Details on Acronym: [DWV2017] | |
| [DWV2017] | (Dai+Wang+Vadakkumthani+, 2017)= ([DWV2017a]) |
| Write: | <<[DWV2017] JHHMM.m XN>> |
| N: | 24 |
| Object: | (X) (SIMBAD class: X = X-ray Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | N=26 X-ray sources in the field of ten 3FGL gamma-ray millisecond pulsars (MSPs). Use of archival X-ray observations from the Swift, Chandra, XMM-Newton, and Suzaku satellites. |
| Ref: | =2017RAA....17...72D |
| by | DAI X.-J. , WANG Z.-X., VADAKKUMTHANI J., XING Y. |
| RAA, 17, 72 (2017) | |
| Identification of candidate millisecond pulsars from Fermi LAT observations II. | |
| o | Table 4: <[DWV2017] JHHMM.m XN> N=24. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [DWV2017a] | |
| [DWV2017a] | (Dai+Wang+Vadakkumthani+, 2017) |
| ***** | Avoid the usage of [DWV2017a], prefer [DWV2017] |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |