Modifying the Health Star Rating nutrient profiling algorithm to account for ultra‐processing

Modifying the Health Star Rating nutrient profiling algorithm to account for ultra‐processing

Aim: To modify the Australian and New Zealand Health Star Rating to account for ultra‐processing and compare the alignment of the modified ratings with NOVA classifications and the current Australian Dietary Guidelines classifications of core (recommended foods) and discretionary (foods to limit). M...

Bibliografske podrobnosti
Main Authors:	Barrett, EM, Pettigrew, S, Neal, B, Rayner, M, Coyle, DH, Jones, A, Maganja, D, Gaines, A, Mozaffarian, D, Taylor, F, Ghammachi, N, Wu, JHY
Format:	Journal article
Jezik:	English
Izdano:	Wiley 2024

Podobne knjige/članki

Consumer choice and the role of front-of-pack labelling: the Health Star Rating system
od: Damian Maganja, et al.
Izdano: (2019-03-01)

Neutron decay, dark matter and neutron stars
od: Beck D.H.
Izdano: (2019-01-01)

Meeting the Challenge: Accounting for Change
od: Pettigrew, A, et al.
Izdano: (1994)

No short hair behaviors of ultra-compact stars
od: Yan Peng
Izdano: (2021-03-01)

AN ELEMENTAL ASSAY OF VERY, EXTREMELY, AND ULTRA-METAL-POOR STARS
od: Hansen, T., et al.
Izdano: (2015)

DELVE 6: An Ancient, Ultra-faint Star Cluster on the Outskirts of the Magellanic Clouds
od: W. Cerny, et al.
Izdano: (2023-01-01)

Can Dark Stars Account for the Star Formation Efficiency Excess at Very High Redshifts?
od: Lei Lei, et al.
Izdano: (2025-01-01)

METAL-POOR STARS OBSERVED WITH THE MAGELLAN TELESCOPE. III. NEW EXTREMELY AND ULTRA METAL-POOR STARS FROM SDSS/SEGUE AND INSIGHTS ON THE FORMATION OF ULTRA METAL-POOR STARS
od: Placco, Vinicius M., et al.
Izdano: (2015)

ENVIRONMENTAL ACCOUNTING IN AGRICULTURE: NUTRIENT ACCOUNTING AND OTHER ASPECTS
od: P URFI, et al.
Izdano: (2003-04-01)

OBSERVATIONAL CONSTRAINTS ON FIRST-STAR NUCLEOSYNTHESIS. II. SPECTROSCOPY OF AN ULTRA METAL-POOR CEMP-no STAR
od: Placco, Vinicius M., et al.
Izdano: (2017)

Accounting for tourism benefits in marine reserve design.
od: Daniel F Viana, et al.
Izdano: (2017-01-01)

Enhancing the effectiveness of the Health Star Rating via presentation modifications
od: Simone Pettigrew, et al.
Izdano: (2020-02-01)

CONCEPTS BEHIND NUTRIENT PROFILING
od: Rayner, M
Izdano: (2009)

Upper bound on the radii of regular ultra-compact star photonspheres
od: Yan Peng
Izdano: (2019-03-01)

Socio-economic difference in purchases of ultra-processed foods in Australia: an analysis of a nationally representative household grocery purchasing panel
od: Daisy H. Coyle, et al.
Izdano: (2022-12-01)

Do healthier packaged foods cost more? A pilot study evaluating health stars and food prices
od: M.Y. de Abreu, et al.
Izdano: (2017-06-01)

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection
od: Rovilos, E, et al.
Izdano: (2012)

Nutrient supply from marine small-scale fisheries
od: Daniel F. Viana, et al.
Izdano: (2023-07-01)

The S-PLUS Ultra-short Survey: Photometric Recalibration with the Best Star Database
od: Xiaolu Li, et al.
Izdano: (2025-01-01)

Improving the performance of the Health Star Rating front-of-pack nutrition labelling system by incorporating added sugar
od: Peters, S, et al.
Izdano: (2017)

Accounting for the Nutrients in Reclaimed Water for Landscape Irrigation
od: Christopher J. Martinez, et al.
Izdano: (2011-08-01)

Accounting for the Nutrients in Reclaimed Water for Landscape Irrigation
od: Christopher J. Martinez, et al.
Izdano: (2011-08-01)

Accounting for the Nutrients in Reclaimed Water for Landscape Irrigation
od: Christopher J. Martinez, et al.
Izdano: (2011-08-01)

The Application of Management Accounting Techniques at Star Hotels in Denpasar City
od: Ni Made Adi Erawati, et al.
Izdano: (2018-10-01)

EXPLORING THE ORIGIN OF LITHIUM, CARBON, STRONTIUM, AND BARIUM WITH FOUR NEW ULTRA METAL-POOR STARS
od: Hansen, T., et al.
Izdano: (2015)

Evolution of star formation in the UKIDSS Ultra Deep Survey field - I. Luminosity functions and cosmic star formation rate out to z=1.6
od: Drake, AB, et al.
Izdano: (2013)

IS IT POSSIBLE TO DEVELOP A GLOBAL NUTRIENT PROFILE MODEL?
od: Rayner, M
Izdano: (2013)

Discovery of a radio-emitting neutron star with an ultra-long spin period of 76 s
od: Caleb, M, et al.
Izdano: (2022)

A Study on Reactive Ultra-Fine Fly Ash and Sulfoaluminate Cement in Self-Leveling Mortar
od: Pei-Min Chuang, et al.
Izdano: (2025-01-01)

Incorporating added sugar improves the performance of the Health Star Rating front-of-pack labelling system in Australia
od: Peters, SAE, et al.
Izdano: (2017)

Systematically Measuring Ultra-diffuse Galaxies (SMUDGes). VI. Nuclear Star Clusters
od: Mika Lambert, et al.
Izdano: (2024-01-01)

Unexpected Management Choices When Accounting for Uncertainty in Ecosystem Service Tradeoff Analyses
od: Reniel B. Cabral, et al.
Izdano: (2017-07-01)

Nutrient profiling and the regulation of marketing to children. Possibilities and pitfalls.
od: Rayner, M, et al.
Izdano: (2013)

Nutrient profiling and the regulation of marketing to children. Possibilities and pitfalls
od: Rayner, M, et al.
Izdano: (2013)

The star formation rate of the Universe at z approximate to 6 from the Hubble Ultra-Deep Field
od: Bunker, A, et al.
Izdano: (2004)

Skyrmions, Skyrme stars and black holes with Skyrme hair in five spacetime dimension
od: Yves Brihaye, et al.
Izdano: (2017-11-01)

When nutrient profiling can (and cannot) be useful.
od: Scarborough, P, et al.
Izdano: (2014)

AN ULTRA-FAST X-RAY DISK WIND IN THE NEUTRON STAR BINARY GX 340+0
od: Miller, J. M., et al.
Izdano: (2017)

The dynamics and kinematics of the coastal boundary layer off Long Island
od: Pettigrew, Neal Robert
Izdano: (2005)

Validating a nutrient profile model.
od: Arambepola, C, et al.
Izdano: (2008)