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

Author:

Wright Angus H.ORCID,Kuijken KonradORCID,Hildebrandt HendrikORCID,Radovich MarioORCID,Bilicki Maciej,Dvornik Andrej,Getman Fedor,Heymans Catherine,Hoekstra Henk,Li Shun-ShengORCID,Miller Lance,Napolitano Nicola R.,Xia Qianli,Asgari Marika,Brescia MassimoORCID,Buddelmeijer HugoORCID,Burger PierreORCID,Castignani Gianluca,Cavuoti StefanoORCID,de Jong JelteORCID,Edge AlastairORCID,Giblin Benjamin,Giocoli CarloORCID,Harnois-Déraps Joachim,Jalan PriyankaORCID,Joachimi Benjamin,John William Anjitha,Joudaki Shahab,Kannawadi ArunORCID,Kaur GursharanjitORCID,La Barbera Francesco,Linke LailaORCID,Mahony ConstanceORCID,Maturi Matteo,Moscardini LauroORCID,Nakoneczny Szymon J.ORCID,Paolillo Maurizio,Porth LucasORCID,Puddu EmanuellaORCID,Reischke Robert,Schneider Peter,Sereno MauroORCID,Shan HuanYuan,Sifón Cristóbal,Stölzner Benjamin,Tröster Tilman,Valentijn EdwinORCID,van den Busch Jan Luca,Verdoes Kleijn GijsORCID,Wittje Anna,Yan ZiangORCID,Yao JiORCID,Yoon Mijin,Zhang Yun-HaoORCID

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 5σ limiting 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.

Funder

European Research Council

Deutsches Zentrum für Luft- und Raumfahrt

Deutsche Forschungsgemeinschaft

Royal Society

Imperial College London

INAF

Polish National Science Center

Polish Ministry of Science and Higher Education

Science and Technology Facilities Council

Max-Planck-Gesellschaft

Alexander von Humboldt-Stiftung

Nederlandse Organisatie voor Wetenschappelijk Onderzoek

Istituto Nazionale di Astrofisica

Royal Society of Edinburgh

Agencia Nacional de Investigacion y Desarrollo

National Natural Science Foundation of China

Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

Netherlands Research School for Astronomy

Samenwerkingsverband Noord-Nederland

China Postdoctoral Science Foundation

Shanghai Post-doctoral Excellence Program

European Southern Observatory

National Science Foundation

Publisher

EDP Sciences

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