We report a timing solution for the accreting Neutron Star GRO J1744-28, observed during its ongoing outburst (ATel #5790, #5810, #5845, #5858, #5883). We analyzed all the available Swift-XRT observations taken in Window Timing mode, from 2nd to 17th February 2014. These observations have an effective exposure time of ~13 ks. The intervals in which X-ray bursts are clearly detected (Atel #5883) were removed.
Detection of a spin derivative in GRO J1744-28 with Swift/XRT
PINTORE, FABIO;SANNA, ANDREA;BURDERI, LUCIANO;
2014-01-01
Abstract
We report a timing solution for the accreting Neutron Star GRO J1744-28, observed during its ongoing outburst (ATel #5790, #5810, #5845, #5858, #5883). We analyzed all the available Swift-XRT observations taken in Window Timing mode, from 2nd to 17th February 2014. These observations have an effective exposure time of ~13 ks. The intervals in which X-ray bursts are clearly detected (Atel #5883) were removed.
File in questo prodotto:
Non ci sono file associati a questo prodotto.
I metadati presenti in IRIS UNICA sono rilasciati con licenza Creative Commons CC0 1.0 Universal, mentre i file delle pubblicazioni sono protetti da diritto d'autore, salvo diversa indicazione.
