High resolution SZ observations at the IRAM 30


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PDF High resolution SZ observations at the

How to improve high resolution SZ observations ? The New IRAM KIDs Array (NIKA): ➡ Dual-band KID camera ➡ Developed in Grenoble (France) ➡ Observing at 

PDF A case study of the IRAM NOEMA large program CORE

Using the IRAM NOEMA and the IRAM 30 m telescope the CORE survey has obtained high-resolution observations of 20 well-known highly luminous star-forming regions in the 1 37 mm wavelength regime in both line and dust continuum emission

PDF Insights from the IRAM NOEMA large program CORE

We have observed 20 high-mass YSOs at the highest angu-lar resolution currently possible for 1 3 mm observations in the northern sky (0 400 800 au at 2 kpc) using the Northern Extended Millimetre Array (NOEMA) interferometer and the IRAM 30-m telescope (PI: Henrik Beuther) One of the objectives of this

  • High resolution SZ observations at the IRAM 30-m telescope with

    Its high surface accuracy (∼ 50μ m) allows observations down to a wavelength of 1mm (corresponding to 280 Ghz).
    At this wavelength, the angular resolution of the IRAM 30m telescope is 10''.

3 sept. 2014 · In this paper, we give the status of the NIKA camera, focussing on the KID technology. We then present observations of three galaxy clusters: RX  Autres questions
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