275.23763 -14.33405:



USNO B1.0 with Gator:
No sources were found within 5".

USNO B1.0 with "Integrated Image and Catalog Archive Service":
again, just for the visual, not much info here:


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USNO A2.0 with same archive as above:



With DSS (just visual, no information)



2Mass with Gator:
2 sources were found within 5":
The closest was at a distance of 1.079200
RA: 275.237796, DEC: -14.334303, err_maj: 0.08, err_min: 0.08, err-ang: 90, j_mag:16.008, j_msigcom:0.096, j_snr:8.8, h_m: 14.235, h_msigcom:0.075, h_snr: 8.4, k_mag: 12.635, k_msigcom: null, k_snr:null, FLAGS: ph_qual: BBU, rd_flg:220, bl_flg: 110, cc_flg:0c0, j-h=1.7730, h-k=--, j-k=--

The farther was a distance of 3.970672
RA: 275.237272, DEC: -14.333003, err_maj: 0.07, err_min: 0.06, err-ang: 4, j_mag:15.931, j_msigcom:0.094, j_snr:9.4, h_m: 13.073, h_msigcom:0.064, h_snr: 24.5, k_mag: 11.663, k_msigcom: 0.043, k_snr:71.8, FLAGS: ph_qual: BAA, rd_flg: 222, bl_flg: 111, cc_flg:ccc, j-h=2.8580, h-k=1.4100, j-k=4.2680

There seems consistently to be no source matching the chandra source in the optical surveys for this source (unfortunately, that would be convenient). I'm not sure what to make of the infrared sources, if they are in fact supportive of the pulsar being located here, even if not visible in the optical..?