Bibcode
Rowan-Robinson, M.; Babbedge, T.; Oliver, S.; Trichas, M.; Berta, S.; Lonsdale, C.; Smith, G.; Shupe, D.; Surace, J.; Arnouts, S.; Ilbert, O.; Fevre, O. L.; Afonso-Luis, A.; Perez-Fournon, I.; Hatziminaoglou, E.; Polletta, M.; Farrah, D.; Vaccari, M.
Referencia bibliográfica
VizieR On-line Data Catalog: II/290. Originally published in: 2008MNRAS.386..697R
Fecha de publicación:
11
2008
Número de citas
2
Número de citas referidas
1
Descripción
The SWIRE Photometric Redshift Catalogue consists of 1025119 sources,
split between the SWIRE fields as follows: EN1 (218117), EN2 (125364),
Lockman (229238), SWIRE-VVDS (34630), SWIRE-SXDS (55432), XMM-LSS
(excluding VVDS and SXDS) (212572), Chandra DFS (149766). It is
available via IRSA and also at http://astro.ic.ac.uk/~mrr/swirephotzcat
.
The areas from the SWIRE Survey in which we have optical photometry and
are able to derive photometric redshifts are as follows:
(1) 8.72deg2 of ELAIS-N1, in which we have five-band
(U'g'r'i'Z') photometry from the Wide Field Survey (WFS),
(2) 4.84deg2 of ELAIS-N2, in which we have five-band
(U'g'r'i'Z') photometry from the WFS,
(3) 7.53deg2 of the Lockman Hole, in which we have 3-band
photometry (g'r'i') from the SWIRE photometry program, with U-band
photometry in 1.24deg2,
(4) 4.56deg2 in Chandra Deep Field South (CDFS), in which we
have 3-band (g'r'i') photometry from the SWIRE photometry program,
(5) 6.97deg2 of XMM-LSS, in which we have five-band (UgriZ)
photometry from Pierre et al. (2007, Cat. J/MNRAS/382/279). In addition
within XMM we have 10-band photometry (ugrizUBVRI) from the VVDS program
(0.7deg2), and very deep five-band photometry (BVRi'z') in
1.12deg2 of the Subaru XMM Deep Survey (SXDS).
(1 data file).