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 | X152235.89+273657.2 | chandra | ccd2 | 811.455 | 562.409 | 19.8471 | 5.29742 | 0.00391496 | 0.00104495 | 9.34708 | 1 | 0.889951 | 0.889951 | 0 | 4.50684 | F | F | 3.11e+20 | 4.79289e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X152235.46+273455.2 | chandra | ccd2 | 823.048 | 314.506 | 11.1643 | 4.05513 | 0.00220221 | 0.000799894 | 5.25788 | 0.999979 | 0.918441 | 0.918441 | 0 | 6.21583 | F | F | 3.14e+20 | 2.94756e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X152228.26+274017.1 | chandra | ccd2 | 1017.61 | 968.624 | 14.102 | 3.75932 | 0.00278171 | 0.000741549 | 6.6414 | 1 | 0.426802 | 0.426802 | 0 | 1.03401 | F | F | 3.06e+20 | 3.2234e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X152231.17+274221.4 | chandra | ccd3 | 721.02 | 238.361 | 11.4126 | 4.58369 | 0.00225257 | 0.000904711 | 3.68385 | 0.999588 | 0.865511 | 0.419905 | 328.473 | 2.41134 | F | F | 3.03e+20 | 2.63282e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X152229.45+274220.6 | chandra | ccd3 | 767 | 236.278 | 11.4414 | 4.24274 | 0.00225825 | 0.000837412 | 3.69314 | 0.999588 | 0.86327 | 0.557542 | 179.002 | 2.16569 | A | F | 3.03e+20 | 2.76646e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 1 | X152154.72+274239.3 | chandra | ccd1 | 686.417 | 464.667 | 11.1079 | 3.46412 | 0.00219108 | 0.000683314 | 11.4087 | 1 | 1.56994 | 0.887175 | 163.236 | 6.76018 | A | F | 2.99e+20 | 2.74682e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X152251.83+273418.6 | chandra | ccd2 | 379.917 | 239.833 | 10.8227 | 3.46412 | 0.00213482 | 0.000683315 | 5.09698 | 0.999979 | 2.42026 | 1.05097 | 114.416 | 8.8265 | A | F | 3.16e+20 | 3.27507e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X152211.41+273500.4 | chandra | ccd0 | 442.2 | 561.5 | 9.19469 | 3.16229 | 0.00181481 | 0.000624159 | 12.1078 | 1 | 1.2368 | 0.806394 | 14.8504 | 6.20936 | A | F | 3.12e+20 | 2.39375e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X152246.48+273326.2 | chandra | ccd2 | 524.5 | 133.2 | 8.94837 | 3.1623 | 0.00176511 | 0.000623778 | 4.21428 | 0.999744 | 2.54927 | 1.65357 | 126.363 | 8.73473 | A | F | 3.17e+20 | 2.67424e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X152159.00+273806.4 | chandra | ccd0 | 777.375 | 939.875 | 7.32316 | 2.82844 | 0.00144541 | 0.000558265 | 9.64329 | 1 | 1.54814 | 0.520733 | 124.93 | 6.01871 | A | F | 3.06e+20 | 1.80317e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X152231.40+274149.7 | chandra | ccd3 | 714.5 | 173.5 | 7.1518 | 3.00004 | 0.00141159 | 0.000592133 | 2.30852 | 0.980683 | 0.492 | 0.492 | 67.5 | 2.09841 | F | F | 3.04e+20 | 1.64397e-14 | 1 | dx | ||||
| Report | 3 | X152243.56+273908.0 | chandra | ccd2 | 604 | 828 | 3.92737 | 2 | 0.000774693 | 0.00039451 | 1.84961 | 0.959343 | 0.492 | 0.492 | 45 | 4.6105 | F | F | 3.09e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X152216.90+273141.1 | chandra | ccd0 | 294.111 | 156.472 | 30.0469 | 6.00009 | 0.00593053 | 0.00118427 | 39.5664 | 1 | 4.51195 | 1.8047 | 159.863 | 9.02312 | A | F | 3.17e+20 | 9.3208e-14 | 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