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Simple Target
List Of Targets
Fast Xmatch with large catalogs or Simbad
Target
Name (resolved by
Sesame
) or
Position
:
J2000
B1975
B1950
B1900
B1875
B1855
Galactic
Supergal.
Ecl.J2000
Target dimension:
deg
arcmin
arcsec
NB: The epoch used for the query is the original epoch of the table(s)
Radius
Box size
J/MNRAS/510/4998
-1
ATOMS IV Gas clumps properties and SFRs (Zhang+, 2022)
ReadMe+ftp
2022MNRAS.510.4998Z
Similar Catalogs
Post annotation
1.
J/MNRAS/510/4998/table2
(c)
Gas clumps identified in CS J = 2-1
(177 rows)
meta
J/MNRAS/510/4998/table2
2.
J/MNRAS/510/4998/table3
(c)
Gas clumps identified in HC3N J = 11-10
(185 rows)
meta
J/MNRAS/510/4998/table3
3.
J/MNRAS/510/4998/table4
(c)
Gas clumps identified in H40α
(75 rows)
meta
J/MNRAS/510/4998/table4
4.
J/MNRAS/510/4998/table5
(c)
Luminosities of ATOMS sources
(146 rows)
meta
J/MNRAS/510/4998/table5
5.
J/MNRAS/510/4998/table7
(c)
SFRs and gas masses of ATOMS sources
(146 rows)
meta
J/MNRAS/510/4998/table7
Xmatch is
on
off
Radius:
arcsec
Master table:
all - matching rows only
J/MNRAS/510/4998/table2
J/MNRAS/510/4998/table3
J/MNRAS/510/4998/table4
J/MNRAS/510/4998/table5
J/MNRAS/510/4998/table7
Simple Constraint
List Of Constraints
Query by
Constraints
applied on Columns
(
Output Order:
+
-
)
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join
Column
Constraint
Explain
(
UCD
)
(ALL)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
(ALL)
IRAS
(char)
IRAS source identifier (IHHMMm±DDMM) (IRAS)
(
meta.id;meta.main
)
(
ID_MAIN
)
(ALL)
ID
[1/4] Relative ID number to IRAS source identifier (ID)
(
meta.id
)
(
ID_NUMBER
)
(1+2+3)
OffsetRA
arcsec
Offset in right ascension relative to IRAS RAdeg position (OffsetRA)
(
pos.eq.ra;arith.diff
)
(
POS_EQ_RA_OFF
)
(1+2+3)
OffsetDE
arcsec
Offset in declination relative to IRAS DEdeg position (OffsetDec)
(
pos.eq.dec;arith.diff
)
(
POS_EQ_DEC_OFF
)
(1+2+3)
Rasp
The aspect ratio is defined as the ratio between de-convolved semimajor size a and semiminor size b (r
asp
)
(
phys.size.axisRatio
)
(
PHYS_AXIS-RATIO
)
(1+2+3)
Reff
pc
The effective radius is defined as sqrt(ab) (R
eff
)
(
phys.size.radius
)
(
PHYS_SIZE_RADIUS_GENERAL
)
(1+2+3)
Speak
Jy.km/beam/s
Peak integrated intensity (S
peak
)
(
spect.line.intensity;em.mm.100-200GHz
)
(
SPECT_LINE_INTENSITY
)
(1+2+3)
Stotal
Jy.km/s
Total flux intensity (S
total
)
(
spect.line.intensity;em.mm.100-200GHz
)
(
SPECT_LINE_INTENSITY
)
(ALL)
Simbad
(char)
ask the
Simbad
data-base about this object
(
meta.ref.url
)
(
DATA_LINK
)
(1+2+3+5)
_RA
deg
(i)
Right Ascension (J2000) from SIMBAD (not part of the original data)
(
pos.eq.ra;meta.main
)
(
POS_EQ_RA_MAIN
)
ALL
cols
(i)
indexed column
(1+2+3+5)
_DE
deg
(i)
