| Search in Xamin or Browse... |
SMCROSXRAY - ROSAT PSPC Survey of the Small Magellanic Cloud |
HEASARC Archive |
A ROSAT PSPC X-Ray Survey of the Small Magellanic Cloud
Kahabka P., Pietsch W., Filipovic M.D., Haberl F.
<Astron. Astrophys. Suppl. Ser. 136, 81 (1999)>
=1999A&AS..136...81K
Catalog_Name
The source designation constructed from the catalog sequential number
together with the prefix 'KPF99' recommended by the Dictionary of
Nomenclature for this catalog.
Name
The ROSAT source designation.
RA
The right ascension in the selected equinox. The equinox of the positions in
the input table for this catalog was J2000.
Dec
The declination in the selected equinox. The equinox of the positions in the
input table for this catalog was J2000.
LII
Galactic longitude of the source.
BII
Galactic latitude of the source.
Error_Radius
The 90% confidence positional uncertainty of the X-ray position, in
arcseconds.
Count_Rate
The total count rate of the X-ray source in the 0.1-2.4 keV energy range.
Count_Rate_Error
The 1-sigma error of the total count rate.
Hardness_Ratio_1
The soft hardness ratio HR1 = (H-S)/(H+S), where H is the counts in ROSAT
PSPC channels 52-201 (energies from 0.5-2.1 keV), and S is the counts in
ROSAT PSPC channels 11-41 (0.1-0.4 keV).
Hardness_Ratio_1_Error
The 1-sigma error of the soft hardness ratio.
Hardness_Ratio_2
The hard hardness ratio HR2 = (H2-H1)/(H2+H1), where H1 is the counts in
ROSAT PSPC channels 52-90 (energies from 0.5-0.9 keV), and H2 is the counts
in ROSAT PSPC channels 91-201 (0.9-2.0 keV).
Hardness_Ratio_2_Error
The 1-sigma error of the hard hardness ratio.
Source_Extent
The source extent of the X-ray source, in arcseconds, in those
cases where the likelihood ratio for extent is greater than 10.
Likelihood
The likelihood ratio of existence LH_exist which is related to the
probability of existence P by P ~ (1-exp(-LH_exist)). Only sources for which
LH_exist > 10 (P > (1 - 4.5 x 10-5)) are included in this catalog.
Off_Axis
The off-axis angle of the X-ray source, in arcminutes, for the detecttion
with the highest LH_exist from the different bands.
Ww_Number
The source number of the corresponding Einstein identification given by Wang
& Wu, 1992, ApJS, 78, 391.
Einstein_Offset
The offset, in arcseconds, of the ROSAT PSPC position from the Einstein
source position.
Spect_Type
The spectral type of the Simbad-identified star.
App_Mag
The magnitude of the Simbad-identified star.
SIMBAD_Offset
The offset, in arcseconds, of the ROSAT PSPC position from the position of
the Simbad-identified star.
Broad_Class
The source classification scheme used in the catalog (more details on how
sources were assigned to these classes can be found in Table 3 of the
published version of this catalog):
A: background AGN or quasar
B: hard X-ray binary
BL: luminous hard X-ray binary
BW: weak hard X-ray binary
D: (possible) artifact
F: foreground star
R: supernova remnant or extended structure
S: super-soft source
SL: luminous super-soft source
SW: low-luminosity super-soft source
Refined_Class
A refined source classification for candidate AGN and hard X-ray binaries:
AB: class A or B (see broad class definitions)
H: HII region
Note
A note on either the radio or the optical identification.
Class
An approximate browse classification, derived from the value of the
broad_class field. Notice that in some cases, the refined_class parameter
gives additional or different classification information.