PPT-BSRT vs WS cross-calibration MD

Fill 5456 LAST MEETING INJECTION gt Use BSRT calibration factors used before the MD gt Compare it with WS emittances LAST MEETING INJECTION gt Use BSRT calibration factors used before the MD. LMC. . 02-OCT-2012. F.Roncarolo. on behalf of the . BSRT . team. W.Andreazza. , . E.Bravin. , . A.Boccardi. , J. -. J.Gras. , . A.Goldblatt. , . M.Hamani. , . T.Lefevre. , . R.Jones. , . A.Nosych. , . Sean R. Stratton. TA-All Meeting – June 2010. Motivation. We’re still trying to understand the relative energy scale differences between our FDs.. The UVLED was used to . cross-calibrate all three FD sites.. Craig Markwardt & Bev . LaMarr. GSFC. PI: Keith . Gendreau. , NASA GSFC . Science: . Understanding ultra-dense matter via soft X-ray timing spectroscopy of neutron stars . Platform: International Space Station . Remember to be alert: the data might answer questions you didn’t ask. Keith Jahoda. 29 March 2012. PCA Energy Calibration - status. Current (final) calibration is described in . Shaposhnikov. et al. “Advances in the RXTE PCA Calibration: Nearing the Statistical Limit” (in preparation). Aerosol Chemical Monitor Calibration Centre. Evaluation protocol. Evelyn . Freney. , Olivier . Favez. , . Valerie. Gros, Jean . Sciare. . Yunjiang. ZHANG, . Tanguy . AMODEO. Bologna. George J. Bendo. and the SPIRE-ICC. Basic Equations. Derivative of flux calibration curves (from empirical analysis):. Flux calibration curve (integral of above equation):. V. 0. is a zero-point voltage that is selected to match the background in dark sky. . USGS EROS. rmorfitt@usgs.gov. Work Performed by. SGT: Mike Choate, . Mark . Lubke, . Obaidul. . Haque. , . Ajit. . Sampath. , Jim . Storey. , . and . Esad. . Micijevic. SDSU: . Dennis . Helder. , and Ashish Shrestha . GSICS Executive Panel, Boulder, 15-16 May 2015 . Peng Zhang, Jun Gao. Satellite Introdution. GF-1 satellite mission. GF-1 satellite is the first CHEOS constellation satellite launched on April 26, 2013 . Landsat Cal/Val Team. Landsat Calibration Meeting, May 2018. Topics. TIRS. Noise. Stability. Vicarious calibration comparison. OLI. Noise. Stability. Relative Calibration. Comparison to Sentinel 2 MSIs. GOES-R Program Calibration and Validation Robert A. Iacovazzi, Jr .* (1) , Edward C. Grigsby (1), Steve Goodman (2), Changyong Cao (3), Jaime Daniels (3), and Kathleen McIntyre (1) NASA (1), IceCube Calibration Overview Kurt Woschnagg University of California, Berkeley MANTS 2009 Berlin, 25 September 2009 4800 identical sensors in ultraclean, stable ice n m g geometry timing charge ice properties: Alan E. E. Rogers - co-I MIT Haystack . Raul A. . Monsalve. - Postdoc Arizona State University. Judd D. Bowman - PI Arizona State University. H1 – low-1 10x10 ground plane. H2 – low-1 30x30 ground plane. results. Icíar. Montilla, . M. . Reyes, M. . Núñez. , J. Marco de la . R. osa, O. . Tubio. , M. . Puga. (. Instituto. de . Astrofísica. de Canarias). Ali . Basden. . (Durham University). GTCAO overview. Add 12 event classes for SVX detector. .  . Done. Generate calibration parameters for Q-vector and flattening run by run .  . on-going. Status of centrality calibration. The calibrations for run-343031-347349 are good to use..