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• W2398216083 abstract "We have developed an analytical method based on forward-modelling techniques to characterize the high-mass end of the red sequence (RS) galaxy population at redshift z ∼ 0.55, from the DR10 BOSS (Baryon Oscillation Spectroscopic Survey) CMASS spectroscopic sample, which comprises ∼600 000 galaxies. The method, which follows an unbinned maximum likelihood approach, allows the deconvolution of the intrinsic CMASS colour–colour–magnitude distributions from photometric errors and selection effects. This procedure requires modelling the covariance matrix for the i-band magnitude, g − r colour and r − i colour using Stripe 82 multi-epoch data. Our results indicate that the error-deconvolved intrinsic RS distribution is consistent, within the photometric uncertainties, with a single point (<0.05 mag) in the colour–colour plane at fixed magnitude, for a narrow redshift slice. We have computed the high-mass end (0.55Mi ≲ −22) of the 0.55i-band RS luminosity function (RS LF) in several redshift slices within the redshift range 0.52 < z < 0.63. In this narrow redshift range, the evolution of the RS LF is consistent, within the uncertainties in the modelling, with a passively evolving model with Φ* = (7.248 ± 0.204) × 10− 4 Mpc−3 mag−1, fading at a rate of 1.5 ± 0.4 mag per unit redshift. We report RS completeness as a function of magnitude and redshift in the CMASS sample, which will facilitate a variety of galaxy-evolution and clustering studies using BOSS. Our forward-modelling method lays the foundations for future studies using other dark-energy surveys like the Extended Baryon Oscillation Spectroscopic Survey or the Dark Energy Spectroscopic Instrument, which are affected by the same type of photometric blurring/selection effects." @default.
• W2398216083 created "2016-06-24" @default.
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• W2398216083 date "2016-06-09" @default.
• W2398216083 modified "2023-10-13" @default.
• W2398216083 title "The high-mass end of the red sequence at<i>z</i>∼ 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function" @default.
• W2398216083 cites W1791095791 @default.
• W2398216083 cites W1860273276 @default.
• W2398216083 cites W1881487679 @default.
• W2398216083 cites W1893350802 @default.
• W2398216083 cites W1900607984 @default.
• W2398216083 cites W1943306457 @default.
• W2398216083 cites W1963611021 @default.
• W2398216083 cites W1965543352 @default.
• W2398216083 cites W1976360590 @default.
• W2398216083 cites W1977280707 @default.
• W2398216083 cites W1978875836 @default.
• W2398216083 cites W1979742375 @default.
• W2398216083 cites W1981769908 @default.
• W2398216083 cites W1982330764 @default.
• W2398216083 cites W1982558330 @default.
• W2398216083 cites W1985370957 @default.
• W2398216083 cites W1986834411 @default.
• W2398216083 cites W1993993296 @default.
• W2398216083 cites W2012056991 @default.
• W2398216083 cites W2013330090 @default.
• W2398216083 cites W2024370579 @default.
• W2398216083 cites W2024409675 @default.
• W2398216083 cites W2031521127 @default.
• W2398216083 cites W2044324411 @default.
• W2398216083 cites W2060794086 @default.
• W2398216083 cites W2060864745 @default.
• W2398216083 cites W2063568047 @default.
• W2398216083 cites W2064911290 @default.
• W2398216083 cites W2072016033 @default.
• W2398216083 cites W2081198904 @default.
• W2398216083 cites W2082266584 @default.
• W2398216083 cites W2082592033 @default.
• W2398216083 cites W2084655795 @default.
• W2398216083 cites W2095917766 @default.
• W2398216083 cites W2097957963 @default.
• W2398216083 cites W2099901303 @default.
• W2398216083 cites W2102600871 @default.
• W2398216083 cites W2104403548 @default.
• W2398216083 cites W2106239882 @default.
• W2398216083 cites W2109510044 @default.
• W2398216083 cites W2112030812 @default.
• W2398216083 cites W2114163622 @default.
• W2398216083 cites W2120393071 @default.
• W2398216083 cites W2127497368 @default.
• W2398216083 cites W2128806658 @default.
• W2398216083 cites W2136644880 @default.
• W2398216083 cites W2137457078 @default.
• W2398216083 cites W2147875900 @default.
• W2398216083 cites W2150195330 @default.
• W2398216083 cites W2154300700 @default.
• W2398216083 cites W2154889989 @default.
• W2398216083 cites W2155148078 @default.
• W2398216083 cites W2155431150 @default.
• W2398216083 cites W2156305595 @default.
• W2398216083 cites W2156905179 @default.
• W2398216083 cites W2157544440 @default.
• W2398216083 cites W2157604520 @default.
• W2398216083 cites W2157917411 @default.
• W2398216083 cites W2159898631 @default.
• W2398216083 cites W2163933621 @default.
• W2398216083 cites W2167156940 @default.
• W2398216083 cites W2167481042 @default.
• W2398216083 cites W2170689655 @default.
• W2398216083 cites W2204578610 @default.
• W2398216083 cites W2253551740 @default.
• W2398216083 cites W2593311270 @default.
• W2398216083 cites W2963574165 @default.
• W2398216083 cites W3098640821 @default.
• W2398216083 cites W3099582894 @default.
• W2398216083 cites W3102795811 @default.
• W2398216083 cites W3103438512 @default.
• W2398216083 cites W3105631369 @default.
• W2398216083 cites W3105733428 @default.
• W2398216083 cites W3106026166 @default.
• W2398216083 cites W3106072945 @default.
• W2398216083 cites W3106167992 @default.
• W2398216083 cites W3106338086 @default.

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