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1. Translation, Cultural Adaptation, and Validation of the Cantonese Version of SarQoL in Hong Kong’s Older Population: An Interviewer-Administered Questionnaire for Assessing Sarcopenia-Specific Quality of Life in Fieldwork Practice

Author

Yu R, Lai D, Leung G, Tam LY, Cheng C, Kong S, Tong C, Lu Z, Leung JC, Chan A, Kwok T, and Woo J

Subjects
interviewer-administered, psychometric, quality of life, sarcopenia, sarqol, translation, validation, Geriatrics, RC952-954.6
Abstract

Ruby Yu,1,2 Derek Lai,2 Grace Leung,2 Lok-Yan Tam,2 Clara Cheng,2 Sara Kong,2 Cecilia Tong,2 Zhihui Lu,1 Jason CS Leung,3 Amany Chan,3 Timothy Kwok,1,3 Jean Woo1,2 1Department of Medicine and Therapeutics, Faculty of Medicine, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong; 2The Jockey Club Institute of Ageing, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong; 3The Jockey Club Centre for Osteoporosis Care and Control, The Chinese University of Hong Kong, Shatin, New Territories, Hong KongCorrespondence: Ruby Yu, Department of Medicine & Therapeutics, Faculty of Medicine, The Chinese University of Hong Kong, Room 124021, 10/F, Lui Che Woo Clinical Sciences Building, Prince of Wales Hospital, Shatin, New Territories, Hong Kong, Email rubyyu@cuhk.edu.hkObjective: This study examined the psychometric properties of the Cantonese version of the SarQoL® questionnaire.Participants: A total of 118 (including 60 non-sarcopenic and 58 sarcopenic) community-dwelling older adults aged 65 years or above with Cantonese as their mother tongue.Methods: Translation and cultural adaptation of the SarQoL were conducted using a standardized protocol. To validate the Cantonese SarQoL, psychometric properties including discriminative power, reliability (including internal consistency and test–retest reliability), and construct validity (including convergent and divergent validity), as well as floor and ceiling effects, were assessed.Results: The translation of the questionnaire was completed without significant difficulties. Results indicated that the Cantonese SarQoL had (1) good discriminative power (sarcopenic participants had lower overall scores, mean = 66.1 vs 75.0, p < 0.001; the overall score was negatively predictive of the presence of sarcopenia, adjusted OR = 0.949, 95% CI = [0.912, 0.983]), (2) good internal consistency (Cronbach’s alpha = 0.835; correlations between domain and overall scores ranged from 0.576 to 0.868), (3) excellent test-retest agreement (intraclass correlation coefficient = 0.801), (4) good construct validity (convergent: moderate to strong correlations were found between the overall score and almost all of the SF-36 and EQ-5D domains; divergent: weaker correlations were found between the overall score and SF-36 social functioning, ρ = − 0.098, and EQ-5D self-care, ρ = − 0.331), and (5) no floor or ceiling effect.Conclusion: The Cantonese SarQoL is valid and reliable, and thus can be used as an interviewer-administered questionnaire for assessing sarcopenia-specific quality of life in fieldwork practice.Keywords: interviewer-administered questionnaire, psychometric, quality of life, sarcopenia, SarQoL, translation, validation

Published
2023

2. ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields

Author

Merlin, E., Santini, P., Paris, D., Castellano, M., Fontana, A., Treu, T., Finkelstein, S. L., Dunlop, J. S., Haro, P. Arrabal, Bagley, M., Boyett, K., Calabrò, A., Correnti, M., Davis, K., Dickinson, M., Donnan, C. T., Ferguson, H. C., Fortuni, F., Giavalisco, M., Glazebrook, K., Grazian, A., Grogin, N. A., Hathi, N., Hirschmann, M., Kartaltepe, J. S., Kewley, L. J., Kirkpatrick, A., Kocevski, D. D., Koekemoer, A. M., Leung, G., Lotz, J. M., Lucas, R. A., Magee, D. K., Marchesini, D., Mascia, S., McLeod, D. J., McLure, R. J., Nanayakkara, T., Napolitano, L., Nonino, M., Papovich, C., Pentericci, L., Pérez-González, P. G., Pirzkal, N., Ravindranath, S., Roberts-Borsani, G., Somerville, R. S., Trenti, M., Trump, J. R., Vulcani, B., Wang, X., Watson, P. J., Wilkins, S. M., Yang, G., and Yung, L. Y. A.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present a set of photometric catalogs primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the high redshift Universe. The set gathers data from eight JWST NIRCam observational programs, targeting the Abell 2744 (GLASS-JWST, UNCOVER, DDT2756 and GO3990), EGS (CEERS), COSMOS and UDS (PRIMER), and GOODS North and South (JADES and NGDEEP) deep fields, for a total area of $\sim$0.2 sq. degrees. Photometric estimates are obtained by means of well-established techniques, including tailored improvements designed to enhance the performance on the specific dataset. We also include new measurements from HST archival data, thus collecting 16 bands spanning from 0.44 to 4.44 $\mu$m. A grand total of $\sim$530 thousand sources is detected on stacks of NIRCam 3.56 and 4.44 $\mu$m mosaics. We assess the photometric accuracy by comparing fluxes and colors against archival catalogs. We also provide photometric redshift estimates, statistically validated against a large set of robust spectroscopic data. The catalogs are publicly available on the Astrodeep website., Comment: 28 pages, 16 figures; accepted for publication on Astronomy & Astrophysics

