SIDESsides.bolshoi202ivo://lam.cesam/sides/q/bolshoi2022The CeSAM VO teamBéthermin, M.2025-05-28T15:56:37ZCeSAM VO teamLAM, 38 rue Frederic Joliot-Curie 13388 Marseille cedex 13cesam-vo@lam.frgalaxiestheoretical-modelsastronomical-simulations A simulation of the extragalactic sky including clustering based on
empirical prescriptions.2022arXiv220412827Bhttps://vo.lam.fr/tableinfo/sides.bolshoi2022SimulationResearchpySIDESInfraredMillimetersides SIDES A simulation of the extragalactic sky including clustering based on
empirical prescriptions.
sides.bolshoi2022 A simulation of the extragalactic sky including clustering based on
empirical prescriptions.5600000indexInternal identifiermeta.id;meta.mainlongindexedprimaryredshiftRedshiftsrc.redshiftdoubleindexednullableraSimulated Right Ascensiondegpos.eq.ra;meta.maindoubleindexednullabledecSimulated Declinationdegpos.eq.dec;meta.maindoubleindexednullablemhaloHost halo masssolMassphys.massdoubleindexednullablemstarStellar masssolMassphys.massdoubleindexednullableqflagQuenching flag (0: star-forming, 1: passive)meta.codeshortsfrStar Formation RatesolMass/yrphys.sfrdoubleindexednullableissbStaburst flag (0:normal, 1: starburst)meta.codeshortmuLensing magnificationarith.factordoublenullabledlumLuminosity distanceMpcpos.distancedoublenullableumeanIntensity of the radiation fieldphysdoublenullablelirInfrared luminositysolLumphys.luminosity;em.IRdoubleindexednullablelfirFar Infrared luminositysolLumphys.luminosity;em.IRdoublenullables2424 microns monochromatic flux densityJyphot.flux.density;em.IR.15-30umdoublenullables7070 microns monochromatic flux densityJyphot.flux.density;em.IR.60-100umdoublenullables100100 microns monochromatic flux densityJyphot.flux.density;em.IR.60-100umdoublenullables160160 microns monochromatic flux densityJyphot.flux.density;em.mm.1500-3000GHzdoublenullables250250 microns monochromatic flux densityJyphot.flux.density;em.mm.750-1500GHzdoublenullables350350 microns monochromatic flux densityJyphot.flux.density;em.mm.750-1500GHzdoublenullables500500 microns monochromatic flux densityJyphot.flux.density;em.mm.400-750GHzdoublenullables850850 microns monochromatic flux densityJyphot.flux;em.mm.200-400GHzdoublenullables11001100 microns monochromatic flux densityJyphot.flux.density;em.mm.200-400GHzdoublenullables20002000 microns monochromatic flux densityJyphot.flux.density;em.mm.100-200GHzdoublenullablesmips24MIPS 24 micron flux densityJyphot.flux.density;em.IR.15-30umdoublenullablespacs70PACS 70 micron flux densityJyphot.flux.density;em.IR.60-100umdoublenullablespacs100PACS 100 micron flux densityJyphot.flux.density;em.IR.60-100umdoublenullablespacs160PACS 160 micron flux densityJyphot.flux.density;em.mm.1500-3000GHzdoublenullablesspire250SPIRE 250 micron flux densityJyphot.flux.density;em.mm.750-1500GHzdoublenullablesspire350SPIRE 350 micron flux densityJyphot.flux.density;em.mm.750-1500GHzdoublenullablesspire500SPIRE 500 micron flux densityJyphot.flux.density;em.mm.400-750GHzdoublenullablesnika1200NIKA2 1200 micron flux densityJyphot.flux.density;em.mm.200-400GHzdoublenullablesnika2000NIKA2 2000 micron flux densityJyphot.flux.density;em.mm.100-200GHzdoublenullablelprimco10Pseudo luminosity of CO(1-0)K.km.s**-1.pc**2phys.luminosity;em.line.COdoublenullableico10Flux of the CO(1-0) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico21Flux of the CO(2-1) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico32Flux of the CO(3-2) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico43Flux of the CO(4-3) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico54Flux of the CO(5-4) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico65Flux of the CO(6-5) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico76Flux of the CO(7-6) lineJy.km.s**-1phot.flux;em.line.COdoublenullableico87Flux of the CO(8-7) lineJy.km.s**-1phot.flux;em.line.COdoublenullablelcii_lagacheLuminosity of [CII] line using the L18 relationsolLumphys.luminosity;em.linedoublenullableicii_lagacheFlux of [CII] line using the L18 relationJy.km.s**-1phot.flux;em.linedoublenullablelcii_de_loozeLuminosity of [CII] line using the DL14 relationsolLumphys.luminosity;em.linedoublenullableicii_de_loozeFlux of [CII] line using the DL14 relationJy.km.s**-1phot.flux;em.linedoublenullableici10Flux of [CI](1-0) lineJy.km.s**-1phot.flux;em.linedoublenullableici21Flux of [CI](2-1) lineJy.km.s**-1phot.flux;em.linedoublenullable