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 | X151544.62-370901.4 | chandra | ccd7 | 336.852 | 699.116 | 43.3087 | 6.58093 | 0.00136529 | 0.000207462 | 14.9319 | 1 | 0.422939 | 0.422939 | 0 | 0.857497 | F | F | 6.88e+20 | 1.07648e-14 | 1 | dspx | ||||
| Report | srcpi bgdpi arf rmf | 2 | X151548.44-370916.4 | chandra | ccd7 | 243.89 | 668.661 | 941.168 | 31.4157 | 0.02967 | 0.000990369 | 324.494 | 1 | 0.417807 | 0.417807 | 0 | 0.308533 | F | F | 6.87e+20 | 1.12817e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 3 | X151545.24-371112.4 | chandra | ccd7 | 321.25 | 432.25 | 7.14148 | 2.82845 | 0.000225133 | 8.91659e-05 | 2.46222 | 0.987318 | 0.492 | 0.492 | 118.155 | 2.34545 | F | F | 6.85e+20 | 2.19669e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X151545.73-371049.4 | chandra | ccd7 | 309.817 | 479.631 | 10.6336 | 4.54592 | 0.000335222 | 0.000143309 | 3.66623 | 0.999529 | 0.285794 | 0.285794 | 0 | 1.94729 | F | F | 6.85e+20 | 2.51855e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X151543.57-371024.4 | chandra | ccd7 | 362.21 | 530.411 | 13.804 | 4.7608 | 0.000435168 | 0.000150083 | 4.75931 | 0.999975 | 0.64365 | 0.64365 | 0 | 1.78159 | F | F | 6.86e+20 | 3.27319e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X151547.89-371009.9 | chandra | ccd7 | 256.875 | 559.25 | 7.0991 | 2.82845 | 0.000223797 | 8.91658e-05 | 2.44761 | 0.987318 | 0.492 | 0.492 | 84.4354 | 1.20435 | F | F | 6.86e+20 | 1.67593e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X151552.81-370945.6 | chandra | ccd7 | 137.834 | 609.288 | 21.8301 | 5.40698 | 0.000688187 | 0.000170453 | 7.52654 | 1 | 0.522742 | 0.522742 | 0 | 1.10052 | F | F | 6.86e+20 | 7.8209e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X151541.43-370945.0 | chandra | ccd7 | 413.625 | 610 | 7.20457 | 2.82844 | 0.000227121 | 8.91657e-05 | 2.48398 | 0.987318 | 0.492 | 0.492 | 155.593 | 1.67697 | F | F | 6.87e+20 | 1.70954e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X151555.67-370845.5 | chandra | ccd7 | 68.3215 | 731.44 | 14.9966 | 4.1639 | 0.000472764 | 0.000131266 | 5.1705 | 0.999992 | 0.500622 | 0.500622 | 0 | 1.36412 | F | F | 6.88e+20 | 3.60017e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 10 | X151552.21-370822.4 | chandra | ccd7 | 152.225 | 778.256 | 14.2936 | 4.11598 | 0.0004506 | 0.000129755 | 4.92812 | 0.999975 | 0.894582 | 0.279597 | 19.358 | 0.89269 | A | F | 6.89e+20 | 3.42152e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 11 | X151534.78-371148.0 | chandra | ccd7 | 575.227 | 359.864 | 9.21596 | 3.31666 | 0.00029053 | 0.000104556 | 3.17746 | 0.9973 | 0.700116 | 0.600469 | 145.162 | 3.98553 | F | F | 6.84e+20 | 2.25206e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 13 | X151550.89-370907.5 | chandra | ccd7 | 184 | 686.25 | 9.32798 | 3.46415 | 0.000294061 | 0.000109206 | 3.21608 | 0.9973 | 0.73698 | 0.536666 | 159.077 | 0.41965 | T | F | 6.88e+20 | 2.20677e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 14 | X151532.35-371202.9 | chandra | ccd7 | 634.746 | 330.019 | 38.6795 | 6.81259 | 0.00121936 | 0.000214765 | 13.3358 | 1 | 1.0059 | 1.0059 | 0 | 4.50832 | F | F | 6.84e+20 | 9.5068e-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