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 | 1 | X175532.13-275130.6 | chandra | ccd3 | 386.161 | 61.0098 | 34.4621 | 5.87044 | 0.0159774 | 0.00272166 | 73.0741 | 1 | 3.8341 | 1.61764 | 124.769 | 8.12087 | F | F | 7.55e+21 | 2.58218e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X175602.13-273920.2 | chandra | ccd0 | 785.1 | 711 | 9.59495 | 3.16229 | 0.0044484 | 0.00146609 | 20.4429 | 1 | 1.00598 | 0.492 | 127.934 | 5.97723 | A | F | 7.63e+21 | 6.56879e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X175555.76-273932.3 | chandra | ccd0 | 957.773 | 687.092 | 14.1954 | 3.76768 | 0.00658127 | 0.00174677 | 30.2446 | 1 | 0.954496 | 0.954496 | 0 | 4.99476 | F | F | 7.7e+21 | 9.55294e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X175545.34-273607.8 | chandra | ccd2 | 208.625 | 922.25 | 5.83853 | 2.82848 | 0.00270685 | 0.00131133 | 12.5106 | 1 | 4.66134 | 1.22217 | 122.388 | 7.74483 | A | F | 7.96e+21 | 4.35364e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X175549.96-274633.4 | chandra | ccd1 | 954.9 | 853.7 | 4.94326 | 2.23607 | 0.00229179 | 0.00103668 | 10.452 | 1 | 0.511417 | 0.492 | 43.7552 | 2.93911 | F | F | 7.53e+21 | 3.16803e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X175548.19-274036.3 | chandra | ccd2 | 131.5 | 376.5 | 4.09696 | 2.23609 | 0.00189943 | 0.00103669 | 8.7788 | 0.999997 | 1.7411 | 0.492 | 173.736 | 3.36604 | A | F | 7.76e+21 | 2.66621e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X175601.72-274448.4 | chandra | ccd1 | 637.75 | 1067 | 3.96944 | 2 | 0.00184031 | 0.000927238 | 8.39298 | 0.999996 | 0.71246 | 0.492 | 6.15401 | 3.91198 | F | F | 7.49e+21 | 2.67735e-14 | 1 | dx | ||||
| Report | 4 | X175533.22-274433.5 | chandra | ccd3 | 356.75 | 908.25 | 3.96191 | 2 | 0.00183682 | 0.000927238 | 8.40091 | 0.999996 | 0.492 | 0.492 | 82.9819 | 2.59951 | F | F | 7.78e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X175551.69-274756.9 | chandra | ccd1 | 908.25 | 684 | 3.96051 | 2 | 0.00183616 | 0.000927238 | 8.37408 | 0.999996 | 0.563899 | 0.492 | 102.821 | 4.37116 | F | F | 7.49e+21 | 2.60347e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X175534.92-274759.4 | chandra | ccd3 | 310.5 | 489.75 | 3.92967 | 2 | 0.00182187 | 0.000927238 | 8.33254 | 0.999996 | 0.8263 | 0.492 | 176.693 | 4.63569 | A | F | 7.6e+21 | 2.58478e-14 | 1 | dx | ||||
| Report | 3 | X175509.76-274938.4 | chandra | ccd3 | 989 | 288 | 3.89975 | 2 | 0.001808 | 0.000927239 | 8.26911 | 0.999996 | 1.89056 | 0.492 | 90 | 9.61696 | A | F | 7.93e+21 | 0 | 1 | d | |||||
| Report | 2 | X175546.32-275148.7 | chandra | ccd1 | 1053.17 | 212.833 | 2.94816 | 1.73205 | 0.00136682 | 0.000803012 | 6.23359 | 0.999913 | 1.2553 | 0.492 | 87.7577 | 7.94865 | A | F | 7.45e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X175536.16-274050.5 | chandra | ccd2 | 456.5 | 347.5 | 2.93544 | 2.00003 | 0.00136092 | 0.000927252 | 6.28995 | 0.999921 | 1.99374 | 1.06351 | 68.9554 | 3.55385 | A | F | 7.9e+21 | 1.95269e-14 | 1 | dx | ||||
| Report | 1 | X175602.99-274508.3 | chandra | ccd1 | 603.5 | 1026.5 | 1.98642 | 1.41421 | 0.000920942 | 0.000655656 | 4.20009 | 0.998421 | 0.492 | 0.492 | 90 | 4.27169 | F | F | 7.47e+21 | 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