VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+A/674/A64
  FIFI-LS spectroscopy of Gy 3-7 in outer Galaxy (Le+, 2023)
cube/fits
Post annotation
img(gal)
1.J/A+A/674/A64/list(c)List of datacubes (10 rows)
2.J/A+A/674/A64/table2CO rotational temperature, the number of emitting molecules, and total line luminosities of CO and [OI] lines toward dense cores in Gy 3-7 and IM YSOs from Matuszak et al. (2015A&A...578A..20M) (8 rows)
3.J/A+A/674/A64/table4Physical parameters for a subset of YSO candidates with at least 5 photometric data points (12 rows)
4.J/A+A/674/A64/tablea1Parameters of the 22 GHz H2O maser lines detected toward CMa l224 with RT4 (7 rows)
5.J/A+A/674/A64/tableb1Flux SOFIA FIFI-LS toward the two dense cores within a beam size of 20" (9 rows)
6.J/A+A/674/A64/tablec1(c)*Multi-wavelength photometry of YSO candidates in the IRAS field. (Note) (15 rows)
7.J/A+A/674/A64/tabled1CO rotational temperature and number of emitting molecules for HM YSOs, derived by fitting the rotational diagram of CO using all and only four available CO transitions (10 rows)
8.J/A+A/674/A64/tabled2Far-IR line cooling luminosity of the sample in the Milky Way (MW), LMC, and SMC used to compare with results of this study (29 rows)

 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1+6)RAJ2000 deg (i) Right Ascension of center (J2000) (pos.eq.ra;meta.main)
  (1+6)DEJ2000 deg (i) Declination of center (J2000) (pos.eq.dec;meta.main)
  (1)Nx  Number of pixels along X-axis (meta.number)
  (1)Ny  Number of pixels along Y-axis (meta.number)
  (1)Nz  Number of slices (meta.number)
  (1)Obs.date s (n)Observation date (time.epoch;obs)
  (1)bWAVE 0.1nm Lower value of wavelength interval (em.wl)
  (1)BWAVE 0.1nm Upper value of wavelength interval (em.wl)
  (1)dWAVE 0.1nm Wavelength resolution (spect.resolution)
  (1)size Kibyte Size of FITS file (phys.size;meta.fits)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)FileName (char) Name of FITS file, in subdirectory fits (meta.id;meta.fits)
  (1)Title (char) Title of the FITS file (meta.title;meta.fits)
  (2+4+8)Group (char) [AB] Group (Note 1)   (meta.id)
  (2+7+8)Source (char) Source name (meta.id;meta.main)
  (2)Trot K CO rotational temperature (Note 2)   (phys.temperature)
  (2)e_Trot K Uncertainty of rotational temperature (Note 2)   (stat.error)
  (2)logNtot  Base-10 logarithm of total number of emitting molecules (Note 2)   (meta.number)
  (2)e_logNtot  Uncertainty of logNtot (Note 2)   (stat.error)
  (2)LCO mLsun Total CO luminosity in warm component (Note 3)   (phys.luminosity)
  (2)e_LCO mLsun Uncertainty of LCO (Note 3)   (stat.error)
  (2)LOI63 mLsun Luminosity of [O I] 63 um line (phys.luminosity)
  (2)e_LOI63 mLsun Uncertainty of LOI63 (stat.error)
  (2)LOI145 mLsun Luminosity of [O I] 145 um line (phys.luminosity)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)e_LOI145 mLsun Uncertainty of LOI145 (stat.error)
  (3+6)ID  Source identification number (meta.id;meta.main)
  (3)ModelSet (char) Model Set name (Note G1)   (meta.id;stat.fit)
  (3)Class (char) YSO class as determined from the SED fitting (see Sect. 4.5) (src.class)
  (3)R* Rsun Stellar radius (phys.size.radius)
  (3)T* K Stellar temperature (phys.temperature)
  (3)L* Lsun Stellar Luminosity (phys.luminosity)
  (3)M* Msun (n) Stellar mass (Note 1)   (phys.mass)
  (3)Age Myr (n) Stellar age (Note 1)   (time.age)
  (3)Note (char) Note for YSO (Note 2)   (meta.note)
  (4)Obs.date (char) Observation date (time.epoch;obs)
  (4)Vp km/s Central velocity of of the water maser line (phys.veloc;em.wl.central)
  (4)e_Vp km/s Uncertainty of Vp (stat.error)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)Sp Jy Flux density peak (phot.flux.density;em.radio)
  (4)e_Sp Jy Uncertainty of Sp (stat.error;src.spType)
  (4)FWHM km/s FWHM (phys.angSize)
