The Extended Chandra Deep Field-South Survey

Primary Research Papers

• The 2 Ms Chandra Deep Field-North Survey and the 250 ks Extended Chandra Deep Field-South Survey: Improved Point-Source Catalogs
• Additional data products - Event files, images, exposure/background/sensitivity maps, etc. (tar file; machine readable)

Y.Q. Xue, B. Luo, W.N. Brandt, D.M. Alexander, F.E. Bauer, B.D. Lehmer, G. Yang, 2016, ApJS, 224, 15

• The Extended Chandra Deep Field-South Survey: Optical Spectroscopy of Faint X-ray Sources with the VLT and Keck
• Catalogs and reduced spectra

J.D. Silverman, V. Mainieri, M. Salvato, G. Hasinger, J. Bergeron, P. Capak, G. Szokoly, A. Finoguenov, R. Gilli, P. Rosati, P. Tozzi, C. Vignali, D.M. Alexander, W.N. Brandt, B.D. Lehmer, B. Luo, D. Rafferty, Y.Q. Xue, I. Balestra, F.E. Bauer, M. Brusa, A. Comastri, J. Kartaltepe, A.M. Koekemoer, T. Miyaji, D.P. Schneider, E. Treister, L. Wisotski, M. Schramm, 2010, ApJS, 191, 124

• Discovery of the Most-Distant Double-Peaked Emitter at z = 1.369

B. Luo, W.N. Brandt, J.D. Silverman, I.V. Strateva, F.E. Bauer, P. Capak, J. Kartaltepe, B.D. Lehmer, V. Mainieri, M. Salvato, G. Szokoly, D.P. Schneider, C. Vignali, 2009, ApJ, 695, 1227

• Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies Using X-ray Emission: Results from the Chandra Deep Fields
• Table 1 - Properties of X-ray detected late-type galaxies (ASCII; machine readable)
• Table 2 - Stacked mean properties of late-type galaxies (ASCII; machine readable)
• Supplementary Table - Properties of the utilized late-type galaxies (ASCII; machine readable)

B.D. Lehmer, W.N. Brandt, D.M. Alexander, E.F. Bell, A.E. Hornschemeier, D.H. McIntosh, F.E. Bauer, R. Gilli, V. Mainieri, D.P. Schneider, J.D. Silverman, A.T. Steffen, P. Tozzi, C. Wolf, 2008, ApJ, 681, 1163

• The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large-Scale Structures

J.D. Silverman, V. Mainieri, B.D. Lehmer, D.M. Alexander, F.E. Bauer, J. Bergeron, W.N. Brandt, R. Gilli, G. Hasinger, D.P. Schneider, P. Tozzi, C. Vignali, A.M. Koekemoer, T. Miyaji, P. Popesso, P. Rosati, G. Szokoly, 2008, 675, 1025

• The X-ray Evolution of Early-Type Galaxies in the Extended Chandra Deep Field-South

B.D. Lehmer, W.N. Brandt, D.M. Alexander, E.F. Bell, D.H. McIntosh, F.E. Bauer, G. Hasinger, V. Mainieri, T. Miyaji, D.P. Schneider, A.T. Steffen, 2007, ApJ, 657, 681

• The X-ray-to-Optical Properties of Optically Selected Active Galaxies Over Wide Luminosity and Redshift Ranges

A.T. Steffen, I. Strateva, W.N. Brandt, D.M. Alexander, A.M. Koekemoer, B.D. Lehmer, D.P. Schneider, C. Vignali, 2006, AJ, 131, 2826

• The Properties and Redshift Evolution of Intermediate-Luminosity Off-Nuclear X-ray Sources in the Chandra Deep Fields

B.D. Lehmer, W.N. Brandt, A.E. Hornschemeier, D.M. Alexander, F.E. Bauer, A.M. Koekemoer, D.P. Schneider, A.T. Steffen, 2006, AJ, 131, 2394

• The Extended Chandra Deep Field-South Survey. Chandra Point-Source Catalogs
• Additional data products

B.D. Lehmer, W.N. Brandt, D.M. Alexander, F.E. Bauer, D.P. Schneider, P. Tozzi, J. Bergeron, G.P. Garmire, R. Giacconi, R. Gilli, G. Hasinger, A.E. Hornschemeier, A.M. Koekemoer, V. Mainieri, T. Miyaji, M. Nonino, P. Rosati, J.D. Silverman, G. Szokoly, C. Vignali, 2005, ApJS, 161, 21

Other Relevant Papers Using the X-ray Data

• The LABOCA Survey of the Extended Chandra Deep Field-South: Two Modes of Star Formation in Active Galactic Nucleus Hosts?
Lutz et al., 2010, ApJ, 712, 1287

• A Submillimetre Galaxy at z = 4.76 in the LABOCA Survey of the Extended Chandra Deep Field-South
Coppin et al., 2009, MNRAS, 395, 1905

• The VLA Survey of the Chandra Deep Field-South. III. X-Ray Spectral Properties of Radio Sources
Tozzi et al., 2009, ApJ, 698, 740

Contact and Funding Information

Support for this work was partially provided by the National Aeronautics and Space Administration through Chandra Award Number GO4-5157 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060.

This material is partially based upon work supported by the National Science Foundation under Grant No. 9983783. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the authors and do not necessarily reflect the views of the National Science Foundation.