Source List

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 1 X174354.86-294443.2 chandra ccd3 1162.28 978.084 35265.7 187.792 3.03725 0.0161735 9505.8 1 4.11844 4.11844 0 7.89418 F F 1.27e+22 1.23447e-10 1 dsxf
Report srcpi bgdpi arf 8 X174421.58-294710.2 chandra ccd3 455.183 679.197 41.6621 7.42784 0.00358814 0.00063972 11.2299 1 1.0862 1.0862 0 6.7051 F F 1.25e+22 6.09287e-14 1 dsx
Report srcpi bgdpi arf 3 X174418.97-294418.5 chandra ccd3 523.99 1028.25 18.1361 6.77612 0.00156197 0.000583591 4.88855 0.999981 1.57354 1.57354 0 8.87647 F F 1.25e+22 2.78008e-14 1 dsx
Report srcpi bgdpi arf 7 X174419.17-294347.4 chandra ccd3 518.262 1090.98 16.0493 4.58264 0.00138224 0.000394678 4.32606 0.999898 2.98383 1.77499 35.0988 9.38172 A F 1.25e+22 2.49414e-14 1 dx
Report srcpi bgdpi arf 4 X174430.02-295356.4 chandra ccd2 455.735 856.304 13.1927 4.77203 0.00113622 0.000410991 4.26246 0.999837 1.95464 0.513483 96.3532 6.16497 F F 1.24e+22 1.92669e-14 1 dsx
Report srcpi bgdpi arf 5 X174419.23-294652.7 chandra ccd3 516.889 714.222 15.1974 4.24268 0.00130887 0.000365399 4.09643 0.999772 1.9294 0.998417 105.735 6.64767 A F 1.25e+22 2.21392e-14 1 dx
Report srcpi bgdpi arf 2 X174425.73-294755.9 chandra ccd3 344.9 585.767 13.9948 3.873 0.0012053 0.00033356 3.77228 0.999508 1.00377 0.628661 171.732 6.77095 A T 1.25e+22 2.38303e-14 1 dx
Report srcpi bgdpi arf 2 X174420.14-295452.1 chandra ccd2 716.269 742.885 12.4513 3.60556 0.00107236 0.000310527 4.02292 0.999837 0.996351 0.492 125.494 4.5394 A T 1.25e+22 1.78143e-14 1 dpx
Report srcpi bgdpi arf 1 X174345.70-295040.1 chandra ccd1 368.246 494.529 17.7201 4.20952 0.00152614 0.000362545 13.7919 1 0.871583 0.871583 0 4.04876 F F 1.27e+22 2.43085e-14 1 dsx
Report 1 X174357.56-295748.0 chandra ccd0 318 616.4 9.78888 3.16228 0.000843063 0.00027235 10.8521 1 0.70328 0.650478 143.872 5.46291 F F 1.26e+22 0 1 d
Report srcpi bgdpi arf 2 X174341.63-295324.9 chandra ccd1 475.167 158.944 8.55725 3.00001 0.00073699 0.000258375 6.66029 0.999999 0.814459 0.492 12.489 4.61579 A T 1.27e+22 1.18108e-14 1 dx
Report srcpi bgdpi arf 6 X174407.22-294428.7 chandra ccd3 834.5 1007 7.57325 3.16232 0.000652243 0.000272354 2.04136 0.975405 1.19315 0.638555 151.898 8.02948 A F 1.26e+22 1.12683e-14 1 dx
Report srcpi bgdpi arf 3 X174429.77-295225.5 chandra ccd2 461.643 1040.64 6.65687 2.64576 0.00057332 0.000227865 2.15078 0.980985 0.665892 0.492 29.8718 5.92334 F F 1.24e+22 1.02277e-14 1 dx
Report srcpi bgdpi arf 2 X174359.32-295412.5 chandra ccd0 271.667 1054.5 5.7622 2.44949 0.000496267 0.000210962 6.38809 0.999977 0.736784 0.492 150.521 1.89266 T T 1.26e+22 8.08953e-15 1 dx
Report srcpi bgdpi arf 3 X174329.58-295729.6 chandra ccd0 1057.17 653.333 4.91395 2.44952 0.000423212 0.000210963 5.44771 0.999798 1.69829 1.45333 19.4176 8.7321 F F 1.28e+22 7.46717e-15 1 dx
Report srcpi bgdpi arf 4 X174400.80-295342.5 chandra ccd0 232.5 1115.5 3.85464 2.00001 0.000331979 0.00017225 4.27333 0.998481 0.492 0.492 45 1.31616 F F 1.26e+22 1.07748e-14 1 dx
Report srcpi bgdpi arf 5 X174344.30-295519.0 chandra ccd0 668.5 919.167 2.89176 1.73205 0.000249052 0.000149172 3.20586 0.990387 0.621484 0.492 165.695 4.87196 F F 1.27e+22 4.13864e-15 1 dx
Report srcpi bgdpi arf 6 X174350.94-295911.3 chandra ccd0 493.16 447.603 29.3801 5.42061 0.00253035 0.000466848 32.5714 1 1.77283 1.77283 0 7.18682 F F 1.26e+22 4.38727e-14 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