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ASCAGIS - ASCA GIS Source Catalog (AMSS-I + AMSS-II) |
HEASARC Archive |
For each source, the ASCA source name, position, 90% error radius, count rates (both observed and as corrected for Galactic absorption) in the 3 energy bands, detection signifances and fluxes in the 3 energy bands, and hardness ratio and associated error are provided.
The ASCA Medium Sensitivity Survey (the GIS Catalog Project): Source Catalog. Ueda Y., Ishisaki Y., Takahashi T., Makishima K., Ohashi T. <Astrophys. J. Suppl. Ser. 133, 1 (2001)> =2001ApJS..133....1U The ASCA Medium Sensitivity Survey (the GIS Catalog Project): Source Catalog II. Ueda Y., Ishisaki Y., Takahashi T., Makishima K., Ohashi T. <Astrophys. J. Suppl. Ser. 161, 185 (2005)> =2005ApJS..161..185U
Name
The ASCA source name constructed in the recommended IAU fashion,
using the prefix '1AXG (1st ASCA X-Ray GIS source) and the J2000 equatorial
coordinates.
RA
The Right Ascension of the source. This was provided in J2000 degrees
with a precision of 0.0001 degrees in the original tables.
Dec
The Declination of the source. This was provided in J2000 degrees
with a precision of 0.0001 degrees in the original tables.
LII
The Galactic Longitude of the source.
BII
The Galactic Latitude of the source.
Error_Radius
The positional error radius (90% confidence), including both
the statistical and systematic errors, in arcminutes. See Section 3.3 of
Paper I for more details.
SNR_Total
The detection significance, i.e., number of sigma, in the
0.7-7 keV band.
SNR_Hard
The detection significance, i.e., number of sigma, in the
2-10 keV band.
SNR_Soft
The detection significance, i.e., number of sigma, in the
0.7-2 keV band.
Count_Rate_Total
The vignetting-corrected "observed" count rate in the
0.7-7 keV band at the reference position in the X-Ray Telescope coordinate
(8.5' offset) integrated within a radius of 5.9', in counts per second.
This has not been corrected for Galactic absorption.
Count_Rate_Hard
The vignetting-corrected "observed" count rate in the
2-10 keV band, at the reference position in the X-Ray Telescope coordinate
(8.5' offset) integrated within a radius of 5.9', in counts per second.
This has not been corrected for Galactic absorption.
Count_Rate_Soft
The vignetting-corrected "observed" count rate in the
0.7-2.0 keV band, at the reference position in the X-Ray Telescope coordinate
(8.5' offset) integrated within a radius of 5.9', in counts per second.
This has not been corrected for Galactic absorption.
Corr_Count_Rate_Total
The 0.7-7 keV count rate, in counts per second,
corrected for Galactic interstellar absorption using the Dickey and Lockman
(1990, ARA&A, 28, 215) estimate.
Corr_Count_Rate_Hard
The 2-10 keV count rate, in counts per second,
corrected for Galactic interstellar absorption using the Dickey and Lockman
(1990, ARA&A, 28, 215) estimate.
Corr_Count_Rate_Soft
The 0.7-2 keV count rate, in counts per second,
corrected for Galactic interstellar absorption using the Dickey and Lockman
(1990, ARA&A, 28, 215) estimate.
Flux_Total
The 0.7-7 keV flux, in cgs units of erg/s/cm2, corrected for
Galactic interstellar absorption. This flux has been obtained using the
observed count rate in the same band and assuming a power-law with
Galactic absorption, with the best-fit photon index derived from the
observed hardness ratio HR1. See Section 2.4 of Paper I for more details.
Flux_Hard
The 2-10 keV flux, in cgs units of erg/s/cm2, corrected for
Galactic interstellar absorption. This flux has been obtained using the
observed count rate in the same band and assuming a power-law with
Galactic absorption, with the best-fit photon index derived from the
observed hardness ratio HR1. See Section 2.4 of Paper I for more details.
Flux_Soft
The 0.7-2 keV flux, in cgs units of erg/s/cm2, corrected for
Galactic interstellar absorption. This flux has been obtained using the
observed count rate in the same band and assuming a power-law with
Galactic absorption, with the best-fit photon index derived from the
observed hardness ratio HR1. See Section 2.4 of Paper I for more details.
HR1
The hardness ratio, HR1, defined as HR1 = (H-S)/(H+S), where H is
corr_count_rate_hard (the 2-10 keV count rate corrected for Galactic
interstellar absorption) and S is corr_count_rate_soft (the 0.7-2 keV flux,
corrected for Galactic interstellar absorption).
HR1_Error
The 1-sigma statistical error in the hardness ratio, HR1.
Field_ID
The identification of the field in which the source was detected.
The information on these fields is given in Table 1 of AMSS-I for fields
starting with 'I-' and Table 1 of AMSS-II for fields starting with 'II-'.
Target_Flag
This parameter is a flag which to set to 'Y' to indicate
that the source was the target of the ASCA observation.
Catalog_Part
This parameter is a flag which indicates from which part of
the AMSS Catalog the entry originates ('I' for AMSS-I, 'II' for AMSS-II).
Duplicate_Source
This parameter is a flag which is set to 'Y' to indicate
that the entry is likely a duplicate of another AMSS source, else it is set to
'N'. Most (81/86) of the duplicates are AMSS-I sources that were independently
redetected in AMSS-II, with the remainder being sources that were duplicated
within AMSS-I. To identify duplicates, the authors looked for pairs if sources
whose positions coincided within twice the combined 90% positional errors.
85 of the 86 duplicates are listed in Table 4 of Paper II, while the remaining
duplicate pair (the two sources with the identical name 1AXG J053056+1331
in AMSS-I) was noticed by the HEASARC while compiling the Browse version of
this table.