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 | X175404.83-285313.5 | chandra | ccd0 | 456.961 | 537.808 | 12.4213 | 3.60556 | 0.00576691 | 0.00167398 | 24.0013 | 1 | 2.37515 | 0.492 | 4.5833 | 7.22891 | A | F | 6.47e+21 | 8.42293e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X175312.44-284745.5 | chandra | ccd2 | 839.045 | 1010.59 | 9.21991 | 3.31666 | 0.00428059 | 0.00153985 | 18.1507 | 1 | 2.37052 | 2.12751 | 27.8278 | 9.89765 | F | F | 7.26e+21 | 7.20251e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X175338.95-285658.4 | chandra | ccd1 | 964.833 | 1100.06 | 8.94692 | 3 | 0.00415385 | 0.00139283 | 16.8748 | 1 | 0.492 | 0.492 | 134.132 | 1.0734 | F | F | 6.65e+21 | 5.59187e-14 | 1 | dx | ||||
| Report | 3 | X175333.12-285910.3 | chandra | ccd3 | 109.357 | 656.928 | 6.94231 | 2.64575 | 0.0032278 | 0.00123013 | 12.7169 | 1 | 0.492 | 0.492 | 170.008 | 2.86767 | F | F | 6.64e+21 | 0 | 1 | d | |||||
| Report | 2 | X175350.02-285815.5 | chandra | ccd1 | 669.5 | 943.357 | 6.93109 | 2.64575 | 0.00321795 | 0.00122836 | 13.0727 | 1 | 0.570909 | 0.492 | 14.1504 | 3.80623 | F | F | 6.45e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X175401.12-290043.5 | chandra | ccd1 | 373.786 | 642.214 | 6.66158 | 2.64576 | 0.00309282 | 0.00122837 | 12.5644 | 1 | 1.41309 | 0.968292 | 114.308 | 7.20379 | F | F | 6.2e+21 | 4.67854e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X175318.91-290030.5 | chandra | ccd3 | 488.333 | 493.833 | 5.9327 | 2.44949 | 0.00275839 | 0.00113888 | 10.8675 | 1 | 0.539971 | 0.492 | 31.1503 | 5.46134 | F | F | 6.78e+21 | 3.91142e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X175328.24-285433.5 | chandra | ccd2 | 416.7 | 181.5 | 4.95671 | 2.23607 | 0.00230129 | 0.00103816 | 9.75798 | 1 | 0.492 | 0.492 | 2.37139e-08 | 2.31241 | F | F | 6.86e+21 | 3.12063e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X175323.72-285353.4 | chandra | ccd2 | 537.25 | 263 | 3.95992 | 2 | 0.0018385 | 0.000928555 | 7.79566 | 0.999992 | 0.492 | 0.492 | 46.4312 | 3.47467 | F | F | 6.93e+21 | 2.56976e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X175356.58-290109.5 | chandra | ccd1 | 495 | 589.5 | 3.68775 | 2.00001 | 0.00171214 | 0.000928559 | 6.95547 | 0.999792 | 1.368 | 0.639746 | 128.953 | 6.74675 | A | F | 6.25e+21 | 2.44851e-14 | 1 | dx | ||||
| Report | 1 | X175339.95-285822.5 | chandra | ccd1 | 938.167 | 929.167 | 2.95791 | 1.73205 | 0.00137329 | 0.000804152 | 5.57892 | 0.999792 | 0.639127 | 0.492 | 45 | 2.30911 | F | F | 6.59e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X175316.18-285036.8 | chandra | ccd2 | 738.833 | 662.5 | 2.89942 | 1.73205 | 0.00134613 | 0.000804153 | 5.70791 | 0.99985 | 0.510281 | 0.492 | 28.155 | 7.0508 | F | F | 7.14e+21 | 2.33824e-14 | 1 | dx | ||||
| Report | 2 | X175308.53-290012.4 | chandra | ccd3 | 765.167 | 530.5 | 2.87794 | 1.73206 | 0.00133809 | 0.000805313 | 5.27179 | 0.999741 | 0.492 | 0.492 | 2.8684e-08 | 6.96724 | F | F | 6.92e+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