About Lfi player
Forum Photon Emitters Programming and other assorted Bit-level Alchemy Lfi player Thread: Lfi player 04-28-2013, 22:19 #11 Join Date Feb 2013 Posts 3 I know it's a post from 2009 but hey, I just want to just a thumbs up.Great software. Thanks for sharing it! 08-18-2013, 09:54 #12 Join Date Jul 2012 Location BRAZIL Posts 34 08-18-2013, 09:55 #13 Join Date Jul 2012 Location BRAZIL Posts 34 08-26-2013, 05:55 #14 Join Date Oct 2008 Posts 29 De Nada :-)I'm so glad people still find LFI Player useful after all these years. 08-28-2013, 16:56 #15 Join Date Feb 2008 Location UK and US Posts 98 Hi Michael Give me a call, we'll have to catch up.Clive. Posting Permissions You may not post new threads You may not post replies You may not post attachments You may not edit your posts BB code is On Smilies are On [IMG] code is On [VIDEO] code is On HTML code is Off Forum Rules All times are GMT -8. The time now is 22:57. Powered by vBulletin Version 4.2.5 Copyright © 2025 vBulletin Solutions Inc. All rights reserved.
Key features of the Lfi player that are enabled through these drivers include:
- LFI Player DAC problem - Page 3 - photonlexicon.com
- LFI Player DAC problem - Page 4 - photonlexicon.com
- LFI Player DAC problem - Page 2 - photonlexicon.com
- Laserpointer galvo Riya LFI player test - YouTube
- LFI Player DAC problem - Page 5 - photonlexicon.com
- LFI Player Software Rides Again - Page 2
- Download LFI_Player_V1.2.3.zip (LFI Player 3D Laser
– LiteBIRD Kick Off Meeting - JAXS 1 July 2019 21 A joint map from LFI and WMAPPreliminary LFI+WMAP The WMAP low-ell polarization likelihood can be analyzed using a map-based formalism similar for LFI. Good consistency already at the level of angular power spectrum This enables use of a joint (weighted-average by pixel) dataset U. Natale et al. in prep. Paolo Natoli – LFI Systematics and Impact on Science – LiteBIRD Kick Off Meeting - JAXS 1 July 2019 22 The LFI+WMAP dataset Good consistency across different Galactic masksPreliminary Good consistency across different Galactic masks Dt scatter by mask compared to simulations U. Natale et al. in prep. Paolo Natoli – LFI Systematics and Impact on Science – LiteBIRD Kick Off Meeting - JAXS 1 July 2019 23 t from LFI and WMAP from LFI+WMAP PreliminaryNull test is map-based, estimate has ~20% error on t (from low ell only) Includes TE (and, potentially, BB, TB, EB...) But from a pixel-based likelihood. Can be used to constrain models for which an EE spectrum-based likelihood (as HFI) in unsuited, e.g. non-isotropic cosmologies (CMB anomalies) Cosmological birefringence Paolo Natoli – LFI Systematics and Impact on Science – LiteBIRD Kick Off Meeting - JAXS 1 July 2019 24 Joint view of existing constraints on tL. Pagano Paolo Natoli – LFI Systematics and Impact on Science – LiteBIRD Kick Off Meeting - JAXS 1 July 2019 25 Conclusions and lessons learnedIn low ell polarization, LFI has provided constraints based on 70 GHz, used as baseline in 2015 and as consistency in 2018. Low ell polarization is an hard measurement. The Planck experience shows that systematic errors can arise at the level of data processing, in the interplay between calibration, map-making and component separation Validation through end-to-end simulations is an extremely important step Solving problems requires time. LFI could benefit from a well integrated team, thanks to strong links between Science Ground Segment and Science exploitation teams. Post-legacy analysis is delivering a joint pixel based dataset for LFI and WMAP, competitive in terms of noise and suitable for many non-standard analyses. Paolo Natoli – LFI Systematics
