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 | 5 | X044603.28+312241.5 | chandra | ccd7 | 736.812 | 303.621 | 202.268 | 14.528 | 0.0201498 | 0.00144727 | 96.4632 | 1 | 0.512305 | 0.406705 | 292.379 | 0.667524 | F | F | 2.77e+21 | 1.88194e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X044558.13+312427.2 | chandra | ccd7 | 870.699 | 518.391 | 165.421 | 12.8616 | 0.0164792 | 0.00128127 | 78.8906 | 1 | 0.699485 | 0.484501 | 342.147 | 2.56484 | F | F | 2.78e+21 | 1.4113e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X044558.21+311340.8 | chandra | ccd6 | 669.5 | 213.208 | 39.5793 | 7.14153 | 0.00394408 | 0.000711655 | 42.888 | 1 | 2.0295 | 1.5924 | 146.725 | 9.0724 | F | F | 2.73e+21 | 4.97448e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X044628.71+312813.9 | chandra | ccd7 | 74.7778 | 978.944 | 15.4712 | 4.24268 | 0.00154123 | 0.000422653 | 7.37833 | 1 | 1.53832 | 0.857576 | 106.98 | 7.39121 | A | F | 2.8e+21 | 1.54045e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X044607.11+312341.1 | chandra | ccd7 | 636.625 | 424.25 | 7.6318 | 2.82843 | 0.000760275 | 0.000281767 | 3.63967 | 0.999346 | 0.492 | 0.492 | 18.2644 | 1.11226 | F | F | 2.78e+21 | 6.44483e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X044603.62+312815.9 | chandra | ccd7 | 727.167 | 982.833 | 5.48412 | 2.4495 | 0.000546324 | 0.000244018 | 2.61542 | 0.985178 | 0.738884 | 0.492 | 113.274 | 5.71113 | A | F | 2.8e+21 | 4.93607e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X044548.67+311943.5 | chandra | ccd6 | 917.833 | 950.5 | 2.94042 | 1.73205 | 0.000293014 | 0.000172599 | 3.18624 | 0.988796 | 0.492 | 0.492 | 180 | 4.73773 | F | F | 2.76e+21 | 3.40001e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X044613.85+312027.9 | chandra | ccd6 | 261.9 | 1040.5 | 4.92265 | 2.23607 | 0.000490543 | 0.000222825 | 5.33418 | 0.999743 | 0.492 | 0.492 | 2.35031e-08 | 2.65566 | F | F | 2.76e+21 | 9.04739e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X044613.11+311936.9 | chandra | ccd6 | 281.167 | 936.833 | 5.77717 | 2.4495 | 0.000575696 | 0.000244093 | 6.26014 | 0.999969 | 0.763435 | 0.492 | 82.5343 | 3.30127 | A | F | 2.76e+21 | 6.39447e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X044551.07+312046.5 | chandra | ccd6 | 855.167 | 1078.5 | 8.68972 | 3.00001 | 0.000865932 | 0.000298951 | 9.41617 | 1 | 0.539465 | 0.492 | 148.283 | 3.73219 | F | F | 2.76e+21 | 9.72956e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X044615.74+311721.6 | chandra | ccd6 | 212.75 | 662 | 3.85354 | 2 | 0.000384006 | 0.000199301 | 4.17569 | 0.99815 | 0.501152 | 0.492 | 133.569 | 5.59422 | F | F | 2.75e+21 | 4.53474e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X044557.17+311543.9 | chandra | ccd6 | 696.5 | 463.3 | 4.32394 | 2.23609 | 0.000430881 | 0.000222826 | 4.68541 | 0.999743 | 1.02627 | 0.492 | 156.97 | 7.1286 | A | F | 2.74e+21 | 5.56644e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X044555.38+311930.3 | chandra | ccd6 | 743.58 | 924.084 | 30.6513 | 5.53636 | 0.00305443 | 0.000551703 | 33.2137 | 1 | 1.12172 | 1.12172 | 0 | 3.87046 | F | F | 2.76e+21 | 3.41821e-14 | 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