Bibliography

[1]P. B. Stetson. DAOPHOT - A computer program for crowded-field stellar photometry. PASP, 99:191–222, March 1987. doi:10.1086/131977.
[2]G. S. Da Costa. Basic Photometry Techniques. In S. B. Howell, editor, Astronomical CCD Observing and Reduction Techniques, volume 23 of Astronomical Society of the Pacific Conference Series, 90. 1992.
[3]E. Bertin and S. Arnouts. SExtractor: Software for source extraction. A&AS, 117:393–404, June 1996. doi:10.1051/aas:1996164.
[4]A. Stuart and K. Ord. Kendall’s Advanced Theory of Statistics: Volume 1: Distribution Theory. Number vol.~1~;vol.~1994 in Kendall’s Advanced Theory of Statistics. Wiley, 2009. ISBN 9780340614303. URL: https://books.google.fr/books?id=tW18thQWJQIC.
[5]J. F. Jarvis and J. A. Tyson. FOCAS - Faint Object Classification and Analysis System. AJ, 86:476–495, March 1981. doi:10.1086/112907.
[6]L. Infante. A faint object processing software - Description and testing. A&A, 183:177–184, September 1987.
[7]M. D. Richard and R. P. Lippmann. Neural network classifiers estimate bayesian a posteriori probabilities. Neural Computation, pages 461–483, 1991.
[8]M. Saerens, P. Latinne, and C. Decaestecker. Any reasonable cost function can be used for a posteriori probability approximation. IEEE Transactions on Neural Networks, 13(5):1204–1210, Sep 2002. doi:10.1109/TNN.2002.1031952.
[9]E. Bertin. SkyMaker: astronomical image simulations made easy. Mem.Soc.Ast.It, 80:422, 2009.
[10]A. F. J. Moffat. A Theoretical Investigation of Focal Stellar Images in the Photographic Emulsion and Application to Photographic Photometry. A&A, 3:455, December 1969.
[11]C. Marmo and E. Bertin. MissFITS and WeightWatcher: Two Optimised Tools for Managing FITS Data. In R. W. Argyle, P. S. Bunclark, and J. R. Lewis, editors, Astronomical Data Analysis Software and Systems XVII, volume 394 of Astronomical Society of the Pacific Conference Series, 619. August 2008.
[12]D. C. Wells, E. W. Greisen, and R. H. Harten. FITS - a Flexible Image Transport System. A&AS, 44:363, June 1981.
[13]A. S. Szalay, A. J. Connolly, and G. P. Szokoly. Simultaneous Multicolor Detection of Faint Galaxies in the Hubble Deep Field. AJ, 117:68–74, January 1999. arXiv:astro-ph/9811086, doi:10.1086/300689.
[14]E. Bertin, Y. Mellier, M. Radovich, G. Missonnier, P. Didelon, and B. Morin. The TERAPIX Pipeline. In D. A. Bohlender, D. Durand, and T. H. Handley, editors, Astronomical Data Analysis Software and Systems XI, volume 281 of Astronomical Society of the Pacific Conference Series, 228. 2002.
[15]C. E. Duchon. Lanczos Filtering in One and Two Dimensions. Journal of Applied Meteorology, 18:1016–1022, August 1979. doi:10.1175/1520-0450(1979)018<1016:LFIOAT>2.0.CO;2.
[16]C. Kanzow, N. Yamashita, and M. Fukushima. Levenberg-Marquardt methods with strong local convergence properties for solving nonlinear equations with convex constraints. Journal of Computational and Applied Mathematics, 172(2):375–397, 2004. URL: http://www.sciencedirect.com/science/article/pii/S0377042704001256, doi:http://dx.doi.org/10.1016/j.cam.2004.02.013.
[17]C. M. Hirata, R. Mandelbaum, U. Seljak, J. Guzik, N. Padmanabhan, C. Blake, J. Brinkmann, T. Budávari, A. Connolly, I. Csabai, R. Scranton, and A. S. Szalay. Galaxy-galaxy weak lensing in the Sloan Digital Sky Survey: intrinsic alignments and shear calibration errors. MNRAS, 353:529–549, September 2004. arXiv:astro-ph/0403255, doi:10.1111/j.1365-2966.2004.08090.x.
[18]P. Melchior and M. Viola. Means of confusion: how pixel noise affects shear estimates for weak gravitational lensing. MNRAS, 424:2757–2769, August 2012. arXiv:1204.5147, doi:10.1111/j.1365-2966.2012.21381.x.
[19]A. Refregier, T. Kacprzak, A. Amara, S. Bridle, and B. Rowe. Noise bias in weak lensing shape measurements. MNRAS, 425:1951–1957, September 2012. arXiv:1203.5050, doi:10.1111/j.1365-2966.2012.21483.x.
[20]T. Kacprzak, J. Zuntz, B. Rowe, S. Bridle, A. Refregier, A. Amara, L. Voigt, and M. Hirsch. Measurement and calibration of noise bias in weak lensing galaxy shape estimation. MNRAS, 427:2711–2722, December 2012. arXiv:1203.5049, doi:10.1111/j.1365-2966.2012.21622.x.
[21]M.I.A. Lourakis. Levmar: levenberg-marquardt nonlinear least squares algorithms in C/C++. 2004. URL: http://www.ics.forth.gr/~lourakis/levmar/.
[22]C. Broyden. A class of methods for solving nonlinear simultaneous equations. Mathematics of Computation, 19:577–593, 1965.
[23]J. L. Sérsic. Atlas de Galaxias Australes. Cordoba, Argentina: Observatorio Astronomico, 1968, 1968.
[24]L. Ciotti and G. Bertin. Analytical properties of the R^(1/m) law. A&A, 352:447–451, December 1999. arXiv:astro-ph/9911078.
