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 | X181921.05-252536.2 | chandra | ccd7 | 97.7168 | 144.517 | 43.3008 | 7.6051 | 0.00118809 | 0.000208669 | 10.7394 | 1 | 0.544983 | 0.544983 | 0 | 0.633605 | F | F | 1.81e+21 | 9.19895e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X181919.96-252224.5 | chandra | ccd7 | 127.732 | 534.169 | 23.6931 | 5.76009 | 0.000650092 | 0.000158046 | 5.87634 | 1 | 0.573811 | 0.573811 | 0 | 2.58533 | F | F | 1.81e+21 | 5.15048e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X181921.87-252151.3 | chandra | ccd7 | 75.1264 | 601.652 | 17.1491 | 6.16994 | 0.000470536 | 0.00016929 | 4.2533 | 0.999919 | 0.476067 | 0.476067 | 0 | 3.12829 | F | F | 1.81e+21 | 3.75615e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X181921.63-252039.9 | chandra | ccd7 | 81.7771 | 746.78 | 27.572 | 7.68151 | 0.000756519 | 0.000210765 | 6.83838 | 1 | 0.612403 | 0.612403 | 0 | 4.30853 | F | F | 1.81e+21 | 6.14475e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X181920.90-252033.4 | chandra | ccd7 | 101.955 | 759.961 | 47.1456 | 7.45771 | 0.00129358 | 0.000204624 | 11.693 | 1 | 0.90032 | 0.90032 | 0 | 4.42045 | F | F | 1.81e+21 | 1.04877e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X181919.02-251854.7 | chandra | ccd7 | 153.768 | 960.574 | 27.9789 | 7.51355 | 0.000767685 | 0.000206157 | 6.9393 | 1 | 1.5219 | 1.5219 | 0 | 6.08873 | F | F | 1.82e+21 | 6.56307e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 8 | X181921.74-252601.1 | chandra | ccd7 | 78.8268 | 93.9438 | 1287.82 | 36.7261 | 0.0353352 | 0.00100769 | 319.404 | 1 | 0.440296 | 0.440296 | 0 | 1.05023 | F | F | 1.81e+21 | 3.12315e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 9 | X181920.27-252531.2 | chandra | ccd7 | 118.667 | 154.167 | 9.65473 | 3.46415 | 0.000264906 | 9.50491e-05 | 2.39456 | 0.984345 | 0.505465 | 0.492 | 136.95 | 0.596318 | F | F | 1.81e+21 | 2.03847e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X181921.26-252530.3 | chandra | ccd7 | 91.4165 | 156 | 9.62792 | 3.46414 | 0.00026417 | 9.5049e-05 | 2.38791 | 0.984345 | 0.492 | 0.492 | 119.872 | 0.533127 | F | F | 1.81e+21 | 2.01768e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 11 | X181921.62-252425.6 | chandra | ccd7 | 82.0342 | 287.928 | 19.5067 | 5.48891 | 0.000535225 | 0.000150605 | 4.83803 | 0.999984 | 0.574363 | 0.574363 | 0 | 0.550221 | F | F | 1.81e+21 | 4.10246e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 12 | X181922.03-252352.6 | chandra | ccd7 | 70.7029 | 355.073 | 13.6803 | 5.57303 | 0.000375359 | 0.000152912 | 3.39297 | 0.998568 | 0.518154 | 0.518154 | 0 | 1.10662 | F | F | 1.81e+21 | 2.88548e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 13 | X181920.45-252615.0 | chandra | ccd7 | 113.75 | 65 | 9.52928 | 3.46415 | 0.000261464 | 9.50492e-05 | 2.36344 | 0.984345 | 0.730605 | 0.492 | 112.624 | 1.29394 | T | F | 1.81e+21 | 2.01732e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 14 | X181923.37-252627.1 | chandra | ccd7 | 33.7779 | 41.0334 | 21.0481 | 4.94088 | 0.000577517 | 0.000135568 | 5.22033 | 0.999997 | 0.396364 | 0.396364 | 0 | 1.55258 | F | F | 1.8e+21 | 4.48265e-15 | 1 | dsx |
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