Publication type: Non-refereed

  • Publication
    IPHAS Discovers Hundreds of New Planetary Nebulae at the Galactic Plane
    The Isaac Newton Telescope H-alpha survey (IPHAS) of the northern galactic plane is near completion. The photometric (H-alpha, R, I) catalogue and the mosaic...
  • Publication
    IPHAS symbiotic stars candidates (Corradi+, 2008)
    As the present study was progressing, we started a campaign of spectroscopic follow-up of the Hα emitters detected by IPHAS. Accordingly a dozen candidate...
  • Publication
    IPHAS: Surveying the North Galactic Plane in H-alpha
    H-alpha emission is ubiquitous in our Galaxy. It traces ionised gas of assorted nebulae such as HII regions, planetary nebulae, Wolf-Rayet nebulae, and...
  • Publication
    IPHAS: The INT/WFC Photometric H-alpha Survey of the Northern Galactic Plane
    H-alpha emission both traces diffuse ionised nebulae and is commonly prominent in the spectra of pre- and post-main-sequence stars and interacting binaries...
  • Publication
    IPHASX J052531.2+281946: a new Planetary Nebula towards the Galactic Anticentre
    A planetary nebula has been discovered in the course of the INT/WFC Photometric Hα Survey (IPHAS) of the northern galactic plane. It is located near the...
  • Publication
    IR And X-ray Tests Of The Clumpy Torus Models Of AGN
    On-going explorations of AGN based at mid-IR wavelengths has tightly constrained individual torus sizes to a few pc and found that spectral fitting in the N...
  • Publication
    IR images of N159 in the LMC.
    The authors obtained near infrared images in J, H, and K filters of the H II region N159 in the LMC with the IR Imager on the 1.5 m telescope of CTIO. Some 50...
  • Publication
    IR light curves of eclipsing dwarf novae
    We present JHK light curves of eclipsing dwarf novae (IP Peg and HT Cas) obtained with the 4.2m WHT telescope at La Palma and attempt experimental fits on the H...
  • Publication
    IR light curves of four new low-mass eclipsing binaries
    In the last decade a significant amount of observational effort has been made to determine the physical parameters of low mass stars (M 1 Msol). The most...