![[Use this service from your browser]](/static/img/usesvcbutton.png)
Further access options are discussed below
For a list of all services and tables belonging to this service's resource, see Information on resource ' SIDES'
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).
You can access this service using:
This service is published as follows:
local means it is listed on our front page, ivo_managed means it has a record in the VO registry.
The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| DEC | Delta (ICRS) | Declination (ICRS decimal) | deg | pos.eq.dec |
| dlum | dLum | Luminosity distance | Mpc | pos.distance |
| hscs_pos | Position/Name | Coordinates (as h m s, d m s or decimal degrees), or SIMBAD-resolvable object | N/A | N/A |
| hscs_sr | Search radius | Search radius in arcminutes | N/A | N/A |
| 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 |
| 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 |
| maxrec | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
| 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 | Alpha (ICRS) | Right Ascension (ICRS decimal) | deg | pos.eq.ra |
| redshift | Redshift | Redshift | N/A | src.redshift |
| responseformat | Output Format | File format requested for output. | N/A | meta.code.mime |
| 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 |
| SR | Search Radius | Search radius | deg | N/A |
| 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 |
| verb | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
The following fields are contained in the output by default. More fields may be available for selection; these would be given below in the VOTable output fields.
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| _r | Dist. | Distance to cone center | deg | pos.distance |
| 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 |
The following fields are available in VOTable output. The verbosity level is a number intended to represent the relative importance of the field on a scale of 1 to 30. The services take a VERB argument. A field is included in the output if their verbosity level is less or equal VERB*10.
| Name | Table Head | Description | Unit | UCD | Verb. Level |
|---|---|---|---|---|---|
| index | Index | Internal identifier | N/A | meta.id;meta.main | 1 |
| redshift | Redshift | Redshift | N/A | src.redshift | 1 |
| ra | RA | Simulated Right Ascension | deg | pos.eq.ra;meta.main | 1 |
| dec | Dec | Simulated Declination | deg | pos.eq.dec;meta.main | 1 |
| mhalo | mHalo | Host halo mass | solMass | phys.mass | 1 |
| mstar | mStar | Stellar mass | solMass | phys.mass | 1 |
| qflag | qFlag | Quenching flag (0: star-forming, 1: passive) | N/A | meta.code | 1 |
| sfr | SFR | Star Formation Rate | solMass/yr | phys.sfr | 1 |
| issb | isSB | Staburst flag (0:normal, 1: starburst) | N/A | meta.code | 1 |
| mu | mu | Lensing magnification | N/A | arith.factor | 1 |
| dlum | dLum | Luminosity distance | Mpc | pos.distance | 1 |
| umean | uMean | Intensity of the radiation field | N/A | phys | 1 |
| lir | LIR | Infrared luminosity | solLum | phys.luminosity;em.IR | 1 |
| lfir | LFIR | Far Infrared luminosity | solLum | phys.luminosity;em.IR | 1 |
| s24 | S24 | 24 microns monochromatic flux density | Jy | phot.flux.density;em.IR.15-30um | 1 |
| s70 | S70 | 70 microns monochromatic flux density | Jy | phot.flux.density;em.IR.60-100um | 1 |
| s100 | S100 | 100 microns monochromatic flux density | Jy | phot.flux.density;em.IR.60-100um | 1 |
| s160 | S160 | 160 microns monochromatic flux density | Jy | phot.flux.density;em.mm.1500-3000GHz | 1 |
| s250 | S250 | 250 microns monochromatic flux density | Jy | phot.flux.density;em.mm.750-1500GHz | 1 |
| s350 | S350 | 350 microns monochromatic flux density | Jy | phot.flux.density;em.mm.750-1500GHz | 1 |
| s500 | S500 | 500 microns monochromatic flux density | Jy | phot.flux.density;em.mm.400-750GHz | 1 |
| s850 | S850 | 850 microns monochromatic flux density | Jy | phot.flux;em.mm.200-400GHz | 1 |
| s1100 | S1100 | 1100 microns monochromatic flux density | Jy | phot.flux.density;em.mm.200-400GHz | 1 |
| s2000 | S2000 | 2000 microns monochromatic flux density | Jy | phot.flux.density;em.mm.100-200GHz | 1 |
| smips24 | sMIPS24 | MIPS 24 micron flux density | Jy | phot.flux.density;em.IR.15-30um | 1 |
| spacs70 | sPACS70 | PACS 70 micron flux density | Jy | phot.flux.density;em.IR.60-100um | 1 |
| spacs100 | sPACS100 | PACS 100 micron flux density | Jy | phot.flux.density;em.IR.60-100um | 1 |
| spacs160 | sPACS160 | PACS 160 micron flux density | Jy | phot.flux.density;em.mm.1500-3000GHz | 1 |
| sspire250 | sSPIRE250 | SPIRE 250 micron flux density | Jy | phot.flux.density;em.mm.750-1500GHz | 1 |
| sspire350 | sSPIRE350 | SPIRE 350 micron flux density | Jy | phot.flux.density;em.mm.750-1500GHz | 1 |
| sspire500 | sSPIRE500 | SPIRE 500 micron flux density | Jy | phot.flux.density;em.mm.400-750GHz | 1 |
| snika1200 | sNIKA1200 | NIKA2 1200 micron flux density | Jy | phot.flux.density;em.mm.200-400GHz | 1 |
| snika2000 | sNIKA2000 | NIKA2 2000 micron flux density | Jy | phot.flux.density;em.mm.100-200GHz | 1 |
| lprimco10 | Lprim CO(1-0) | Pseudo luminosity of CO(1-0) | K.km.s**-1.pc**2 | phys.luminosity;em.line.CO | 1 |
| ico10 | iCO(1-0) | Flux of the CO(1-0) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico21 | iCO(2-1) | Flux of the CO(2-1) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico32 | iCO(3-2) | Flux of the CO(3-2) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico43 | iCO(4-3) | Flux of the CO(4-3) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico54 | iCO(5-4) | Flux of the CO(5-4) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico65 | iCO(6-5) | Flux of the CO(6-5) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico76 | iCO(7-6) | Flux of the CO(7-6) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| ico87 | iCO(8-7) | Flux of the CO(8-7) line | Jy.km.s**-1 | phot.flux;em.line.CO | 1 |
| lcii_lagache | L[CII] Lagache | Luminosity of [CII] line using the L18 relation | solLum | phys.luminosity;em.line | 1 |
| icii_lagache | i[CII] Lagache | Flux of [CII] line using the L18 relation | Jy.km.s**-1 | phot.flux;em.line | 1 |
| lcii_de_looze | L[CII] de Looze | Luminosity of [CII] line using the DL14 relation | solLum | phys.luminosity;em.line | 1 |
| icii_de_looze | i[CII] de Looze | Flux of [CII] line using the DL14 relation | Jy.km.s**-1 | phot.flux;em.line | 1 |
| ici10 | i[CI](1-0) | Flux of [CI](1-0) line | Jy.km.s**-1 | phot.flux;em.line | 1 |
| ici21 | i[CII](2-1) | Flux of [CI](2-1) line | Jy.km.s**-1 | phot.flux;em.line | 1 |
| _r | Dist. | Distance to cone center | deg | pos.distance | 10 |
VOResource XML (that's something exclusively for VO nerds)
![[Operator logo]](/static/img/logo_medium.png){kind=logo}