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J/MNRAS/511/214
-1
Study of CSS/GPS/MPS radio sources (Nascimento+, 2022)
ReadMe+ftp
2022MNRAS.511..214N
Similar Catalogs
Post annotation
1.
J/MNRAS/511/214/table3
Stellar Population Synthesis Results for CSS/GPS sources in our sample
(58 rows)
meta
J/MNRAS/511/214/table3
Simple Constraint
List Of Constraints
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Constraints
applied on Columns
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Column
Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
Source
(char)
Source object name (Object)
(
meta.id;meta.main
)
(
ID_MAIN
)
FC
%
Percentage contribution of Featureless Continuum to SSPs (FC)
(
stat.fit.param
)
(
STAT_PARAM
)
xy
%
Percentage x
y
(t ≤ 50 Myr) Light-weighted young age contribution to SSPs (x
y
)
(
stat.fit.param
)
(
STAT_PARAM
)
xi
%
Percentage x
i
(50 Myr ≤ t ≤ 2 Gyr) Light-weighted intermediate age contribution to SSPs (x
i
)
(
stat.fit.param
)
(
STAT_PARAM
)
xo
%
Percentage x
o
(t > 2 Gyr) Light-weighted old age contribution to SSPs (x
o
)
(
stat.fit.param
)
(
STAT_PARAM
)
my
%
Percentage m
y
(t ≤ 50 Myr) Mass-weighted young age contribution to SSPs (m
y
)
(
stat.fit.param
)
(
STAT_PARAM
)
mi
%
Percentage m
i
(50 Myr ≤ t ≤ 2 Gyr) Mass-weighted intermediate age contribution to SSPs (m
i
)
(
stat.fit.param
)
(
STAT_PARAM
)
mo
%
Percentage m
o
(t > 2 Gyr) Mass-weighted old age contribution to SSPs (m
o
)
(
stat.fit.param
)
(
STAT_PARAM
)
Av
mag
Dust extinction in V band (A
V
)
(
phys.absorption
)
(
PHOT_EXTINCTION_ISM
)
logt*L
[yr]
The light-weighted mean age (<logt*>
L
)
(Note G3)
(
time.age;stat.mean
)
(
TIME_AGE
)
logt*M
[yr]
The mass-weighted mean age ( (<logt*>
M
)
(Note G3)
(
time.age;stat.mean
)
(
TIME_AGE
)
Z*L
The light-weighted mean metallicity (<Z*>
L
)
(Note G3)
(
phys.abund.Z;stat.mean
)
(
PHYS_ABUND_Z
)
Z*M
The mass-weighted mean metallicity (<Z*>
M
)
(Note G3)
(
phys.abund.Z;stat.mean
)
(
PHYS_ABUND_Z
)
logM*
[Msun]
Logarithm of the present stellar mass of the galaxy (M*)
(Note G4)
(
phys.mass
)
(
PHYS_MASS_MISC
)
SFR*
Msun/yr
Logarithm of the Star formation rate over the last 50 Myr (SFR*)
(Note G4)
(
phys.SFR
)
(
PHYS_STAR-FORM_RATE
)
logL1.4
[W/Hz]
Radio uminosity estimated assuming H
0
= 69.8 km/s/Mpc as proposed by Freedman et al.
2019ApJ...882...34F
Hubble Program (LogL
R
)
(
phot.flux.density;em.radio.750-1500MHz
)
(
PHOT_FLUX_RADIO_1.4G
)
MType
(char)
Morphology type determined visually from SDSS images (Morph)
(Note 1)
(
src.morph.type
)
(
MORPH_TYPE
)
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cols
(i)
indexed column
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