The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields

KiDS collaboration, Angus H. Wright, Konrad Kuijken, Hendrik Hildebrandt, Mario Radovich, Maciej Bilicki, Andrej Dvornik, Fedor Getman, Catherine Heymans, Henk Hoekstra, Shun Sheng Li, Lance Miller, Nicola R. Napolitano, Qianli Xia, Marika Asgari, Massimo Brescia, Hugo Buddelmeijer, Pierre Burger, Gianluca Castignani, Stefano CavuotiJelte De Jong, Alastair Edge, Benjamin Giblin, Carlo Giocoli, Joachim Harnois-Déraps, Priyanka Jalan, Benjamin Joachimi, Anjitha John William, Shahab Joudaki, Arun Kannawadi, Gursharanjit Kaur, Francesco La Barbera, Laila Linke, Constance Mahony, Matteo Maturi, Lauro Moscardini, Szymon J. Nakoneczny, Maurizio Paolillo, Lucas Porth, Emanuella Puddu, Robert Reischke, Peter Schneider, Mauro Sereno, Huanyuan Shan, Cristóbal Sifón, Benjamin Stölzner, Tilman Tröster, Edwin Valentijn, Jan Luca Van Den Busch, Gijs Verdoes Kleijn, Anna Wittje

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Abstract

We present the final data release of the Kilo-Degree Survey (KiDS-DR5), a public European Southern Observatory (ESO) wide-field imaging survey optimised for weak gravitational lensing studies. We combined matched-depth multi-wavelength observations from the VLT Survey Telescope and the VISTA Kilo-degree INfrared Galaxy (VIKING) survey to create a nine-band optical-to-near-infrared survey spanning 1347 deg2. The median r-band 5σlimiting magnitude is 24.8 with median seeing 0.7″. The main survey footprint includes 4 deg2 of overlap with existing deep spectroscopic surveys. We complemented these data in DR5 with a targeted campaign to secure an additional 23 deg2 of KiDS- and VIKING-like imaging over a range of additional deep spectroscopic survey fields. From these fields, we extracted a catalogue of 126 085 sources with both spectroscopic and photometric redshift information, which enables the robust calibration of photometric redshifts across the full survey footprint. In comparison to previous releases, DR5 represents a 34% areal extension and includes an i-band re-observation of the full footprint, thereby increasing the effective i-band depth by 0.4 magnitudes and enabling multi-epoch science. Our processed nine-band imaging, single- and multi-band catalogues with masks, and homogenised photometry and photometric redshifts can be accessed through the ESO Archive Science Portal.

Original languageEnglish
Article numberA170
Number of pages54
JournalAstronomy and Astrophysics
Volume686
DOIs
Publication statusPublished - Jun-2024

Keywords

  • Catalogs
  • Cosmology: observations
  • Galaxies: photometry
  • Gravitation
  • Gravitational lensing: weak
  • Surveys

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