- Second run of NIKA at the 30m telescope
- Reflection on new cabin optics to increase the field of view of the Pico Veleta 30m telescope
- Specifications for a wide field of view fully sampled array of bolometers at the IRAM 30m telescope.
- Visits to SCUBA 2 and GISMO teams, and topics of interest from the LTD 12 conference.
- 0.475 ii 1+( )2 = Ep = Eeff in
- Remark: MAMBO pixels sample full beams (not Nyquist !), so 1.2x bigger than HPBW
- Summary of the documents replying the reports from the GISMO team about the October 2008 run at Pico Veleta
- 12/05/2010 SAC meeting IRAM Grenoble 1 Testing of current
- GISMO: A 2-Millimeter Bolometer Camera for the IRAM 30 m Telescope
- Instrument Performance of GISMO, a 2 Millimeter TES Bolometer Camera used at the IRAM 30 m Telescope
- NICA Optical testing summary This memo provides a summary of the optical testing carried out at Cardiff on the
- Astronomy & Astrophysics manuscript no. NIKAv6 c ESO 2010 June 21, 2010
- Optical software investigation S.Leclercq. 02/11/06.
- 28/04/2009 SAC meeting IRAM Grenoble 1 Bolometers at the 30m
- 30-meter cabin refurbishment for a large Field Of View
- Pros and cons of 3 solutions proposed for the rotation axes of a motorized tertiary mirror at the IRAM 30m telescope.
- NCS GISMO Features Identifer -Master URL: not published on WWW
- FXDesert NIKA@IRAM16 Dec 20091 NIKA Oct 2009 Run: Calibration & Sensitivity
- LEKID Optimisation Phase noise of current LEKID design approaching
- Preliminary Report on GISMO Run #2 October 27, 2008
- Remark: I use a prefix letter in front of NET and NEFD to stress the existence of these different definitions, and to stress that authors in litterature are not always clear about the one they use !
- What we need to return at the telescope New array at 1mm with better sensitvity
- Antenna coupled Kinetic Inductance Detectors camera design and performance at IRAM 30m telescope
- Prerun Summary: 30 Pixel LEKIDs Array for the IRAM 30 m Telescope
- GISMO sensitivity at Pico Veleta Feedback on Dominic Benford "Atmospheric Emission at Pico Veleta"
- 10/05/2011 SAC meeting IRAM Grenoble 1 Recent Results with NIKA &
- Activit bolomtres pour le 30m Pico Veleta
- Proposition of a new cabin optics increasing the field of view of the Pico Veleta 30m telescope
- Comments about GISMO Run #2 at Pico Veleta Feedback on Johannes Staguhn et al. "Report on GISMO Run #2"
- IRAM 300, rue de la piscine, Domaine Universitaire, 38406 Saint Martin d'Hres, France Tel : +33 (0)4 76 82 49 00 Fax : +33 (0)4 76 51 59 38
- Bands at the 30m MRT, sizes of pixels and arrays for various FOVs, Power load, NEP, NET, and NEFD from the background S.Leclercq -Nov 2009, update Mar 2010
- Discussion about Noise Equivalent Power and its use for photon noise calculation.
- The analysis performed using mostly only 2mm, as a large part of the 1mm data we got is incorrect !
- Estimation of the NIKA v2 optics grid distortion from empirical fits on a Zemax simulation
- The dual-band NIKA: Technical Note on Calibration v2
