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 | X142515.84+230337.7 | chandra | ccd7 | 693.531 | 486.069 | 44.6606 | 6.96809 | 0.00949968 | 0.00148217 | 20.2083 | 1 | 0.467588 | 0.318987 | 85.5673 | 1.13404 | F | F | 3.29e+20 | 6.21445e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X142517.08+230223.5 | chandra | ccd7 | 658.514 | 335.454 | 33.5823 | 6.28148 | 0.00714322 | 0.00133612 | 15.1955 | 1 | 0.47607 | 0.47607 | 0 | 1.19501 | F | F | 3.3e+20 | 4.67437e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X142429.60+231117.4 | chandra | ccd3 | 839.824 | 688.647 | 23.7543 | 5.8311 | 0.00505271 | 0.00124032 | 45.097 | 1 | 7.49321 | 3.21391 | 137.455 | 12.9452 | A | F | 3.16e+20 | 6.86658e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142447.31+231034.7 | chandra | ccd3 | 343.636 | 601.545 | 18.356 | 4.69047 | 0.00390444 | 0.000997694 | 34.8483 | 1 | 3.62578 | 2.05669 | 22.4169 | 9.63201 | A | F | 3.2e+20 | 5.17363e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142458.11+230517.2 | chandra | ccd7 | 1190.1 | 687.9 | 9.64361 | 3.16229 | 0.00205126 | 0.00067264 | 4.36361 | 0.999823 | 0.69311 | 0.541288 | 62.7688 | 4.07064 | F | F | 3.25e+20 | 1.61279e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142444.99+231115.8 | chandra | ccd3 | 408.722 | 685.056 | 7.74709 | 3.00002 | 0.00164786 | 0.000638126 | 14.7077 | 1 | 3.49476 | 1.20827 | 15.018 | 10.5 | A | F | 3.19e+20 | 2.20857e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X142414.48+230314.9 | chandra | ccd2 | 794.375 | 676.625 | 6.99771 | 2.82845 | 0.00148846 | 0.000601631 | 13.9201 | 1 | 2.09589 | 1.46243 | 106.92 | 13.3018 | F | F | 3.17e+20 | 2.01178e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142528.13+230504.4 | chandra | ccd7 | 348.214 | 661.929 | 6.86272 | 2.64575 | 0.00145975 | 0.00056277 | 3.10529 | 0.995438 | 0.492 | 0.492 | 47.1994 | 4.27486 | F | F | 3.31e+20 | 1.0143e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X142449.36+230846.4 | chandra | ccd3 | 286.3 | 381.3 | 4.85052 | 2.23607 | 0.00103174 | 0.000475628 | 9.20858 | 1 | 0.492 | 0.492 | 19.3299 | 7.93204 | F | F | 3.21e+20 | 1.32733e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X142446.85+225843.1 | chandra | ccd6 | 1049.5 | 843.1 | 4.588 | 2.23608 | 0.0009759 | 0.000475629 | 8.95164 | 0.999992 | 1.43345 | 0.769532 | 27.504 | 7.15795 | A | F | 3.25e+20 | 1.12154e-14 | 1 | dx | ||||
| Report | 2 | X142503.40+225752.7 | chandra | ccd6 | 585 | 740.5 | 3.98282 | 2 | 0.000847174 | 0.000425414 | 7.77087 | 0.999992 | 0.492 | 0.492 | 180 | 5.36853 | F | F | 3.29e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X142510.49+225857.8 | chandra | ccd6 | 386 | 872.75 | 3.95678 | 2 | 0.000841634 | 0.000425414 | 7.72005 | 0.999992 | 0.492 | 0.492 | 109.33 | 3.90225 | F | F | 3.3e+20 | 8.38927e-15 | 1 | dx | ||||
| Report | 3 | X142515.41+225910.6 | chandra | ccd6 | 248 | 898.75 | 3.95455 | 2 | 0.00084116 | 0.000425414 | 7.71571 | 0.999992 | 0.492 | 0.492 | 37.9819 | 3.73777 | F | F | 3.31e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X142503.15+225520.7 | chandra | ccd6 | 592.25 | 431.5 | 3.80981 | 2.00001 | 0.000810373 | 0.000425415 | 7.43331 | 0.999992 | 1.50088 | 0.492 | 117.701 | 7.78773 | A | F | 3.3e+20 | 8.69199e-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