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 | 3 | X175440.83-271952.3 | chandra | ccd7 | 513.399 | 572.977 | 175.079 | 14.6402 | 0.0815168 | 0.00681645 | 27.9438 | 1 | 12.7516 | 7.63845 | 92.0988 | 14.3563 | F | F | 9.67e+21 | 6.90284e-13 | 1 | dscxf | ||||
| Report | srcpi bgdpi arf | 4 | X175540.75-271417.5 | chandra | ccd2 | 373.647 | 624.339 | 32.0355 | 6.1818 | 0.0149158 | 0.00287825 | 12.8875 | 1 | 1.90323 | 0.719094 | 55.8106 | 5.46612 | F | F | 8.89e+21 | 2.29143e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X175440.48-271944.4 | chandra | ccd7 | 522.577 | 588.539 | 19.3366 | 5.09913 | 0.00900313 | 0.00237415 | 3.08626 | 0.99805 | 4.54798 | 1.49217 | 7.22808 | 14.4453 | A | F | 9.68e+21 | 1.83078e-13 | 1 | dcx | ||||
| Report | 1 | X175542.05-272235.1 | chandra | ccd3 | 154.944 | 639.5 | 8.92782 | 3 | 0.00415679 | 0.0013968 | 19.1871 | 1 | 0.723575 | 0.492 | 98.6207 | 3.03103 | F | F | 8.53e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X175610.97-271427.1 | chandra | ccd0 | 588 | 769.167 | 8.75801 | 3 | 0.00407773 | 0.0013968 | 19.7827 | 1 | 0.632098 | 0.504759 | 144.928 | 7.6847 | F | F | 8.44e+21 | 6.55063e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X175539.03-272319.0 | chandra | ccd3 | 236.5 | 550.3 | 4.9632 | 2.23607 | 0.00231086 | 0.00104111 | 10.6666 | 1 | 0.492 | 0.492 | 145.901 | 3.9355 | F | F | 8.53e+21 | 3.32023e-14 | 1 | dx | ||||
| Report | 2 | X175543.74-272413.9 | chandra | ccd3 | 109 | 438.75 | 3.96271 | 2 | 0.00184504 | 0.0009312 | 8.51641 | 0.999997 | 0.492 | 0.492 | 11.9812 | 4.59454 | F | F | 8.41e+21 | 0 | 1 | d | |||||
| Report | 2 | X175554.50-272528.8 | chandra | ccd1 | 824 | 473.5 | 3.91341 | 2 | 0.00182209 | 0.000931201 | 8.55577 | 0.999997 | 0.897793 | 0.492 | 149.679 | 6.15743 | A | F | 8.21e+21 | 0 | 1 | d | |||||
| Report | 1 | X175603.88-272415.8 | chandra | ccd1 | 570 | 621.75 | 3.88538 | 2 | 0.00180903 | 0.000931202 | 8.49447 | 0.999997 | 0.561567 | 0.492 | 9.99155 | 6.15347 | F | F | 8.13e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X175510.98-272043.3 | chandra | ccd3 | 996.25 | 866.25 | 3.83389 | 2.00001 | 0.00178506 | 0.000931202 | 8.23956 | 0.999997 | 0.825109 | 0.492 | 45 | 7.74363 | A | F | 9.05e+21 | 2.97691e-14 | 1 | dx | ||||
| Report | 3 | X175552.64-272057.7 | chandra | ccd1 | 874.167 | 1024.5 | 2.98149 | 1.73205 | 0.00138818 | 0.000806443 | 6.51834 | 0.999932 | 0.492 | 0.492 | 180 | 2.05205 | F | F | 8.46e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X175609.03-272003.8 | chandra | ccd0 | 641.167 | 84.8333 | 2.97277 | 1.73205 | 0.00138412 | 0.000806443 | 6.71494 | 0.999947 | 0.569535 | 0.492 | 53.3496 | 5.23821 | F | F | 8.25e+21 | 2.07943e-14 | 1 | dx | ||||
| Report | 3 | X175618.02-271218.5 | chandra | ccd0 | 396.7 | 1030.3 | 4.77843 | 2.23608 | 0.00222484 | 0.00104112 | 10.7936 | 0.999998 | 0.665687 | 0.492 | 37.2379 | 10.3015 | F | F | 8.41e+21 | 0 | 1 | d | |||||
| Report | 4 | X175609.28-271848.7 | chandra | ccd0 | 634.167 | 237.5 | 2.96147 | 1.73205 | 0.00137886 | 0.000806443 | 6.68941 | 0.999947 | 0.627179 | 0.492 | 180 | 5.34592 | F | F | 8.3e+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