'Orion kl' presentation slideshows

HERSCHEL HIFI FIRST RESULTS

HERSCHEL HIFI FIRST RESULTS. Cecilia Ceccarelli. OUTLINE. INTRODUCTION TO HERSCHEL & HIFI HIFI FIRST RESULTS from HEXOS HIFI FIRST RESULTS from CHESS. HERSCHEL in a nutshell. A 3.5-mt passively cooled telescope Payload cooled at the Helium superfluid temperature

572 views • 56 slides

3mm spectral-line observing with Mopra

3mm spectral-line observing with Mopra. Tony Wong ATNF & UNSW. Mopra Induction Weekend - 28 May 2005. Outline. How bright is your source? Estimate expected brightness temperature What is the required integration time? Depends on T mb , T sys , bandwidth What are the required calibrations?

444 views • 30 slides

343 views • 20 slides

Prelude to MIRI Herschel: A WISH come true

Prelude to MIRI Herschel: A WISH come true. RCW120 Herschel A. Zavagno. The HIFI forest of lines in Orion. Bergin et al. 2010. Orion KL. Orion KL - Band 1. Wang et al. 2010. Low-mass protostars: NGC 1333. p-H 2 O ground-state Line: 1 THz. L~20 L Sun D~750 lyr. outflow.

292 views • 16 slides

Mopra Calibration @ 115GHz 2005-2009

Mopra Calibration @ 115GHz 2005-2009. The MAGMA Perspective Annie Hughes & Tony Wong. Why this talk?. Flux monitoring undertaken as part of the MAGMA survey may be valuable for: users who want to combine data from MPCOR and MOPS (2006 to present)

95 views • 9 slides