Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf rmf | 2 | X122637.62-624613.1 | chandra | ccd7 | 998.73 | 905.61 | 841.799 | 29.8336 | 0.281348 | 0.00997106 | 171.396 | 1 | 1.21391 | 0.734569 | 110.289 | 2.98553 | A | F | 1.3e+22 | 1.87769e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X122716.83-623915.0 | chandra | ccd3 | 726.167 | 393.143 | 212.047 | 14.8275 | 0.0708707 | 0.00495567 | 75.8879 | 1 | 5.5703 | 3.76321 | 89.9993 | 10.2651 | F | F | 1.29e+22 | 8.2996e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 3 | X122606.82-624913.3 | chandra | ccd6 | 385.393 | 450.709 | 40.6913 | 6.37897 | 0.0136 | 0.002132 | 86.6505 | 1 | 1.55515 | 0.882402 | 138.76 | 4.69034 | F | F | 1.31e+22 | 2.11671e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X122646.90-624505.4 | chandra | ccd7 | 869.268 | 1043.22 | 11.8585 | 3.44362 | 0.00396337 | 0.00115093 | 2.41447 | 0.985913 | 0.824919 | 0.824919 | 0 | 3.87666 | F | F | 1.3e+22 | 5.40879e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X122636.69-624751.9 | chandra | ccd7 | 1011 | 704.4 | 9.83834 | 3.16228 | 0.00328818 | 0.0010569 | 2.00315 | 0.966702 | 0.492 | 0.492 | 40.8621 | 1.68227 | F | F | 1.3e+22 | 4.30603e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X122642.03-624917.5 | chandra | ccd7 | 936.611 | 530.5 | 8.90005 | 3 | 0.00297459 | 0.00100267 | 1.81211 | 0.966702 | 0.492 | 0.492 | 129.754 | 0.736104 | F | F | 1.29e+22 | 3.81014e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122524.05-625204.5 | chandra | ccd6 | 978.7 | 99.8999 | 4.23847 | 2.23609 | 0.00141659 | 0.00074735 | 9.02566 | 0.999996 | 2.25311 | 1.01169 | 70.1169 | 10.0514 | A | F | 1.32e+22 | 2.53264e-14 | 1 | dx | ||||
| Report | 1 | X122552.34-624917.8 | chandra | ccd6 | 586.5 | 440.5 | 0.988927 | 1 | 0.000330521 | 0.000334222 | 2.10588 | 0.97898 | 0.492 | 0.492 | 90 | 6.34363 | F | F | 1.32e+22 | 0 | 1 | d |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest