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 | X145445.88-373547.9 | chandra | ccd7 | 884.944 | 996.278 | 7.29953 | 3.00004 | 0.00209461 | 0.000860866 | 8.29793 | 1 | 1.75449 | 0.955235 | 11.0328 | 8.69254 | A | F | 6.17e+20 | 1.85883e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X145608.18-373852.8 | chandra | ccd3 | 222.643 | 855.786 | 6.37825 | 2.64577 | 0.00183025 | 0.000759207 | 11.6691 | 1 | 1.12841 | 1.10547 | 96.2644 | 7.89947 | F | F | 6.22e+20 | 2.23148e-14 | 1 | dx | ||||
| Report | 3 | X145540.25-374023.8 | chandra | ccd3 | 896.9 | 671.5 | 4.94636 | 2.23607 | 0.00141937 | 0.000641644 | 9.04941 | 0.999999 | 0.492 | 0.492 | 57.5084 | 3.89523 | F | F | 6.24e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X145559.06-373304.3 | chandra | ccd2 | 476.7 | 507.3 | 4.65342 | 2.23608 | 0.00133531 | 0.000641646 | 8.86012 | 0.999989 | 1.34179 | 0.492 | 37.081 | 7.19348 | A | F | 6.16e+20 | 1.64982e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X145448.17-374328.3 | chandra | ccd7 | 828 | 60.6667 | 4.64623 | 2.44953 | 0.00133325 | 0.000702897 | 5.28173 | 0.999846 | 1.62961 | 1.25417 | 32.1651 | 10.281 | F | F | 6.26e+20 | 1.18082e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X145518.87-373619.6 | chandra | ccd7 | 88 | 932.75 | 3.89227 | 2 | 0.00111689 | 0.000573904 | 4.42464 | 0.998779 | 0.492 | 0.492 | 75.1276 | 2.21639 | F | F | 6.2e+20 | 9.42195e-15 | 1 | dx | ||||
| Report | 2 | X145600.11-373212.4 | chandra | ccd2 | 451.25 | 612.75 | 3.89184 | 2 | 0.00111677 | 0.000573904 | 7.41008 | 0.999989 | 0.996337 | 0.492 | 144.4 | 7.87951 | A | F | 6.15e+20 | 0 | 1 | d | |||||
| Report | 3 | X145548.96-373014.0 | chandra | ccd2 | 720.5 | 853.75 | 3.92067 | 2 | 0.00112504 | 0.000573904 | 7.46497 | 0.999989 | 0.492 | 0.492 | 25.4531 | 7.96414 | F | F | 6.13e+20 | 0 | 1 | d | |||||
| Report | 4 | X145516.82-374158.6 | chandra | ccd7 | 137.25 | 243.75 | 3.86094 | 2 | 0.0011079 | 0.000573905 | 4.38902 | 0.998779 | 0.704643 | 0.492 | 23.3679 | 5.39732 | F | F | 6.26e+20 | 0 | 1 | d | |||||
| Report | 4 | X145552.03-373432.7 | chandra | ccd2 | 646.833 | 327.833 | 2.97642 | 1.73205 | 0.000854088 | 0.000497015 | 5.6671 | 0.999806 | 0.492 | 0.492 | 90 | 5.22539 | F | F | 6.17e+20 | 0 | 1 | d | |||||
| Report | 5 | X145546.55-373019.7 | chandra | ccd2 | 778.833 | 842.167 | 2.89364 | 1.73205 | 0.000830334 | 0.000497016 | 5.50949 | 0.999806 | 0.492 | 0.492 | 109.903 | 7.65519 | F | F | 6.13e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X145558.02-372944.5 | chandra | ccd2 | 501.5 | 913.5 | 1.97938 | 1.41421 | 0.000567986 | 0.000405811 | 3.76874 | 0.997151 | 0.492 | 0.492 | 90 | 9.36755 | F | F | 6.12e+20 | 8.15093e-15 | 1 | dx | ||||
| Report | 7 | X145552.56-373139.0 | chandra | ccd2 | 633.833 | 680.833 | 2.94292 | 1.73205 | 0.000844476 | 0.000497016 | 5.60333 | 0.999806 | 0.492 | 0.492 | 45 | 7.20009 | F | F | 6.14e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X145547.81-374056.9 | chandra | ccd3 | 714.5 | 604 | 1.95977 | 1.41422 | 0.000562358 | 0.000405812 | 3.58541 | 0.996442 | 0.5535 | 0.492 | 90 | 5.27403 | F | F | 6.24e+20 | 6.73435e-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