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M51CXO - M 51 Chandra X-Ray Discrete Source Catalog |
HEASARC Archive |
The Chandra observations of M 51 were performed on 2000 June 20 and 2001 June 23 with the ACIS instrument. The background was stable in both observations, and effective exposure times of 14.9 and 26.8ks were obtained for the observations in 2000 and 2001, respectively.
The luminous X-ray source population in M51 observed with Chandra. Terashima Y., Wilson A.S. <Astrophys. J., 601, 735-758 (2004)> =2004ApJ...601..735T
Source_Number
A running number for the X-ray source in order of
increasing J2000.0 Right Ascension in each of the original tables. Since this
HEASARC table is formed from the concatenation of 3 tables from the reference
paper, the source number by itself is not a unique source identifier.
The combination of table number and source number, however,
uniquely identifies an X-ray source in this table.
Table_Number
This HEASARC-created parameter indicates from which table
the X-ray source was taken: a value of 2 indicates that it is one of the
84 sources spatially coincident with NGC 5194 listed in Table 2 of the
reference paper, a value of 3 means it is one of the 12 sources spatially
coincident with the companion galaxy NGC 5195 listed in Table 3, and a value
of 4 means it is one of the 17 other sources elsewhere in the Chandra field
listed in Table 4. The combination of table number and source number
uniquely identifies an X-ray source in this table.
RA
The Right Ascension of the X-ray source in the selected equinox. This was
given in J2000.0 coordinates to a precision of 0.01 seconds of time in the
original tables.
Dec
The Declination of the X-ray source in the selected equinox. This was
given in J2000.0 coordinates to a precision of 0.1 arcseconds in the original
table.
LII
The Galactic Longitude of the X-ray source.
BII
The Galactic Latitude of the X-ray source.
Name
The name of the X-ray source using the 'CXOM51' prefix followed by
the J2000.0 coordinates (JHHMMSS.s+DDMMSS), as recommended by the CDS
Dictionary of Nomenclature of Celestial Objects.
Alt_Name
The alternate mame of the X-ray source using the '[TW2004]' prefix
(from Terashima and Wilson 2004), followed by the string 'NGC 5194' for
sources from Table 2 of the reference paper, or 'NGC 5195' for sources from
Table 3, or 'Source' for sources from Table 4, and ending with the X-ray
source number value, as recommended by the CDS Dictionary of Nomenclature of
Celestial Objects, e.g., '[TW2004] NGC 5194 1'.
FB_Counts
The observed counts for the X-ray source in the full (0.5 - 8 keV)
band for the combined data set of the first and second observations. The
number of counts has not been corrected for vignetting.
FB_Counts_Error
The RMS 1-sigma uncertainty in the full-band counts for the
combined observation.
SB_Counts_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
SB_Counts
The observed counts for the X-ray source in the soft (0.5 - 2 keV)
band for the combined data set of the first and second observations. The
number of counts has not been corrected for vignetting.
SB_Counts_Error
The RMS 1-sigma uncertainty in the soft-band counts for the
combined observation.
HB_Counts_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
HB_Counts
The observed counts for the X-ray source in the hard (2 - 8 keV)
band for the combined data set of the first and second observations. The
number of counts has not been corrected for vignetting.
HB_Counts_Error
The RMS 1-sigma uncertainty in the hard-band counts for the
combined observation.
FB_Counts_Obs1_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
FB_Counts_Obs1
The observed counts for the X-ray source in the full
(0.5 - 8 keV) band for the first observation. The number of counts has
not been corrected for vignetting.
FB_Counts_Obs1_Error
The RMS 1-sigma uncertainty in the full-band counts
for the first observation.
SB_Counts_Obs1_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
SB_Counts_Obs1
The observed counts for the X-ray source in the soft
(0.5 - 2 keV) band for the first observation. The number of counts has
not been corrected for vignetting.
SB_Counts_Obs1_Error
The RMS 1-sigma uncertainty in the soft-band counts
for the first observation.
HB_Counts_Obs1_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
HB_Counts_Obs1
The observed counts for the X-ray source in the hard
(2 - 8 keV) band for the first observation. The number of counts has
not been corrected for vignetting.
HB_Counts_Obs1_Error
The RMS 1-sigma uncertainty in the hard-band counts
for the first observation.
FB_Counts_Obs2_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection
FB_Counts_Obs2
The observed counts for the X-ray source in the full
(0.5 - 8 keV) band for the second observation. The number of counts
has not been corrected for vignetting.
FB_Counts_Obs2_Error
The RMS 1-sigma uncertainty in the full-band counts
for the second observation.
SB_Counts_Obs2_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
SB_Counts_Obs2
The observed counts for the X-ray source in the soft
(0.5 - 2 keV) band for the second observation. The number of counts has
not been corrected for vignetting.
SB_Counts_Obs2_Error
The RMS 1-sigma uncertainty in the soft-band counts
for the second observation.
HB_Counts_Obs2_Limit
This parameter is set to '<' if the value quoted in the
associated counts parameter is an upper limit rather than a detection.
HB_Counts_Obs2
The observed counts for the X-ray source in the hard
(2 - 8 keV) band for the second observation. The number of counts has
not been corrected for vignetting.
HB_Counts_Obs2_Error
The RMS 1-sigma uncertainty in the hard-band counts
for the second observation.