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 | 6 | X175550.82-340910.5 | chandra | ccd2 | 665.413 | 366.882 | 43.3034 | 7.02477 | 0.00838795 | 0.00136071 | 17.6141 | 1 | 1.09534 | 0.536119 | 72.3998 | 4.57371 | F | F | 2.49e+21 | 1.01301e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X175635.83-341059.7 | chandra | ccd0 | 547.12 | 368.66 | 26.7026 | 5.16746 | 0.00517234 | 0.00100095 | 8.86953 | 1 | 3.47482 | 1.68832 | 7.89237 | 6.2753 | A | F | 2.41e+21 | 6.35047e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X175625.98-342020.1 | chandra | ccd1 | 596.302 | 241.812 | 13.9473 | 5.85958 | 0.00270162 | 0.00113501 | 3.08894 | 0.997978 | 1.62094 | 1.62094 | 0 | 8.88316 | F | F | 2.39e+21 | 3.65633e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X175605.37-341338.2 | chandra | ccd3 | 77.3322 | 849.935 | 13.9238 | 4.10344 | 0.00269707 | 0.000794844 | 8.1561 | 1 | 0.32964 | 0.32964 | 0 | 1.19889 | F | F | 2.43e+21 | 3.02741e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X175607.35-341935.4 | chandra | ccd1 | 1064.86 | 332.357 | 11.7628 | 3.74169 | 0.00227847 | 0.000724771 | 2.60514 | 0.993808 | 1.88254 | 1.05546 | 99.4065 | 7.143 | A | F | 2.39e+21 | 2.91932e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X175559.23-340340.2 | chandra | ccd2 | 452.967 | 1037.83 | 11.571 | 3.87304 | 0.00224131 | 0.000750213 | 4.7066 | 0.999938 | 2.52068 | 2.50831 | 128.252 | 8.89993 | F | T | 2.52e+21 | 3.01843e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X175635.72-341003.7 | chandra | ccd0 | 549.192 | 481.961 | 11.3566 | 3.60558 | 0.00219979 | 0.000698405 | 3.77222 | 0.99952 | 1.3183 | 0.904282 | 18.8363 | 6.54927 | F | F | 2.42e+21 | 2.71562e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X175652.11-340947.2 | chandra | ccd0 | 136.128 | 515.375 | 54.4876 | 8.52144 | 0.0105543 | 0.00165062 | 18.0986 | 1 | 4.08088 | 4.08088 | 0 | 9.84432 | F | F | 2.43e+21 | 1.45477e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X175546.73-340752.0 | chandra | ccd2 | 768.136 | 525.955 | 9.87525 | 3.31664 | 0.00191285 | 0.000642438 | 4.01685 | 0.99945 | 1.15619 | 0.697288 | 142.515 | 6.10682 | A | F | 2.51e+21 | 2.39811e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X175600.35-341538.3 | chandra | ccd3 | 203.3 | 605.2 | 9.64256 | 3.16228 | 0.00186778 | 0.000612538 | 5.64829 | 0.999988 | 0.758488 | 0.492 | 45.3892 | 3.41221 | A | F | 2.42e+21 | 2.17988e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X175558.61-341745.9 | chandra | ccd3 | 247 | 345.9 | 9.5229 | 3.16229 | 0.0018446 | 0.000612539 | 5.5782 | 0.999988 | 0.559214 | 0.492 | 13.1407 | 5.54273 | F | F | 2.41e+21 | 2.2791e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X175601.30-341756.5 | chandra | ccd3 | 179.2 | 324.4 | 9.44496 | 3.16229 | 0.0018295 | 0.000612539 | 5.53254 | 0.999988 | 0.853188 | 0.492 | 40.8538 | 5.58437 | A | F | 2.41e+21 | 2.25259e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X175548.74-341509.9 | chandra | ccd3 | 495.833 | 662.944 | 8.71579 | 3.00001 | 0.00168826 | 0.000581105 | 5.10542 | 0.999945 | 0.616372 | 0.492 | 101.599 | 4.52066 | F | T | 2.45e+21 | 2.04912e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X175614.73-341411.8 | chandra | ccd1 | 878.944 | 990.167 | 8.7145 | 3.00001 | 0.00168801 | 0.000581105 | 1.93002 | 0.972895 | 0.492 | 0.492 | 25.0972 | 2.47523 | F | F | 2.41e+21 | 1.90101e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X175605.62-341702.7 | chandra | ccd1 | 1108.39 | 642.833 | 8.52085 | 3.00002 | 0.0016505 | 0.000581107 | 1.88713 | 0.958076 | 0.832323 | 0.564979 | 46.2896 | 4.5951 | F | T | 2.41e+21 | 1.97095e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X175602.19-340454.8 | chandra | ccd2 | 378.2 | 886.3 | 8.47439 | 3.16231 | 0.0016415 | 0.000612543 | 3.44704 | 0.998499 | 1.55172 | 0.832195 | 60.1348 | 7.5847 | A | F | 2.51e+21 | 2.10129e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X175538.34-341231.7 | chandra | ccd3 | 758.375 | 984.125 | 7.7479 | 2.82843 | 0.00150078 | 0.000547871 | 4.53846 | 0.99977 | 0.492 | 0.492 | 11.3099 | 5.76824 | F | F | 2.49e+21 | 1.91231e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X175553.58-340327.8 | chandra | ccd2 | 595.722 | 1062.94 | 6.71662 | 3.00005 | 0.00130102 | 0.000581113 | 2.73205 | 0.990666 | 2.55258 | 1.261 | 87.8666 | 9.36136 | A | F | 2.54e+21 | 1.79175e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X175602.37-340713.9 | chandra | ccd2 | 373.5 | 603.5 | 5.7153 | 2.4495 | 0.00110706 | 0.00047447 | 2.32475 | 0.978899 | 0.707722 | 0.492 | 112.5 | 5.28018 | F | F | 2.49e+21 | 1.32397e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 10 | X175601.65-341406.5 | chandra | ccd3 | 170.667 | 791.833 | 5.71084 | 2.4495 | 0.0011062 | 0.000474471 | 3.34522 | 0.996843 | 0.492 | 0.492 | 32.8861 | 1.90992 | F | F | 2.43e+21 | 1.25347e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X175540.90-341935.6 | chandra | ccd3 | 692.9 | 122.7 | 4.13024 | 2.23609 | 0.000800033 | 0.000433134 | 2.41936 | 0.989841 | 1.65337 | 0.492 | 97.2714 | 8.85479 | A | F | 2.42e+21 | 1.11672e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X175538.98-341141.2 | chandra | ccd3 | 742.25 | 1086.75 | 3.76215 | 2.00001 | 0.000728733 | 0.000387404 | 2.20374 | 0.970623 | 0.586816 | 0.492 | 51.6203 | 5.68654 | F | F | 2.49e+21 | 9.27534e-15 | 1 | dx |
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