Observations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysis
Monthly Notices of the Royal Astronomical Society 289:2 (1997) 471-481
Abstract:
We present source counts at 6.7 and 15 μm from our maps of the Hubble Deep Field (HDF) region, reaching 38.6 μJy at 6.7 μm and 255 μJy at 15 μm. These are the first ever extragalactic number counts to be presented at 6.7 μm, and are three decades fainter than IRAS at 12 μm. Both source counts and a P(D) analysis suggest that we have reached the Infrared Space Obsen'atory (ISO) confusion limit at 15 μm: this will have important implications for future space missions. These data provide an excellent reference point for other ongoing ISO surveys. A no-evolution model at 15 μm is ruled out at > 3σ, while two models which fit the steep IRAS 60-μm counts are acceptable. This provides important confirmation of the strong evolution seen in IRAS surveys. One of these models can then be ruled out from the 6.7-μm data. © 1997 RAS.Radio observations of the black hole candidate GX 339−4
AIP Conference Proceedings AIP Publishing 410:1 (1997) 937-941
ASOCAM Observations of CYG X-3: Search for a Hot Stellar Wind
Astrophysics and Space Science Springer Nature 255:1-2 (1997) 205-210
Modelling of infrared emission from Cyg X-3 and the UKIRT IRCAM3 point spread function
Vistas in Astronomy Elsevier 41:1 (1997) 65-70
The decay phase of radio flares from GRS1915+105
Vistas in Astronomy Elsevier 41:1 (1997) 21-26