  (4)e_FWHM km/s Uncertainty of FWHM (stat.error;phys.angSize)
  (4)intSdV Jy.km/s Integrated flux density (phot.flux.density;em.radio)
  (4)e_intSdV Jy.km/s Uncertainty of intSdV (stat.error)
  (5)lambda um Wavelength (em.wl)
  (5)FA 10-16W/m2Flux at core A (phot.flux.density;em.radio)
  (5)e_FA 10-16W/m2Uncertainty of FA (stat.error)
  (5)FB 10-16W/m2(n) Flux at core B (phot.flux.density;em.radio)
  (5)e_FB 10-16W/m2(n) Uncertainty of FB (stat.error)
  (6)SJ mJy (n) 2MASS J flux (phot.flux.density;em.IR.J)
  (6)e_SJ mJy (n) 2MASS J flux error (stat.error)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (6)SH mJy 2MASS H flux (phot.flux.density;em.IR.H)
  (6)e_SH mJy 2MASS H flux error (stat.error)
  (6)SKs mJy 2MASS Ks flux (phot.mag;em.IR.K)
  (6)e_SKs mJy 2MASS Ks flux error (stat.error)
  (6)S3.6 mJy (n) IRAC 3.6um flux (phot.mag;em.IR.3-4um)
  (6)e_S3.6 mJy (n) IRAC 3.6um flux error (stat.error)
  (6)S4.5 mJy (n) IRAC 4.5um flux (phot.mag;em.IR.4-8um)
  (6)e_S4.5 mJy (n) IRAC 4.5um flux error (stat.error)
  (6)SW1 mJy (n) AllWISE 3.4um (W1) flux (phot.mag;em.IR.3-4um)
  (6)e_SW1 mJy (n) AllWISE 3.4um (W1) flux error (stat.error)
  (6)SW2 mJy (n) AllWISE 4.6um (W2) flux (phot.mag;em.IR.4-8um)
  (6)e_SW2 mJy (n) AllWISE 4.6um (W2) flux error (stat.error)
  (6)SW3 mJy (n) AllWISE 12um (W3) flux (phot.flux.density;em.IR.8-15um)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (6)e_SW3 mJy (n) AllWISE 12um (W3) flux error (stat.error)
  (6)SW4 mJy (n) AllWISE 22um (W4) flux (phot.flux.density;em.IR.15-30um)
  (6)e_SW4 mJy (n) AllWISE 22um (W4) flux error (stat.error)
  (6)S70 Jy (n) PACS 70um flux (phot.flux.density;em.IR.30-60um)
  (6)e_S70 Jy (n) PACS 70um flux error (stat.error)
  (6)S160 Jy (n) PACS 160um flux (phot.flux.density;em.mm.1500-3000GHz)
  (6)e_S160 Jy (n) PACS 160um flux error (stat.error)
  (6)S250 Jy (n) SPIRE 250um flux (phot.flux.density;em.mm.750-1500GHz)
  (6)e_S250 Jy (n) SPIRE 250um flux error (stat.error)
  (6)S350 Jy (n) SPIRE 350um flux (phot.flux.density;em.mm.750-1500GHz)
  (6)e_S350 Jy (n) SPIRE 350um flux error (stat.error)
  (6)S500 Jy (n) SPIRE 500um flux (phot.flux.density;em.mm.400-750GHz)
  (6)e_S500 Jy (n) SPIRE 500um flux error (stat.error)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (7)Trot4 K Rotational temperatures calculated using 4 CO transitions with Jup = (14, 16, 17, 22) (phys.temperature)
  (7)e_Trot4 K Uncertainty in Trot4 (stat.error)
  (7)Trota K Rotational temperatures calculated using all detected CO transitions, data is adopted from Karska et al. (2014A&A...562A..45K). (phys.temperature)
  (7)e_Trota K Uncertainty in Trota (stat.error)
  (7)Diff % The relative difference between Trot4 and Trota is taken as |1-Trot4/Trota|*100 (stat.fit.param)
  (8)D kpc Distance (pos.distance)
  (8)e_D kpc (n) Distance error (stat.error)
  (8)r_D  Reference of distances (Note G2)   (meta.ref;pos.frame)
  (8)RGC kpc (n) Galactocentric radius (Note 2)   (pos.distance;pos.galactocentric)
  (8)Z  Metallicity compared to Zsun (Note 3)   (phys.abund.Z)
  (8)logLbol [Lsun] Based-10 logarithm of bolometric to solar luminosity ratio (phys.luminosity)
  (8)r_logLbol  Reference of logLbol (Note G2)   (meta.ref;pos.frame)
  (8)LCO 10-2Lsun Luminosty of CO in warm component (Note 4)   (phys.luminosity)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (8)e_LCO 10-2Lsun (n) Uncertainty of LCO (stat.error)
  (8)LOI 10-2Lsun Luminosity of [OI] line (Note 5)   (phys.luminosity)
  (8)e_LOI 10-2Lsun (n) Uncertainty of LOI (stat.error)
  (8)Lratio  Luminosity ratio of CO to [OI] (phys.luminosity;arith.ratio)
  (8)e_Lratio  (n) Uncertainty of Lratio (stat.error)
  (8)refLline  Reference of the line luminosities (Note G2)   (meta.id;spect.line)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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