Table information for 'sides.bolshoi2022'

General

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Resource Description: A simulation of the extragalactic sky including clustering based on empirical prescriptions.

For a list of all services and tables belonging to this table's resource, see Information on resource ' SIDES'

Citing this table

This table has an associated publication. If you use data from it, it may be appropriate to reference 2022arXiv220412827B (ADS BibTeX entry for the publication) either in addition to or instead of the service reference.

To cite the table as such, we suggest the following BibTeX entry:

@MISC{vo:sides_bolshoi202,
  year=2022,
  title={ {SIDES}},
  author={Béthermin, M.},
  url={https://vo.lam.fr/tableinfo/sides.bolshoi2022},
  howpublished={{VO} resource provided by the {CeSAM} Virtual Observatory Server}
}

Resource Documentation

Simulated Infrared Dusty Extragalactic Sky (SIDES) is a simulation of the extragalactic sky in the far-infrared and the millimetre domain, including clustering, based on dark-matter simulations and empirical prescriptions.

The initial paper presenting the method used to build the initial 2 deg² simulated catalogue and its application to continuum observables is Béthermin, Wu, Lagache, et al. (2017A&A...607A..89B). Please refer to this paper to introduce SIDES.

The new python version of the code (pySIDES, https://gitlab.lam.fr/mbethermin/sides-public-release) is described in Béthermin, Gkogkou, Van Cuyck, et al. (submitted, 2022arXiv220412827B). This paper also introduces the modelling of the main emission lines observables in the millimetre ([CII], CO, [CI]) and discusses the implication for line intensity mapping. Please refer to this paper if you use the line-related observables.

This resource contains the pySIDES catalogue (2022) created using the Bolshoi simulation. To get the 2017 catalogue and other products (simulated CONCERTO cubes), please visit SIDES web site (https://cesamsi.lam.fr/instance/sides/home).

Columns

Sorted alphabetically. [Sort by DB column index]

NameTable Head DescriptionUnitUCD
dec Dec Simulated Declination deg pos.eq.dec;meta.main
dlum dLum Luminosity distance Mpc pos.distance
ici10 i[CI](1-0) Flux of [CI](1-0) line Jy.km.s**-1 phot.flux;em.line
ici21 i[CII](2-1) Flux of [CI](2-1) line Jy.km.s**-1 phot.flux;em.line
icii_de_looze i[CII] de Looze Flux of [CII] line using the DL14 relation Jy.km.s**-1 phot.flux;em.line
icii_lagache i[CII] Lagache Flux of [CII] line using the L18 relation Jy.km.s**-1 phot.flux;em.line
ico10 iCO(1-0) Flux of the CO(1-0) line Jy.km.s**-1 phot.flux;em.line.CO
ico21 iCO(2-1) Flux of the CO(2-1) line Jy.km.s**-1 phot.flux;em.line.CO
ico32 iCO(3-2) Flux of the CO(3-2) line Jy.km.s**-1 phot.flux;em.line.CO
ico43 iCO(4-3) Flux of the CO(4-3) line Jy.km.s**-1 phot.flux;em.line.CO
ico54 iCO(5-4) Flux of the CO(5-4) line Jy.km.s**-1 phot.flux;em.line.CO
ico65 iCO(6-5) Flux of the CO(6-5) line Jy.km.s**-1 phot.flux;em.line.CO
ico76 iCO(7-6) Flux of the CO(7-6) line Jy.km.s**-1 phot.flux;em.line.CO
ico87 iCO(8-7) Flux of the CO(8-7) line Jy.km.s**-1 phot.flux;em.line.CO
index Index Internal identifier N/A meta.id;meta.main
issb isSB Staburst flag (0:normal, 1: starburst) N/A meta.code
lcii_de_looze L[CII] de Looze Luminosity of [CII] line using the DL14 relation solLum phys.luminosity;em.line
lcii_lagache L[CII] Lagache Luminosity of [CII] line using the L18 relation solLum phys.luminosity;em.line
lfir LFIR Far Infrared luminosity solLum phys.luminosity;em.IR
lir LIR Infrared luminosity solLum phys.luminosity;em.IR
lprimco10 Lprim CO(1-0) Pseudo luminosity of CO(1-0) K.km.s**-1.pc**2 phys.luminosity;em.line.CO
mhalo mHalo Host halo mass solMass phys.mass
mstar mStar Stellar mass solMass phys.mass
mu mu Lensing magnification N/A arith.factor
qflag qFlag Quenching flag (0: star-forming, 1: passive) N/A meta.code
ra RA Simulated Right Ascension deg pos.eq.ra;meta.main
redshift Redshift Redshift N/A src.redshift
s100 S100 100 microns monochromatic flux density Jy phot.flux.density;em.IR.60-100um
s1100 S1100 1100 microns monochromatic flux density Jy phot.flux.density;em.mm.200-400GHz
s160 S160 160 microns monochromatic flux density Jy phot.flux.density;em.mm.1500-3000GHz
s2000 S2000 2000 microns monochromatic flux density Jy phot.flux.density;em.mm.100-200GHz
s24 S24 24 microns monochromatic flux density Jy phot.flux.density;em.IR.15-30um
s250 S250 250 microns monochromatic flux density Jy phot.flux.density;em.mm.750-1500GHz
s350 S350 350 microns monochromatic flux density Jy phot.flux.density;em.mm.750-1500GHz
s500 S500 500 microns monochromatic flux density Jy phot.flux.density;em.mm.400-750GHz
s70 S70 70 microns monochromatic flux density Jy phot.flux.density;em.IR.60-100um
s850 S850 850 microns monochromatic flux density Jy phot.flux;em.mm.200-400GHz
sfr SFR Star Formation Rate solMass/yr phys.sfr
smips24 sMIPS24 MIPS 24 micron flux density Jy phot.flux.density;em.IR.15-30um
snika1200 sNIKA1200 NIKA2 1200 micron flux density Jy phot.flux.density;em.mm.200-400GHz
snika2000 sNIKA2000 NIKA2 2000 micron flux density Jy phot.flux.density;em.mm.100-200GHz
spacs100 sPACS100 PACS 100 micron flux density Jy phot.flux.density;em.IR.60-100um
spacs160 sPACS160 PACS 160 micron flux density Jy phot.flux.density;em.mm.1500-3000GHz
spacs70 sPACS70 PACS 70 micron flux density Jy phot.flux.density;em.IR.60-100um
sspire250 sSPIRE250 SPIRE 250 micron flux density Jy phot.flux.density;em.mm.750-1500GHz
sspire350 sSPIRE350 SPIRE 350 micron flux density Jy phot.flux.density;em.mm.750-1500GHz
sspire500 sSPIRE500 SPIRE 500 micron flux density Jy phot.flux.density;em.mm.400-750GHz
umean uMean Intensity of the radiation field N/A phys

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