTIO/MOSAIC and VLT/VIMOS), optical (HST/ACS F435W, F606W, F775W, F814W, and F850LP), and infrared (HST/WFC3 F098M, VLT/ISAAC K s, VLT/HAWK-I K s, and Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 mu m) observations. The catalog is validated via stellar colors, comparison with other published catalogs, zero-point offsets determined from the best-fit templates of the spectral energy distribution of spectroscopically observed objects, and the accuracy of photometric redshifts. The catalog is able to detect unreddened star-forming (passive) galaxies with stellar mass of 10(10) M-circle dot at a 50% completeness level to z similar to 3.4 (2.8), 4.6 (3.2), and 7.0 (4.2) in the three regions. As an example of application, the catalog is used to select both star-forming and passive galaxies at z similar to 2-4 via the Balmer break. It is also used to study the color-magnitude diagram of galaxies at 0 < z < 4.}}, articleno = {{24}}, author = {{Guo, Yicheng and Ferguson, Henry C and Giavalisco, Mauro and Barro, Guillermo and Willner, SP and Ashby, Matthew LN and Dahlen, Tomas and Donley, Jennifer L and Faber, Sandra M and Fontana, Adriano and Galametz, Audrey and Grazian, Andrea and Huang, Kuang-Han and Kocevski, Dale D and Koekemoer, Anton M and Koo, David C and McGrath, Elizabeth J and Peth, Michael and Salvato, Mara and Wuyts, Stijn and Castellano, Marco and Cooray, Asantha R and Dickinson, Mark E and Dunlop, James S and Fazio, GG and Gardner, Jonathan P and Gawiser, Eric and Grogin, Norman A and Hathi, Nimish P and Hsu, Li-Ting and Lee, Kyoung-Soo and Lucas, Ray A and Mobasher, Bahram and Nandra, Kirpal and Newman, Jeffery A and van der Wel, Arjen}}, issn = {{0067-0049}}, journal = {{ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES}}, keywords = {{ORIGINS DEEP SURVEY,SPECTRAL ENERGY-DISTRIBUTIONS,STAR-FORMATION,HISTORY,SIMILAR-TO 2,GMASS ULTRADEEP SPECTROSCOPY,EXTRAGALACTIC,LEGACY SURVEY,REST-FRAME ULTRAVIOLET,UV LUMINOSITY FUNCTION,HIGH-REDSHIFT GALAXIES,SPACE-TELESCOPE,catalogs,galaxies: high-redshift,galaxies: photometry,methods: data,analysis,techniques: image processing}}, language = {{eng}}, number = {{2}}, pages = {{23}}, title = {{CANDELS multi-wavelength catalogs : source detection and photometry in the Goods-South field}}, url = {{http://doi.org/10.1088/0067-0049/207/2/24}}, volume = {{207}}, year = {{2013}}, }
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