Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference

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dc.contributor.authorCluver, Michelle E
dc.contributor.authorKarademir, Geray S
dc.contributor.authorBlake, Chris
dc.contributor.authorTaylor, Edward N
dc.contributor.authorJarrett, Thomas H
dc.contributor.authorTriani, Dian P
dc.date.accessioned2023-06-07T12:38:54Z
dc.date.available2023-06-07T12:38:54Z
dc.date.issued2023
dc.description.abstractWe develop a framework for using clustering-based redshift inference (cluster-z ) to measure the evolving galaxy luminosity function (GLF) and galaxy stellar mass function (GSMF) using Wide-field Infrared Survey Explorer W1 (3.4 μm) mid-infrared photometry and positions. We use multiple reference sets from the Galaxy And Mass Assembly survey, Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey. Combining the resulting cluster-z s allows us to enlarge the study area, and by accounting for the specific properties of each reference set, making best use of each reference set to produce the best overall result.en_US
dc.identifier.citationKarademir, G.S., Taylor, E.N., Blake, C., Cluver, M.E., Jarrett, T.H. and Triani, D.P., 2023. Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference. Monthly Notices of the Royal Astronomical Society, 522(3), pp.3693-3709.en_US
dc.identifier.urihttps://doi.org/10.1093/mnras/stad1250
dc.identifier.urihttp://hdl.handle.net/10566/9066
dc.language.isoenen_US
dc.publisherMonthly Notices of the Royal Astronomical Societyen_US
dc.subjectGalaxies: distanceen_US
dc.subjectMethods: data analysisen_US
dc.subjectMethods: statisticalen_US
dc.subjectRedshiftsen_US
dc.subjectGalaxy luminosity function (GLF)en_US
dc.titleMeasurement of the evolving galaxy luminosity and mass function using clustering-based redshift inferenceen_US
dc.typeArticleen_US

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