| sients in the Chandra Deep Field South. | |
| in source: | NAME CDFS |
| Ref: | =2017MNRAS.467.4841B |
| by | BAUER F.E. , TREISTER E., SCHAWINSKI K., SCHULZE S., LUO B., ALEXANDER D.M., BRANDT W.N., COMASTRI A., FORSTER F., GILLI R., KANN D.A., MAEDA K., NOMOTO K., PAOLILLO M., RANALLI P., SCHNEIDER D.P., SHEMMER O., TANAKA M., TOLSTOV A., TOMINAGA N., TOZZI P., VIGNALI C., WANG J., XUE Y., YANG G. |
| Mon. Not. R. Astron. Soc., 467, 4841-4857 (2017) | |
| A new, faint population of X-ray transients. | |
| o | <[BTS2017] CDF-S XTN> (No. XT1). |
| Ref: | =2019Natur.568..198X |
| by | XUE Y.Q. , ZHENG X.C., LI Y., BRANDT W.N., ZHANG B., LUO B., ZHANG B.-B., BAUER F.E., SUN H., LEHMER B.D., WU X.-F., YANG G., KONG X., LI J.Y., SUN M.Y., WANG J.-X., VITO F. |
| Natur, 568, 198-201 (2019) | |
| A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger. | |
| o | <[BTS2017] CDF-S XTN> (No. XT2). |
====Sorry, no entry could be found==== | |