ORCID Profile
0000-0001-5032-7704
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Publisher: EDP Sciences
Date: 02-2012
Publisher: American Astronomical Society
Date: 13-02-2014
Publisher: American Physical Society (APS)
Date: 30-12-2014
Publisher: EDP Sciences
Date: 02-2014
Publisher: IOP Publishing
Date: 27-01-2021
Publisher: Elsevier BV
Date: 03-2011
Publisher: American Physical Society (APS)
Date: 22-01-2013
Publisher: American Astronomical Society
Date: 24-04-2012
Publisher: EDP Sciences
Date: 04-2013
Publisher: EDP Sciences
Date: 19-11-2012
Publisher: EDP Sciences
Date: 02-2014
Publisher: EDP Sciences
Date: 09-2010
Publisher: EDP Sciences
Date: 06-2010
Publisher: American Astronomical Society
Date: 22-09-2014
Publisher: EDP Sciences
Date: 03-2012
Publisher: EDP Sciences
Date: 02-2014
Publisher: Oxford University Press (OUP)
Date: 02-05-2014
DOI: 10.1093/MNRAS/STU459
Publisher: EDP Sciences
Date: 30-11-2010
Publisher: Oxford University Press (OUP)
Date: 11-02-2014
DOI: 10.1093/MNRAS/STU139
Publisher: WORLD SCIENTIFIC
Date: 26-02-2018
DOI: 10.1142/10986
Publisher: EDP Sciences
Date: 16-06-2011
Publisher: EDP Sciences
Date: 09-2012
Publisher: EDP Sciences
Date: 18-04-2012
Publisher: Oxford University Press (OUP)
Date: 08-2013
Publisher: EDP Sciences
Date: 13-02-2013
Publisher: Oxford University Press (OUP)
Date: 03-06-2014
DOI: 10.1093/MNRAS/STU826
Publisher: EDP Sciences
Date: 17-03-2011
Publisher: EDP Sciences
Date: 11-2014
Publisher: EDP Sciences
Date: 06-2013
Publisher: EDP Sciences
Date: 23-04-2014
Publisher: EDP Sciences
Date: 30-01-2015
Publisher: EDP Sciences
Date: 06-2013
Publisher: EDP Sciences
Date: 15-01-2013
Publisher: Oxford University Press (OUP)
Date: 18-11-2014
Publisher: American Physical Society (APS)
Date: 24-02-2015
Publisher: EDP Sciences
Date: 06-2012
Publisher: EDP Sciences
Date: 07-2011
Publisher: EDP Sciences
Date: 27-07-2015
Publisher: Oxford University Press (OUP)
Date: 12-06-2012
Publisher: EDP Sciences
Date: 27-02-2015
Publisher: EDP Sciences
Date: 16-11-2012
Publisher: American Astronomical Society
Date: 13-09-2012
Publisher: EDP Sciences
Date: 28-03-2014
Publisher: EDP Sciences
Date: 2012
Publisher: American Astronomical Society
Date: 09-05-2017
Publisher: IOP Publishing
Date: 23-02-2021
Publisher: EDP Sciences
Date: 09-2011
Publisher: American Astronomical Society
Date: 08-06-2011
Publisher: Elsevier BV
Date: 04-2011
Publisher: American Physical Society (APS)
Date: 20-11-2013
Publisher: EDP Sciences
Date: 29-08-2012
Publisher: EDP Sciences
Date: 10-12-2014
Publisher: SAGE Publications
Date: 11-2015
DOI: 10.4278/AJHP.140206-QUAN-62
Abstract: To examine associations of intervention dose with weight, physical activity, glycemic control, and diet outcomes in a randomized trial of a telephone counseling intervention. Study design was a secondary analysis of intervention group. Study setting was primary care practices in a disadvantaged community in Australia. Participants were adult patients with type 2 diabetes (n = 151). Up to 27 telephone counseling calls were made during 18 months. Intervention dose was assessed as the number of calls completed (in tertile categories). Primary outcomes were weight and HbA1c, and moderate to vigorous intensity physical activity via accelerometer. Secondary outcomes were dietary energy intake and diet quality via a validated questionnaire. Analyses employed were bivariate associations of call completion with sociodemographics, and confounder-adjusted linear mixed models for associations of call completion with outcomes (multiple imputation of missing data). Only previous diagnosis of depression/anxiety had a statistically significant (p= .008) association with call completion. Call completion was significantly associated with weight loss (p .001) but not the other outcomes (p .05). Relative to low call completion, mean weight loss (as a percentage of baseline weight) was greater in the high–call completion group by −3.3% (95% confidence interval, −5.0% to −1.5%). Increased dose of intervention was associated with greater weight loss. More needs to be done to retain patients for the duration of weight loss and behavior change interventions, particularly those with diabetes and comorbid depression, who were the most difficult to engage.
Publisher: EDP Sciences
Date: 03-2013
Publisher: American Association for the Advancement of Science (AAAS)
Date: 23-01-2015
Abstract: There's a new lab for studying the origins of cosmic rays: our neighbor galaxy, the Large Magellanic Cloud. Astronomers are now making progress on this topic by examining the gamma rays that are produced when cosmic rays interact with gas or lower-energy photons. The H.E.S.S. Collaboration has detected three sources of gamma rays in a variety of forms in the galactic satellite to the Milky Way. The sources include the pulsar wind nebula of N 157B, the supernova remnant N 132D, and the superbubble 30 Dor C. Oddly, supernova 1987A was not detected. Science , this issue p. 406
Publisher: American Physical Society (APS)
Date: 18-04-2011
Publisher: American Astronomical Society
Date: 24-03-2015
Publisher: American Physical Society (APS)
Date: 29-12-2014
Publisher: EDP Sciences
Date: 11-2013
Publisher: EDP Sciences
Date: 30-03-2011
No related grants have been discovered for Hannes Zechlin.