Published
2024
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9. The MOSDEF Survey: Broad Emission Lines at z = 1.4-3.8

Author

Freeman, WR, Siana, B, Kriek, M, Shapley, AE, Reddy, N, Coil, AL, Mobasher, B, Muratov, AL, Azadi, M, Leung, G, Sanders, R, Shivaei, I, Price, SH, Degroot, L, and Kereš, D

Subjects
galaxies: evolution, galaxies: general, galaxies: high-redshift, galaxies: kinematics and dynamics, galaxies: star formation, stars: winds, outflows, astro-ph.GA, stars: winds, outflows, Astronomy & Astrophysics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

We present results from the MOSFIRE Deep Evolution Field survey on broad flux from the nebular emission lines Hα, [N ii], [O iii], Hβ, and [S ii]. The sample consists of 127 star-forming galaxies at 1.37

Published
2019

10. The MOSDEF Survey: Significant Evolution in the Rest-frame Optical Emission Line Equivalent Widths of Star-forming Galaxies at z = 1.4-3.8

Author

Reddy, NA, Shapley, AE, Sanders, RL, Kriek, M, Coil, AL, Shivaei, I, Freeman, WR, Mobasher, B, Siana, B, Azadi, M, Fetherolf, T, Fornasini, FM, Leung, G, Price, SH, Zick, T, and Barro, G

Subjects
dark ages, reionization, first stars, galaxies: abundances, galaxies: evolution, galaxies: high-redshift, galaxies: ISM, astro-ph.GA, dark ages, reionization, first stars, Astronomical And Space Sciences, Organic Chemistry, Physical Chemistry, Astronomy & Astrophysics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

We use extensive spectroscopy from the MOSFIRE Deep Evolution Field survey to investigate the relationships between rest-frame optical emission line equivalent widths (W) and a number of galaxy and interstellar medium (ISM) characteristics for a sample of 1134 star-forming galaxies at redshifts 1.4 ≲ z ≲ 3.8. We examine how the equivalent widths of , , λλ4960, 5008, + Hβ, , and , depend on stellar mass, UV slope, age, star formation rate (SFR) and specific SFR (sSFR), ionization parameter and excitation conditions (O32 and /Hβ), gas-phase metallicity, and ionizing photon production efficiency (ξ ion). The trend of increasing W with decreasing stellar mass is strongest for (and +Hβ). More generally, the equivalent widths of all the lines increase with redshift at a fixed stellar mass or fixed gas-phase metallicity, suggesting that high equivalent width galaxies are common at high redshift. This redshift evolution in equivalent widths can be explained by the increase in SFR and decrease in metallicity with redshift at a fixed stellar mass. Consequently, the dependence of W on sSFR is largely invariant with redshift, particularly when examined for galaxies of a given metallicity. Our results show that high equivalent width galaxies, specifically those with high , have low stellar masses, blue UV slopes, young ages, high sSFRs, ISM line ratios indicative of high ionization parameters, high ξ ion, and low metallicities. As these characteristics are often attributed to galaxies with high ionizing escape fractions, galaxies with high W are likely candidates for the population that dominates cosmic reionization.

Published
2018

11. The Close AGN Reference Survey (CARS): Mrk 1018 halts dimming and experiences strong short-term variability

Author

Krumpe, M., Husemann, B., Tremblay, G. R., Urrutia, T., Powell, M., Davis, T. A., Scharwächter, J., Dexter, J., Busch, G., Combes, F., Croom, S. M., Eckart, A., McElroy, R. E., Perez-Torres, M., and Leung, G.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract

After changing optical AGN type from 1.9 to 1 in 1984, the AGN Mrk 1018 recently reverted back to its type 1.9 state. Our ongoing monitoring now reveals that the AGN has halted its dramatic dimming, reaching a minimum around October 2016. The minimum was followed by an outburst rising with $\sim$0.25 U-band mag/month. The rebrightening lasted at least until February 2017, as confirmed by joint Chandra and Hubble observations. Monitoring was resumed in July 2017 after the source emerged from sunblock, at which point the AGN was found only $\sim$0.4 mag brighter than its minimum. The intermittent outburst was accompanied by the appearance of a red wing asymmetry in broad-line shape, indicative of an inhomogeneous broad-line region. The current flickering brightness of Mrk 1018 following its rapid fading either suggests that the source has reignited, remains variable at a low level, or may continue dimming over the next few years. Distinguishing between these possibilities requires continuous multiwavelength monitoring., Comment: 5 pages, 4 figures, 1 table, accepted as letter for publication in A&A

Published
2017
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13. The MOSDEF Survey: Stellar Continuum Spectra and Star Formation Histories of Active, Transitional, and Quiescent Galaxies at 1.4 < z < 2.6

Author

Zick, TO, Kriek, M, Shapley, AE, Reddy, NA, Freeman, WR, Siana, B, Coil, AL, Azadi, M, Barro, G, Fetherolf, T, Fornasini, FM, De Groot, L, Leung, G, Mobasher, B, Price, SH, Sanders, RL, and Shivaei, I

Subjects
galaxies: evolution, galaxies: high-redshift, astro-ph.GA, Astronomical And Space Sciences, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

Using the MOSFIRE Deep Evolution Field (MOSDEF) rest-frame optical spectroscopic survey, we investigate the star formation histories (SFHs) of different galaxy types, ranging from actively star-forming to quiescent at 1.4 ≤ z ≤ 2.6. SFHs are constrained utilizing stellar continuum spectroscopy, specifically through a combination of Balmer absorption lines, the 4000 Å break, and the equivalent width of the Hα emission line. To attain a sufficiently high signal-to-noise ratio (S/N) to conduct these measurements we stack spectra of galaxies with similar spectral types, as determined from their rest-frame U - V and V - J colors. We bin the MOSDEF sample into five spectral types, subdividing the quiescent and star-forming bins to better explore galaxies transitioning between the two. We constrain the average SFHs for each type, finding that quiescent and transitional galaxies in the MOSDEF sample are dominated by an SFH with an average star formation timescale of τ ∼ 0.1-0.2 Gyr. These findings contrast with measurements from the low-redshift Universe where, on average, galaxies form their stars over a more extended time period (τ > 1 Gyr). Furthermore, our spectral index measurements correlate with mass surface density for all spectral types. Finally, we compare the average properties of the galaxies in our transitional bins to investigate possible paths to quiescence, and speculate on the viability of a dusty post-starburst phase.

Published
2018

14. The MOSDEF Survey: A Stellar Mass-SFR-Metallicity Relation Exists at z ∼ 2.3

Author

Sanders, RL, Shapley, AE, Kriek, M, Freeman, WR, Reddy, NA, Siana, B, Coil, AL, Mobasher, B, Davé, R, Shivaei, I, Azadi, M, Price, SH, Leung, G, Fetherholf, T, Groot, LD, Zick, T, Fornasini, FM, and Barro, G

Subjects
galaxies: abundances, galaxies: high redshift, astro-ph.GA, Astronomical And Space Sciences, Organic Chemistry, Physical Chemistry, Astronomy & Astrophysics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

We investigate the nature of the relation among stellar mass, star formation rate, and gas-phase metallicity (the M∗-SFR-Z relation) at high redshifts using a sample of 260 star-forming galaxies at z∼2.3 from the MOSDEF survey. We present an analysis of the high-redshift M∗-SFR-Z relation based on several emission-line ratios for the first time. We show that a M∗-SFR-Z relation clearly exists at z∼2.3. The strength of this relation is similar to predictions from cosmological hydrodynamical simulations. By performing a direct comparison of stacks of z∼0 and z∼2.3 galaxies, we find that z∼2.3 galaxies have ∼0.1 dex lower metallicity at fixed M∗ and SFR. In the context of chemical evolution models, this evolution of the M∗-SFR-Z relation suggests an increase with redshift of the mass-loading factor at fixed M∗, as well as a decrease in the metallicity of infalling gas that is likely due to a lower importance of gas recycling relative to accretion from the intergalactic medium at high redshifts. Performing this analysis simultaneously with multiple metallicity-sensitive line ratios allows us to rule out the evolution in physical conditions (e.g., N/O ratio, ionization parameter, and hardness of the ionizing spectrum) at fixed metallicity as the source of the observed trends with redshift and with SFR at fixed M∗ at z∼2.3. While this study highlights the promise of performing high-order tests of chemical evolution models at high redshifts, detailed quantitative comparisons ultimately await a full understanding of the evolution of metallicity calibrations with redshift.

Published
2018

15. The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, ξ ion, at z ∼ 2

Author

Shivaei, I, Reddy, NA, Siana, B, Shapley, AE, Kriek, M, Mobasher, B, Freeman, WR, Sanders, RL, Coil, AL, Price, SH, Fetherolf, T, Azadi, M, Leung, G, and Zick, T

Subjects
dark ages, reionization, first stars, galaxies: general, galaxies: high-redshift, galaxies: star formation, H II regions, astro-ph.GA, dark ages, reionization, first stars, Astronomical And Space Sciences, Organic Chemistry, Physical Chemistry, Astronomy & Astrophysics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

We combine Hα and Hβ spectroscopic measurements and UV photometry for a sample of 673 galaxies from the MOSDEF survey to constrain hydrogen-ionizing photon production efficiencies (ζion) at z = 1.4-2.6. We find 〈log(ζion/[s-1erg s-1Hz-1])〉=25.06(25.34), assuming the Calzetti (SMC) curve for the UV dust correction and a scatter of 0.28 dex in the ζiondistribution. After accounting for observational uncertainties and variations in dust attenuation, we conclude that the remaining scatter in ζionis likely dominated by galaxy-to-galaxy variations in stellar populations, including the slope and upper-mass cutoff of the initial mass function, stellar metallicity, star formation burstiness, and stellar evolution (e.g., single/binary star evolution). Moreover, ζionis elevated in galaxies with high ionization states (high [O iii]/[O ii]) and low oxygen abundances (low [N ii]/Hα and high [O iii]/Hβ) in the ionized ISM. However, ζiondoes not correlate with the offset from the z ∼ 0 star-forming locus in the BPT diagram, suggesting no change in the hardness of the ionizing radiation accompanying the offset from the z ∼ 0 sequence. We also find that galaxies with blue UV spectral slopes (〈β〉=-2.1) have ζionelevated by a factor of ∼2 relative to the average ζionof the sample (〈β〉=-1.4). If these blue galaxies are similar to those at z > 6, our results suggest that a lower Lyman-continuum escape fraction is required for galaxies to maintain reionization, compared to the canonical predictions from stellar population models. Furthermore, we demonstrate that even with robustly dust-corrected Hα, the UV dust attenuation can cause on average a ∼0.3 dex systematic uncertainty in calculations.

Published
2018

16. The birth of radio millisecond pulsars and their high-energy signature

Author

Tam, P. H. T., Li, K. L., Kong, A. K. H., Takata, J., Leung, G. C. K., Cheng, K. S., and Hui, C. Y.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract

Millisecond pulsars (MSPs) are thought to born in low-mass X-ray binaries when the neutron star has gained enough angular momentum from the accreting materials of its companion star. It is generally believed that a radio MSP is born when the neutron star stops accreting and enters a rotation-powered state. Exactly what happens during the transition time was poorly understood until a year ago. In the past year, observations have revealed a few objects that not only switched from one state to the other (as predicted in the above picture), but also have swung between the two states within weeks to years. In this work, we present observations of two of these transition objects (PSR J1023+0038 and XSS J12270-4859) and a theoretical framework that tries to explain their high-energy radiation., Comment: 7 pages, 6 figures; presented at the 10th INTEGRAL Workshop: 'A Synergistic View of the High Energy Sky' - Integral2014, held 15-19 September 2014, Annapolis, MD

Published
2014

18. High-Energy Emission of the First Millisecond Pulsar

Author

Ng, C. -Y., Takata, J., Leung, G. C. K., Cheng, K. S., and Philippopoulos, P.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report on X-ray and gamma-ray observations of the millisecond pulsar B1937+21 taken with the Chandra X-ray Observatory, XMM-Newton, and the Fermi Large Area Telescope. The pulsar X-ray emission shows a purely non-thermal spectrum with a hard photon index of 0.9+/-0.1, and is nearly 100% pulsed. We found no evidence of varying pulse profile with energy as previously claimed. We also analyzed 5.5 yr of Fermi survey data and obtained much improved constraints on the pulsar's timing and spectral properties in gamma-rays. The pulsed spectrum is adequately fitted by a simple power-law with a photon index of 2.38+/-0.07. Both the gamma-ray and X-ray pulse profiles show similar two-peak structure and generally align with the radio peaks. We found that the aligned profiles and the hard spectrum in X-rays seem to be common properties among millisecond pulsars with high magnetic fields at the light cylinder. We discuss a possible physical scenario that could give rise to these features., Comment: 10 pages, 4 figures, accepted for publication in ApJ

Published
2014
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19. Multi-wavelength emissions from the millisecond pulsar binary PSR J1023+0038 during an accretion active state

Author

Takata, J., Li, K. L., Leung, G. C. K., Kong, A. K. H., Tam, P. H. T., Hui, C. Y., Wu, E. M. H., Xing, Y., Cao, Y., Tang, S., Wang, Z., and Cheng, K. S.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Recent observations strongly suggest that the millisecond pulsar binary PSR J1023+0038 has developed an accretion disk since 2013 June. We present a multi-wavelength analysis of PSR J1023+0038, which reveals that 1) its gamma-rays suddenly brightened within a few days in June/July 2013 and has remained at a high gamma-ray state for several months; 2) both UV and X-ray fluxes have increased by roughly an order of magnitude, and 3) the spectral energy distribution has changed significantly after the gamma-ray sudden flux change. Time variabilities associated with UV and X-rays are on the order of 100-500 seconds and 50-100 seconds, respectively. Our model suggests that a newly formed accretion disk due to the sudden increase of the stellar wind could explain the changes of all these observed features. The increase of UV is emitted from the disk, and a new component in gamma-rays is produced by inverse Compton scattering between the new UV component and pulsar wind. The increase of X-rays results from the enhancement of injection pulsar wind energy into the intra-binary shock due to the increase of the stellar wind. We also predict that the radio pulses may be blocked by the evaporated winds from the disk and the pulsar is still powered by rotation., Comment: 8 pages, 3 figures; accepted for publication in ApJ

Published
2013
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22. Worldwide comparison of survival from childhood leukaemia for 1995–2009, by subtype, age, and sex (CONCORD-2): a population-based study of individual data for 89 828 children from 198 registries in 53 countries

Author

Bouzbid, S, Hamdi-Chérif, M, Zaidi, Z, Bah, E, Swaminathan, R, Nortje, SH, El Mistiri, MM, Bayo, S, Malle, B, Manraj, SS, Sewpaul-Sungkur, R, Fabowale, Ogunbiyi, OJ, Bradshaw, D, Somdyala, NIM, Stefan, DC, Abdel-Rahman, M, Jaidane, L, Mokni, M, Kumcher, I, Moreno, F, González, MS, Laura, EA, Espinola, SB, Calabrano, GH, Carballo Quintero, B, Fita, R, Garcilazo, DA, Giacciani, PL, Diumenjo, MC, Laspada, WD, Green, MA, Lanza, MF, Ibañez, SG, Lima, CA, de Oliveira, E Lobo, Daniel, C, Scandiuzzi, C, De Souza, PCF, Melo, CD, Del Pino, K, Laporte, C, Curado, MP, de Oliveira, JC, Veneziano, CLA, Veneziano, DB, Azevedo e Silva, G, Galaz, JC, Moya, JA, Herrmann, DA, Vargas, S, Herrera, VM, Uribe, CJ, Bravo, LE, Arias-Ortiz, NE, Jurado, DM, Yépez, MC, Galán, YH, Torres, P, Martínez-Reyes, F, Pérez-Meza, ML, Jaramillo, L, Quinto, R, Cueva, P, Yépez, JG, Torres-Cintrón, CR, Tortolero-Luna, G, Alonso, R, Barrios, E, Nikiforuk, C, Shack, L, Coldman, AJ, Woods, RR, Noonan, G, Turner, D, Kumar, E, Zhang, B, McCrate, FR, Ryan, S, Hannah, H, Dewar, RAD, MacIntyre, M, Lalany, A, Ruta, M, Marrett, L, Nishri, DE, McClure, C, Vriends, KA, Bertrand, C, Louchini, R, Robb, KI, Stuart-Panko, H, Demers, S, Wright, S, George, JT, Shen, X, Brockhouse, JT, O'Brien, DK, Ward, KC, Almon, L, Bates, J, Rycroft, R, Mueller, L, Phillips, C, Brown, H, Cromartie, B, Schwartz, AG, Vigneau, F, MacKinnon, JA, Wohler, B, Bayakly, AR, Clarke, CA, Glaser, SL, West, D, Green, MD, Hernandez, BY, Johnson, CJ, Jozwik, D, Charlton, ME, Lynch, CF, Huang, B, Tucker, TC, Deapen, D, Liu, L, Hsieh, MC, Wu, XC, Stern, K, Gershman, ST, Knowlton, RC, Alverson, J, Copeland, GE, Rogers, DB, Lemons, D, Williamson, LL, Hood, M, Hosain, GM, Rees, JR, Pawlish, KS, Stroup, A, Key, C, Wiggins, C, Kahn, AR, Schymura, MJ, Leung, G, Rao, C, Giljahn, L, Warther, B, Pate, A, Patil, M, Schubert, SS, Rubertone, JJ, Slack, SJ, Fulton, JP, Rousseau, DL, Janes, TA, Schwartz, SM, Bolick, SW, Hurley, DM, Richards, J, Whiteside, MA, Nogueira, LM, Herget, K, Sweeney, C, Martin, J, Wang, S, Harrelson, DG, Cheteri, MB Keitheri, Farley, S, Hudson, AG, Borchers, R, Stephenson, L, Espinoza, JR, Weir, HK, Edwards, BK, Wang, N, Yang, L, Chen, JS, Song, GH, Gu, XP, Zhang, P, Ge, HM, Zhao, DL, Zhang, JH, Zhu, FD, Tang, JG, Shen, Y, Wang, J, Li, QL, Yang, XP, Dong, J, Li, W, Cheng, LP, Chen, JG, Huang, QH, Huang, SQ, Guo, GP, Wei, K, Chen, WQ, Zeng, H, Demetriou, AV, Pavlou, P, Mang, WK, Ngan, KC, Kataki, AC, Krishnatreya, M, Jayalekshmi, PA, Sebastian, P, Sapkota, SD, Verma, Y, Nandakumar, A, Suzanna, E, Keinan-Boker, L, Silverman, BG, Ito, H, Nakagawa, H, Hattori, M, Kaizaki, Y, Sugiyama, H, Utada, M, Katayama, K, Narimatsu, H, Kanemura, S, Koike, T, Miyashiro, I, Yoshii, M, Oki, I, Shibata, A, Matsuda, T, Nimri, O, Ab Manan, A, Pathy, N Bhoo, Chimedsuren, O, Tuvshingerel, S, Al Khater, AHM, Al-Eid, H, Jung, KW, Won, YJ, Chiang, CJ, Lai, MS, Suwanrungruang, K, Wiangnon, S, Daoprasert, K, Pongnikorn, D, Geater, SL, Sriplung, H, Eser, S, Yakut, CI, Hackl, M, Mühlböck, H, Oberaigner, W, Zborovskaya, AA, Aleinikova, OV, Henau, K, Van Eycken, L, Dimitrova, N, Valerianova, Z, Šekerija, M, Zvolský, M, Engholm, G, Storm, H, Innos, K, Mägi, M, Malila, N, Seppä, K, Jégu, J, Velten, M, Cornet, E, Troussard, X, Bouvier, AM, Faivre, J, Guizard, AV, Bouvier, V, Launoy, G, Arveux, P, Maynadié, M, Mounier, M, Fournier, E, Woronoff, AS, Daoulas, M, Clavel, J, Le Guyader-Peyrou, S, Monnereau, A, Trétarre, B, Colonna, M, Cowppli-Bony, A, Molinié, F, Bara, S, Degré, D, Ganry, O, Lapôtre-Ledoux, B, Grosclaude, P, Estève, J, Bray, F, Piñeros, M, Sassi, F, Stabenow, R, Eberle, A, Erb, C, Nennecke, A, Kieschke, J, Sirri, E, Kajueter, H, Emrich, K, Zeissig, SR, Holleczek, B, Eisemann, N, Katalinic, A, Brenner, H, Asquez, RA, Kumar, V, Ólafsdóttir, EJ, Tryggvadóttir, L, Comber, H, Walsh, PM, Sundseth, H, Devigili, E, Mazzoleni, G, Giacomin, A, Bella, F, Castaing, M, Sutera, A, Gola, G, Ferretti, S, Serraino, D, Zucchetto, A, Lillini, R, Vercelli, M, Busco, S, Pannozzo, F, Vitarelli, S, Ricci, P, Pascucci, C, Autelitano, M, Cirilli, C, Federico, M, Fusco, M, Vitale, MF, Usala, M, Cusimano, R, Mazzucco, W, Michiara, M, Sgargi, P, Maule, MM, Sacerdote, C, Tumino, R, Di Felice, E, Vicentini, M, Falcini, F, Cremone, L, Budroni, M, Cesaraccio, R, Contrino, ML, Tisano, F, Fanetti, AC, Maspero, S, Candela, G, Scuderi, T, Gentilini, MA, Piffer, S, Rosso, S, Sacchetto, L, Caldarella, A, La Rosa, F, Stracci, F, Contiero, P, Tagliabue, G, Dei Tos, AP, Zorzi, M, Zanetti, R, Baili, P, Berrino, F, Gatta, G, Sant, M, Capocaccia, R, De Angelis, R, Liepina, E, Maurina, A, Smailyte, G, Agius, D, Calleja, N, Siesling, S, Visser, O, Larønningen, S, Møller, B, Dyzmann-Sroka, A, Trojanowski, M, Gózdz, S, Mezyk, R, Gradalska-Lampart, M, Radziszewska, AU, Didkowska, JA, Wojciechowska, U, Blaszczyk, J, Kepska, K, Bielska-Lasota, M, Kwiatkowska, K, Forjaz, G, Rego, RA, Bastos, J, Silva, MA, Antunes, L, Bento, MJ, Mayer-da-Silva, A, Miranda, A, Coza, D, Todescu, AI, Valkov, MY, Adamcik, J, Safaei Diba, C, Primic-Žakelj, M, Žagar, T, Stare, J, Almar, E, Mateos, A, Quirós, JR, Bidaurrazaga, J, Larrañaga, N, Díaz García, JM, Marcos, AI, Marcos-Gragera, R, Vilardell Gil, ML, Molina, E, Sánchez, MJ, Sureda, P Franch, Montserrat, M Ramos, Chirlaque, MD, Navarro, C, Ardanaz, EE, Moreno-Iribas, CC, Fernández-Delgado, R, Peris-Bonet, R, Galceran, J, Khan, S, Lambe, M, Camey, B, Bouchardy, C, Usel, M, Ess, SM, Herrmann, C, Bulliard, JL, Maspoli-Conconi, M, Frick, H, Kuehni, CE, Schindler, M, Bordoni, A, Spitale, A, Chiolero, A, Konzelmann, I, Dehler, SI, Matthes, KL, Rashbass, J, Stiller, CA, Fitzpatrick, D, Gavin, A, Bannon, F, Black, RJ, Brewster, DH, Huws, DW, White, C, Finan, P, Allemani, C, Bonaventure, A, Carreira, H, Coleman, MP, Di Carlo, V, Harewood, R, Liu, K, Matz, M, Montel, L, Nikšić, M, Rachet, B, Sanz, N, Spika, D, Stephens, R, Peake, M, Murphy, MFG, Chalker, E, Newman, L, Baker, D, Soeberg, MJ, Aitken, J, Scott, C, Stokes, BC, Venn, A, Farrugia, H, Giles, GG, Threlfall, T, Currow, D, You, H, Hendrix, J, Lewis, C, Latorre, MRDO, Tanaka, LF, Bonaventure, Audrey, Harewood, Rhea, Stiller, Charles A, Gatta, Gemma, Clavel, Jacqueline, Stefan, Daniela C, Carreira, Helena, Spika, Devon, Marcos-Gragera, Rafael, Peris-Bonet, Rafael, Piñeros, Marion, Sant, Milena, Kuehni, Claudia E, Murphy, Michael F G, Coleman, Michel P, and Allemani, Claudia