Declination (J2000) from SIMBAD (not part of the original data)
(
pos.eq.dec;meta.main
)
(
POS_EQ_DEC_MAIN
)
(3)
e_Stotal
Jy.km/s
Mean error of Stotal (errS
total
)
(
stat.error
)
(
ERROR
)
(3)
logQ0
[s-1]
The rate of ionizations as computed with equation A5 in the section APPENDIX A From rrls to sfrs (logQ0)
(
arith.rate;phys.atmol.ionization
)
(
PHYS_IONIZATION_PHOTONS_TOTAL
)
(3)
logne
[cm-3]
The electron density according to equation B1 in the section APPENDIX B Derivation of electron density and ionized gas mass (logne)
(
phys.density
)
(
PHYS_DENSITY_ELECT
)
(3+5)
logMion
[Msun]
The mass of ionized gas in computed with equation B2 in the section APPENDIX B Derivation of electron density and ionized gas mass (logMion)
(
phys.mass
)
(
PHYS_MASS_MISC
)
(4)
RAJ2000
"h:m:s"
(i)
Right ascension (J2000)
(
pos.eq.ra;meta.main
)
(
POS_EQ_RA_MAIN
)
(4)
DEJ2000
"d:m:s"
(i)
Declination (J2000)
(
pos.eq.dec;meta.main
)
(
POS_EQ_DEC_MAIN
)
(4)
D
kpc
Distance of the source (Distance)
(
pos.distance
)
(
PHYS_DISTANCE_TRUE
)
(4)
RGC
kpc
Galactocentric distance (RGC)
(
pos.distance;pos.galactocentric
)
(
POS_GAL_GC
)
(4)
logLbol
[Lsun]
Logarithm of the bolometric luminosity are calculated from integrating the whole SED (logLbol)
(
phys.luminosity
)
(
PHOT_BOL_LUMINOSITY
)
(4)
logL'CS
[K.km/s/pc2]
(n)
The molecular carbon monosulfide CS line luminosity from equation 1 of the section 3.3 The L
bol
-L'
mol
scaling relations (logL'CS)
(
phys.luminosity;phys.mol;em.line
)
(
SPECT_LUMINOSITY
)
(4)
logL'HC3N
[K.km/s/pc2]
(n)
The molecular cyanoacetylene HC
3
N line luminosity from equation 1 of the section 3.3 The L
bol
-L'
mol
scaling relations (logL'HC3N)
(
phys.luminosity;phys.mol;em.line
)
(
SPECT_LUMINOSITY
)
(5)
logLH40a
[Jy.kpc2.km/s]
(n)
Logarithm of line H40α luminosity computed with equation A1 of the section APPENDIX A From rrls to sfrs (logLH40a)
(
phys.luminosity;em.line
)
(
SPECT_LUMINOSITY
)
ALL
cols
(n)
indicates a possible blank or NULL column
(i)
indexed column
(5)
logSFRbol
[Msun/Myr]
(n)
Logarithm of the bolometric SFR derived from the Lbol as in equation 2 of the section 4.1 SFRs (logSFRbol)
(
phys.SFR
)
(
PHYS_STAR-FORM_RATE
)
(5)
logSFRH40a
[Msun/Myr]
(n)
Logarithm of the H40α SFR derived as equation A6 of the section APPENDIX A From rrls to sfrs (logSFRH40a)
(
phys.SFR
)
(
PHYS_STAR-FORM_RATE
)
(5)
logMclump
[Msun]
Logarithm of the molecular gas in clumps from Liu et al.
2020MNRAS.496.2790L
Cat.
J/MNRAS/496/2790
(logMclump)
(
phys.mass
)
(
PHYS_MASS_MISC
)
ALL
cols
(n)
indicates a possible blank or NULL column
(i)
indexed column
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https://cdsannotations.u-strasbg.fr/annotations/vizierTable//
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