Details on Acronym: [BTS2017] | |
| [BTS2017] | (Bauer+Treister+Schawinski+, 2017) |
| Write: | <<[BTS2017] CDF-S XTN>> |
| N: | 2 |
| Object: | X-ray Transient (SIMBAD class: X = X-ray Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | Chandra ACIS-I observations of N=2 fast X-ray transients 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). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |