Overview Science Goals ApJ Intro paper Appendix Team and contacts Publications and Presentations Papers Talks Posters Rapid Release Chandra Survey Selection Criteria Fields Observed NOAO Survey Fields Observed Data Archive X-ray Database Optical Database DS9 Virtual Observatory Quantile Analysis Chandra pointings for ChaMPane Bulge Windows Survey Bulge Latitude Survey Internal Related Links The ChaMPlane survey is being conducted at the Harvard-Smithsonian Center for Astrophysics.

Photometric Depth Achieved DEPTH = Photometric depth for 5 sigma detection, determined from measured sky, variance, seeing and magnitude zeropoint. EXPTIME = Total exposure time (seconds ) for the stacked Mosaic image. SEEING = FWHM in arcseconds FIELD FILTER DEPTH EXPTIME SEEING ------- ------ -------- ------- -------- A0620 V 23.40 600 0.940 R 24.00 1140 0.863 I 23.17 840 0.850 Ha 23.38 6600 0.788 B2224 V 22.35 180 1.544 R 24.88 2100 0.911 I 21.50 900 1.307 Ha 23.95 9000 0.963 C123 V 24.39 540 1.096 R 25.31 1200 0.799 I 22.95 540 1.323 Ha 24.22 6900 0.968 C129 V 24.51 540 1.091 R 24.04 1200 1.119 I 23.76 540 0.828 Ha 24.00 6900 0.947 EGJ2227 V 23.04 540 1.484 R 23.85 1200 1.163 I 22.48 540 1.294 Ha 23.30 6900 1.203 G166 V 24.51 540 1.075 R 24.64 1200 1.143 I 23.18 540 0.961 Ha 24.32 7500 1.057 GKPer V 23.48 900 1.372 R 23.15 1260 1.190 I 22.75 540 1.148 Ha 22.77 7200 1.374 J0422 V 24.51 900 1.221 R 24.90 2100 0.994 I 22.99 1410 1.117 Ha 24.23 7500 0.981 NGC1569 V 23.56 900 1.174 R 23.93 1260 1.156 I 22.40 900 1.547 Ha 22.67 4800 1.390 NGC3256 V 23.98 480 0.956 R 24.38 1140 0.895 I 23.50 720 0.855 Ha 23.76 7200 0.876 NGC3603 V 24.70 540 1.096 R 24.18 1200 1.482 I 23.61 540 1.126 Ha 23.39 7500 1.286 PKS0745 V 24.39 480 0.766 R 24.59 1020 0.750 I 23.45 720 0.898 Ha 24.21 6900 0.788 V382Vel V 24.00 1080 0.855 R 23.53 1200 1.798 I 22.65 540 0.818 Ha 22.15 1288 1.948 G116 R 24.99 540 0.901