Table 10
Statistics for the KiDZ spectroscopic sample.
Full compilation | Matched to KiDZ sources | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
Survey | Nspec | [ɀmin, ɀmax] | 〈ɀ〉 | NMAD(ɀ) | Nspec | [ɀmin, ɀmax] | 〈ɀ〉 | NMAD(ɀ) | 〈rauto〉 | Key reference |
VIPERS | 76519 | [0.008, 2.148] | 0.712 | 0.181 | 43 382 | [0.045, 2.148] | 0.713 | 0.177 | 22.6 | Scodeggio etal. (2018) |
G10_COSMOS | 23 545 | [0.007, 4.596] | 0.582 | 0.322 | 20 214 | [0.007, 4.596] | 0.583 | 0.324 | 22.4 | Davies et al. (2015) |
DEVILS | 18 213 | [0.004, 4.786] | 0.581 | 0.333 | 15 103 | [0.005, 4.786] | 0.569 | 0.333 | 21.4 | Davies et al. (2018) |
VVDS | 15 059 | [0.003, 4.540] | 0.609 | 0.295 | 12598 | [0.010, 4.116] | 0.609 | 0.295 | 22.6 | Le Fèvre et al. (2013) |
DEEP2 | 15 888 | [0.009, 2.161] | 0.957 | 0.227 | 11 889 | [0.009, 2.161] | 0.962 | 0.233 | 23.7 | Newman et al. (2013) |
ACES | 4 276 | [0.037, 2.838] | 0.592 | 0.250 | 4 157 | [0.037, 2.838] | 0.591 | 0.250 | 22.4 | Cooper et al. (2012) |
C3R2 | 4348 | [0.030, 4.503] | 1.014 | 0.517 | 3 132 | [0.030, 4.175] | 0.967 | 0.538 | 24.0 | Euclid Collaboration (2021) |
zCOSMOS | 3 496 | [0.006, 4.445] | 1.396 | 1.155 | 2585 | [0.006, 4.445] | 1.490 | 1.110 | 23.6 | priv. comm. (M. Salvato) |
DEIMOS | 4197 | [0.009, 6.604] | 1.272 | 0.421 | 2457 | [0.009, 4.654] | 1.003 | 0.381 | 23.5 | Hasinger et al. (2018) |
OZDES | 12511 | [0.002, 4.541] | 0.574 | 0.352 | 2288 | [0.008, 4.541] | 0.697 | 0.372 | 21.2 | Lidman et al. (2020) |
G15_Deep | 1840 | [0.006, 1.193] | 0.357 | 0.163 | 1840 | [0.006, 1.193] | 0.357 | 0.163 | 21.2 | Kafle et al. (2018) |
GAMA | 241 130 | [0.003, 3.870] | 0.234 | 0.115 | 1755 | [0.006, 0.729] | 0.217 | 0.103 | 19.0 | Driver et al. (2022) |
GOODS | 2517 | [0.002, 6.277] | 1.382 | 0.765 | 1 703 | [0.002, 4.029] | 1.187 | 0.644 | 23.8 | ESO compilation |
hCOSMOS | 1 081 | [0.012, 1.265] | 0.302 | 0.132 | 876 | [0.012, 1.265] | 0.303 | 0.132 | 20.1 | Damjanov et al. (2018) |
SDSS | 109 459 | [0.002, 1.002] | 0.369 | 0.251 | 525 | [0.004, 0.817] | 0.355 | 0.285 | 19.0 | Abolfathi et al. (2018) |
VANDELS | 1 701 | [0.309, 5.784] | 3.086 | 0.765 | 458 | [0.309, 4.537] | 2.346 | 0.875 | 24.5 | Garilli et al. (2021) |
FMOS_COSMOS | 383 | [0.969, 2.486] | 1.568 | 0.083 | 325 | [1.313, 2.486] | 1.568 | 0.080 | 24.1 | Silverman et al. (2015) |
WIGGLEZ | 55 076 | [0.002, 6.159] | 0.598 | 0.204 | 308 | [0.006, 1.776] | 0.586 | 0.190 | 21.6 | Parkinson et al. (2012) |
LEGA_C | 352 | [0.346, 1.085] | 0.798 | 0.155 | 302 | [0.519, 1.050] | 0.806 | 0.153 | 22.9 | van der Wel et al. (2016) |
VUDS | 331 | [0.098, 6.091] | 2.219 | 1.488 | 186 | [0.098, 4.161] | 2.003 | 1.294 | 24.7 | Le Fèvre et al. (2015) |
2dFLens | 43 177 | [0.004, 4.688] | 0.361 | 0.249 | 2 | [0.273, 0.336] | 0.304 | 0.046 | 18.4 | Blake et al. (2016) |
Notes. Sources and statistics of the spectroscopic redshift estimates contained within the full spectroscopic compilation used in KiDZ (‘Full Compilation’) and after matching to sources extracted from KiDZ imaging (including masking, ‘Matched to KiDZ sources’). The numbers in the Nspec column refer to samples with duplicates removed (both internally and between overlapping surveys). Statistics for each sample shown are the minimum and maximum redshift in the sample (ɀmin, ɀmax), the mean redshift of the sample (〈ɀ〉), and the NMAD scatter of the redshifts in the sample (NMAD(ɀ)). For each survey we provide a single key reference; additional relevant papers are provided in the main text.
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