Results 111 to 120 of about 200,534 (264)
We report the discovery of two new Galactic accreting compact objects consistent with the respective positions of the unassociated Fermi-LAT γ -ray sources 4FGL J0639.1-8009 and 4FGL J1824.2+1231. A combination of new and archival X-ray data from Chandra,
Rebecca Kyer +6 more
doaj +1 more source
An Improved One millisecond Mobile Backbone
Pavan Kumar Anasosalu Vasu +4 more
semanticscholar +1 more source
Millisecond-cadence Radio Frequency Interference Filters
Radio frequency interference (RFI) greatly reduces the sensitivity of radio observations to astrophysical signals and creates false-positive candidates in searches for radio transients.
Joseph W. Kania +3 more
doaj +1 more source
A Numerical Study of Sub-Millisecond Integrated Mix-and-Inject Microfluidic Devices for Sample Delivery at Synchrotron and XFELs [PDF]
Majid Hejazian +2 more
openalex +1 more source
Unveiling Low-frequency Eclipses in Spider Millisecond Pulsars Using Wideband GMRT Observations
Eclipses of radio emission have been reported for ∼58 spider millisecond pulsars (MSPs), of which only around 19% have been extensively studied. Such studies at low frequencies are crucial for probing the properties of the eclipse medium.
Sangita Kumari +5 more
doaj +1 more source
Observations of Nine Millisecond Pulsars at 8600 MHz Using the TMRT
We report detection results of nine millisecond pulsars (MSPs) at 8600 MHz using simultaneous 2250 and 8600 MHz observations conducted with the Shanghai Tian Ma Radio Telescope.
Xiao-Wei Wang +9 more
doaj +1 more source
Power-law Magnetic Field Decay and Constant Core Temperatures of Magnetars, Normal and Millisecond Pulsars [PDF]
Yi Xie, Shuang‐Nan Zhang
openalex +1 more source
The Spectrum of the Millisecond Pulsar J0218+4232 - Theoretical Interpretations [PDF]
J. Dyks, B. Rudak
openalex +1 more source
Sub-Millisecond Photoinduced Dynamics of Free and EL222-Bound FMN by Stimulated Raman and Visible Absorption Spectroscopies [PDF]
Yingliang Liu +9 more
openalex +1 more source

