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 | 3 | X215841.94-011500.3 | chandra | ccd7 | 652.527 | 878.438 | 78.9556 | 8.90432 | 0.0203525 | 0.00229529 | 90.0978 | 1 | 0.358918 | 0.358918 | 0 | 0.301735 | F | F | 5.94e+20 | 1.50615e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X215837.18-011359.4 | chandra | ccd7 | 797.519 | 1002.12 | 20.4129 | 4.51806 | 0.00526188 | 0.00116463 | 23.2936 | 1 | 0.532318 | 0.532318 | 0 | 1.2624 | F | F | 5.96e+20 | 3.95908e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X215914.50-011622.7 | chandra | ccd3 | 1031.01 | 617.968 | 17.9943 | 5.00113 | 0.00463843 | 0.00128915 | 6.79294 | 1 | 2.76489 | 2.76489 | 0 | 8.49775 | F | F | 5.77e+20 | 6.15799e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X215842.88-011500.0 | chandra | ccd7 | 623.859 | 878.953 | 14.5659 | 3.81653 | 0.00375469 | 0.000983797 | 16.6214 | 1 | 0.561444 | 0.308248 | 234.789 | 0.494621 | F | F | 5.94e+20 | 2.77537e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X215841.77-011635.4 | chandra | ccd7 | 657.1 | 684.5 | 9.85185 | 3.16228 | 0.0025395 | 0.000815138 | 11.2421 | 1 | 0.492 | 0.492 | 171.061 | 1.80804 | F | F | 5.96e+20 | 1.89267e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X215914.67-011425.4 | chandra | ccd3 | 1025.41 | 855.773 | 9.75544 | 3.31665 | 0.00251465 | 0.000854929 | 3.68273 | 0.999017 | 2.97904 | 1.39909 | 66.5112 | 8.40147 | A | F | 5.74e+20 | 3.31267e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X215850.49-011420.5 | chandra | ccd7 | 391.25 | 958.75 | 7.81253 | 2.82843 | 0.00201383 | 0.000729082 | 8.91503 | 1 | 0.492 | 0.492 | 144.992 | 2.39383 | F | F | 5.88e+20 | 1.52172e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X215939.39-011006.5 | chandra | ccd2 | 44.75 | 368 | 6.37538 | 2.82848 | 0.00164338 | 0.000729095 | 11.7911 | 1 | 4.6177 | 3.21337 | 87.9588 | 15.3071 | F | F | 5.54e+20 | 2.43485e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X215849.00-011406.3 | chandra | ccd7 | 436.833 | 987.667 | 5.83111 | 2.44949 | 0.00150308 | 0.000631404 | 6.65399 | 0.999984 | 0.492 | 0.492 | 175.787 | 2.09319 | F | F | 5.89e+20 | 1.13043e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X215836.64-010801.7 | chandra | ccd6 | 586.333 | 720.667 | 5.65921 | 2.4495 | 0.00145877 | 0.000631405 | 10.0778 | 0.999999 | 0.867438 | 0.745794 | 121.224 | 6.85272 | F | F | 5.89e+20 | 1.67463e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X215845.84-011359.3 | chandra | ccd7 | 533.1 | 1001.9 | 4.90314 | 2.23607 | 0.00126388 | 0.00057639 | 5.59507 | 0.999852 | 0.605164 | 0.492 | 25.0972 | 1.43395 | T | F | 5.91e+20 | 9.45521e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X215846.84-011652.2 | chandra | ccd7 | 502.5 | 650.5 | 3.84026 | 2.00001 | 0.0009899 | 0.000515539 | 4.3822 | 0.998819 | 0.492 | 0.492 | 45 | 2.52824 | F | F | 5.93e+20 | 7.45335e-15 | 1 | dx | ||||
| Report | 2 | X215848.85-011008.7 | chandra | ccd6 | 214.167 | 462.5 | 2.97302 | 1.73205 | 0.000766352 | 0.000446469 | 5.2943 | 0.999679 | 0.492 | 0.492 | 180 | 5.03491 | F | F | 5.84e+20 | 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