[25]J. J. Mohr, R. Armstrong, E. Bertin, G. Daues, S. Desai, M. Gower, R. Gruendl, W. Hanlon, N. Kuropatkin, H. Lin, J. Marriner, D. Petravic, I. Sevilla, M. Swanson, T. Tomashek, D. Tucker, and B. Yanny. The Dark Energy Survey data processing and calibration system. In Software and Cyberinfrastructure for Astronomy II, volume 8451 of Proc. SPIE, 84510D. September 2012. arXiv:1207.3189, doi:10.1117/12.926785.
[26]S. Desai, R. Armstrong, J. J. Mohr, D. R. Semler, J. Liu, E. Bertin, S. S. Allam, W. A. Barkhouse, G. Bazin, E. J. Buckley-Geer, M. C. Cooper, S. M. Hansen, F. W. High, H. Lin, Y.-T. Lin, C.-C. Ngeow, A. Rest, J. Song, D. Tucker, and A. Zenteno. The Blanco Cosmology Survey: Data Acquisition, Processing, Calibration, Quality Diagnostics, and Data Release. ApJ, 757:83, September 2012. arXiv:1204.1210, doi:10.1088/0004-637X/757/1/83.
[27]H. Bouy, E. Bertin, E. Moraux, J.-C. Cuillandre, J. Bouvier, D. Barrado, E. Solano, and A. Bayo. Dynamical analysis of nearby clusters. Automated astrometry from the ground: precision proper motions over a wide field. A&A, 554:A101, June 2013. arXiv:1306.4446, doi:10.1051/0004-6361/201220748.
[28]N. Pogson. Magnitudes of Thirty-six of the Minor Planets for the first day of each month of the year 1857. MNRAS, 17:12–15, November 1856.
[29]M. R. Calabretta and E. W. Greisen. Representations of celestial coordinates in FITS. A&A, 395:1077–1122, December 2002. arXiv:astro-ph/0207413, doi:10.1051/0004-6361:20021327.
[30]E. W. Greisen and M. R. Calabretta. Representations of world coordinates in FITS. A&A, 395:1061–1075, December 2002. arXiv:astro-ph/0207407, doi:10.1051/0004-6361:20021326.
[31]R. G. Kron. Photometry of a complete sample of faint galaxies. ApJS, 43:305–325, June 1980. doi:10.1086/190669.
[32]V. Petrosian. Surface brightness and evolution of galaxies. ApJL, 209:L1–L5, October 1976. doi:10.1086/182253.
[33]M. R. Blanton, J. Dalcanton, D. Eisenstein, J. Loveday, M. A. Strauss, M. SubbaRao, D. H. Weinberg, J. E. Anderson, Jr., J. Annis, N. A. Bahcall, M. Bernardi, J. Brinkmann, R. J. Brunner, S. Burles, L. Carey, F. J. Castander, A. J. Connolly, I. Csabai, M. Doi, D. Finkbeiner, S. Friedman, J. A. Frieman, M. Fukugita, J. E. Gunn, G. S. Hennessy, R. B. Hindsley, D. W. Hogg, T. Ichikawa, Ž. Ivezić, S. Kent, G. R. Knapp, D. Q. Lamb, R. F. Leger, D. C. Long, R. H. Lupton, T. A. McKay, A. Meiksin, A. Merelli, J. A. Munn, V. Narayanan, M. Newcomb, R. C. Nichol, S. Okamura, R. Owen, J. R. Pier, A. Pope, M. Postman, T. Quinn, C. M. Rockosi, D. J. Schlegel, D. P. Schneider, K. Shimasaku, W. A. Siegmund, S. Smee, Y. Snir, C. Stoughton, C. Stubbs, A. S. Szalay, G. P. Szokoly, A. R. Thakar, C. Tremonti, D. L. Tucker, A. Uomoto, D. Vanden Berk, M. S. Vogeley, P. Waddell, B. Yanny, N. Yasuda, and D. G. York. The Luminosity Function of Galaxies in SDSS Commissioning Data. AJ, 121:2358–2380, May 2001. arXiv:astro-ph/0012085, doi:10.1086/320405.
[34]N. Yasuda, M. Fukugita, V. K. Narayanan, R. H. Lupton, I. Strateva, M. A. Strauss, Ž. Ivezić, R. S. J. Kim, D. W. Hogg, D. H. Weinberg, K. Shimasaku, J. Loveday, J. Annis, N. A. Bahcall, M. Blanton, J. Brinkmann, R. J. Brunner, A. J. Connolly, I. Csabai, M. Doi, M. Hamabe, S.-I. Ichikawa, T. Ichikawa, D. E. Johnston, G. R. Knapp, P. Z. Kunszt, D. Q. Lamb, T. A. McKay, J. A. Munn, R. C. Nichol, S. Okamura, D. P. Schneider, G. P. Szokoly, M. S. Vogeley, M. Watanabe, and D. G. York. Galaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data. AJ, 122:1104–1124, September 2001. arXiv:astro-ph/0105545, doi:10.1086/322093.
[35]E. Bertin. Photométrie automatique de galaxies et contraintes sur leur évolution récente. PhD thesis, Université Paris VI, June 1996.
[36]R. S. Stobie. Application of moments to the analysis of panoramic astronomical photographs. In D. A. Elliott, editor, Conference on Applications of Digital Image Processing to Astronomy, volume 264 of Proc. SPIE, 208–212. 1980. doi:10.1117/12.959806.
[37]S. J. Maddox, G. Efstathiou, and W. J. Sutherland. The APM Galaxy Survey - Part Two - Photometric Corrections. MNRAS, 246:433, October 1990.