Pulsars steadily dissipate their rotational energy via relativistic winds. Confinement of these
outflows generates luminous pulsar wind nebulae, seen across the electromagnetic …

We present the results of the most comprehensive survey of the Galactic plane in very high-
energy (VHE) γ-rays, including a public release of Galactic sky maps, a catalog of VHE …

The Giant Metrewave Radio Telescope (GMRT) is today a frontline international facility for
low-frequency radio astronomy, that has produced several exciting and important new …

We present the results of the most comprehensive survey of the Galactic plane in very high-
energy (VHE) gamma-rays, including a public release of Galactic sky maps, a catalog of …

This catalog summarizes 117 high-confidence⩾ 0. 1 GeV gamma-ray pulsar detections
using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite …

Context. For many years, X-ray astronomy missions have used the Crab nebula as a
celestial calibration source for the X-ray flux and spectral shape. However, the object is often …

We have discovered the pulsar associated with the supernova remnant G21. 5-0.9. PSR
J1833-1034, with spin period P= 61.8 ms and dispersion measure 169 cm-3 pc, is very faint …

The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274
known Galactic supernova remnants. Of these, 16 were detected in at least two Planck …

We present molecular spectroscopy toward 50 Galactic supernova remnants (SNRs) taken
at millimeter wavelengths in 12 CO J= 2− 1. These observations are part of a systematic …

We present the results from timing observations with the Giant Metrewave Radio Telescope
of the young pulsar J1833− 1034 in the Galactic supernova remnant G21. 5− 0.9. We detect …