We report on X-ray observations of the solitary 4.8 ms pulsar PSR J0030+0451. The pulsar was one of the last targets observed in DEC-98 by the ROSAT PSPC. X-ray pulses are detected on a $4.5\sigma$ level and make the source the $11^{th}$ millisecond pulsar detected in the X-ray domain. The pulsed fraction is found to be $69\pm18%$. The X-ray pulse profile is characterized by two narrow peaks which match the gross pulse profile observed at 1.4 GHz. Assuming a Crab-like spectrum the X-ray flux is in the range $f_x= 2-3\times 10^{-13}$ erg s$^{-1}$ cm$^{-2} $ ($0.1-2.4$ keV), implying an X-ray efficiency of $L_x/\dot{E}\sim 0.5-5 \times 10^{-3} (d/0.23 {kpc})^2$
We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154–6250 obtained...
X-ray emission from many rotation-powered millisecond pulsars (MSPs) is observed to be of predominan...
PSR J1119-6127 is a recently discovered 1600-yr-old radio pulsar that has a very high inferred surfa...
Millisecond pulsars represent an evolutionarily distinct group among rotation-powered pulsars. Outsi...
We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154-6250 obtained...
We present XMM-Newton observations of the radio pulsar PSR J1119-6127, which has an inferred age of ...
Introduction The 5.75 ms pulsar J0437--4715 is of special interest due to its prominent manifestati...
This grant, titled 'X-Ray Emission from Two Nearby Millisecond Pulsars,' included ROSAT observations...
We report the results of new XMM-Newton observations of the middle-aged (τc = 1.1 × 105 yr) radio pu...
We report on XMM-Newton observations of the "Black Widow pulsar", PSR B1957+20. The pulsar's X-ray e...
PSR J1119-6127 is a recently discovered 1700-year-old radio pulsar that has a very high inferred sur...
The existence of radio pulsars having inferred magnetic elds in the magnetar regime suggests that po...
Abstract. We report the detection of pulsed X-ray emission from the binary millisecond pulsar PSR J0...
I present an analysis of the XMM-Newton observations of four millisecond pulsars, J04374715, J212433...
The radio-quiet pulsar PSR J2021+4026 is mostly known because it is the only rotation-powered pulsar...
We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154–6250 obtained...
X-ray emission from many rotation-powered millisecond pulsars (MSPs) is observed to be of predominan...
PSR J1119-6127 is a recently discovered 1600-yr-old radio pulsar that has a very high inferred surfa...
Millisecond pulsars represent an evolutionarily distinct group among rotation-powered pulsars. Outsi...
We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154-6250 obtained...
We present XMM-Newton observations of the radio pulsar PSR J1119-6127, which has an inferred age of ...
Introduction The 5.75 ms pulsar J0437--4715 is of special interest due to its prominent manifestati...
This grant, titled 'X-Ray Emission from Two Nearby Millisecond Pulsars,' included ROSAT observations...
We report the results of new XMM-Newton observations of the middle-aged (τc = 1.1 × 105 yr) radio pu...
We report on XMM-Newton observations of the "Black Widow pulsar", PSR B1957+20. The pulsar's X-ray e...
PSR J1119-6127 is a recently discovered 1700-year-old radio pulsar that has a very high inferred sur...
The existence of radio pulsars having inferred magnetic elds in the magnetar regime suggests that po...
Abstract. We report the detection of pulsed X-ray emission from the binary millisecond pulsar PSR J0...
I present an analysis of the XMM-Newton observations of four millisecond pulsars, J04374715, J212433...
The radio-quiet pulsar PSR J2021+4026 is mostly known because it is the only rotation-powered pulsar...
We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154–6250 obtained...
X-ray emission from many rotation-powered millisecond pulsars (MSPs) is observed to be of predominan...
PSR J1119-6127 is a recently discovered 1600-yr-old radio pulsar that has a very high inferred surfa...