Published
2017
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23. The histology of ovarian cancer: worldwide distribution and implications for international survival comparisons (CONCORD-2)

Author

Bouzbid, S., Hamdi-Chérif, M., Zaidi, Z., Bah, E., Swaminathan, R., Nortje, S.H., Stefan, D.C., El Mistiri, M.M., Bayo, S., Malle, B., Manraj, S.S., Sewpaul-Sungkur, R., Fabowale, A., Ogunbiyi, O.J., Bradshaw, D., Somdyala, N.I.M., Abdel-Rahman, M., Jaidane, L., Mokni, M., Kumcher, I., Moreno, F., González, M.S., Laura, E.A., Espinola, S.B., Calabrano, G.H., Carballo Quintero, B., Fita, R., Garcilazo, D.A., Giacciani, P.L., Diumenjo, M.C., Laspada, W.D., Green, M.A., Lanza, M.F., Ibañez, S.G., Lima, C.A., Lobo de Oliveira, E., Daniel, C., Scandiuzzi, C., De Souza, P.C.F., Melo, C.D., Del Pino, K., Laporte, C., Curado, M.P., de Oliveira, J.C., Veneziano, C.L.A., Veneziano, D.B., Alexandre, T.S., Verdugo, A.S., Azevedo e Silva, G., Galaz, J.C., Moya, J.A., Herrmann, D.A., Vargas, S., Herrera, V.M., Uribe, C.J., Bravo, L.E., Arias-Ortiz, N.E., Jurado, D.M., Yépez, M.C., Galán, Y.H., Torres, P., Martínez-Reyes, F., Pérez-Meza, M.L., Jaramillo, L., Quinto, R., Cueva, P., Yépez, J.G., Torres-Cintrón, C.R., Tortolero-Luna, G., Alonso, R., Barrios, E., Nikiforuk, C., Shack, L., Coldman, A.J., Woods, R.R., Noonan, G., Turner, D., Kumar, E., Zhang, B., McCrate, F.R., Ryan, S., Hannah, H., Dewar, R.A.D., MacIntyre, M., Lalany, A., Ruta, M., Marrett, L., Nishri, D.E., McClure, C., Vriends, K.A., Bertrand, C., Louchini, R., Robb, K.I., Stuart-Panko, H., Demers, S., Wright, S., George, J.T., Shen, X., Brockhouse, J.T., O'Brien, D.K., Ward, K.C., Almon, L., Bates, J., Rycroft, R., Mueller, L., Phillips, C., Brown, H., Cromartie, B., Schwartz, A.G., Vigneau, F., MacKinnon, J.A., Wohler, B., Bayakly, A.R., Clarke, C.A., Glaser, S.L., West, D., Green, M.D., Hernandez, B.Y., Johnson, C.J., Jozwik, D., Charlton, M.E., Lynch, C.F., Huang, B., Tucker, T.C., Deapen, D., Liu, L., Hsieh, M.C., Wu, X.C., Stern, K., Gershman, S.T., Knowlton, R.C., Alverson, J., Copeland, G.E., Rogers, D.B., Lemons, D., Williamson, L.L., Hood, M., Hosain, G.M., Rees, J.R., Pawlish, K.S., Stroup, A., Key, C., Wiggins, C., Kahn, A.R., Schymura, M.J., Leung, G., Rao, C., Giljahn, L., Warther, B., Pate, A., Patil, M., Schubert, S.S., Rubertone, J.J., Slack, S.J., Fulton, J.P., Rousseau, D.L., Janes, T.A., Schwartz, S.M., Bolick, S.W., Hurley, D.M., Richards, J., Whiteside, M.A., Nogueira, L.M., Herget, K., Sweeney, C., Martin, J., Wang, S., Harrelson, D.G., Keitheri Cheteri, M.B., Farley, S., Hudson, A.G., Borchers, R., Stephenson, L., Espinoza, J.R., Weir, H.K., Edwards, B.K., Wang, N., Yang, L., Chen, J.S., Song, G.H., Gu, X.P., Zhang, P., Ge, H.M., Zhao, D.L., Zhang, J.H., Zhu, F.D., Tang, J.G., Shen, Y., Wang, J., Li, Q.L., Yang, X.P., Dong, J., Li, W., Cheng, L.P., Chen, J.G., Huang, Q.H., Huang, S.Q., Guo, G.P., Wei, K., Chen, W.Q., Zeng, H., Demetriou, A.V., Pavlou, P., Mang, W.K., Ngan, K.C., Kataki, A.C., Krishnatreya, M., Jayalekshmi, P.A., Sebastian, P., Sapkota, S.D., Verma, Y., Nandakumar, A., Suzanna, E., Keinan-Boker, L., Silverman, B.G., Ito, H., Nakagawa, H., Hattori, M., Kaizaki, Y., Sugiyama, H., Utada, M., Katayama, K., Narimatsu, H., Kanemura, S., Koike, T., Miyashiro, I., Yoshii, M., Oki, I., Shibata, A., Matsuda, T., Nimri, O., Ab Manan, A., Bhoo Pathy, N., Chimedsuren, O., Tuvshingerel, S., Al Khater, A.H.M., Al-Eid, H., Jung, K.W., Won, Y.J., Chiang, C.J., Lai, M.S., Suwanrungruang, K., Wiangnon, S., Daoprasert, K., Pongnikorn, D., Geater, S.L., Sriplung, H., Eser, S., Yakut, C.I., Hackl, M., Mühlböck, H., Oberaigner, W., Zborovskaya, A.A., Aleinikova, O.V., Henau, K., Van Eycken, L., Dimitrova, N., Valerianova, Z., Šekerija, M., Zvolský, M., Engholm, G., Storm, H., Innos, K., Mägi, M., Malila, N., Seppä, K., Jégu, J., Velten, M., Cornet, E., Troussard, X., Bouvier, A.M., Faivre, J., Guizard, A.V., Bouvier, V., Launoy, G., Arveux, P., Maynadié, M., Mounier, M., Fournier, E., Woronoff, A.S., Daoulas, M., Clavel, J., Le Guyader-Peyrou, S., Monnereau, A., Trétarre, B., Colonna, M., Cowppli-Bony, A., Molinié, F., Bara, S., Degré, D., Ganry, O., Lapôtre-Ledoux, B., Grosclaude, P., Estève, J., Bray, F., Piñeros, M., Sassi, F., Stabenow, R., Eberle, A., Erb, C., Nennecke, A., Kieschke, J., Sirri, E., Kajueter, H., Emrich, K., Zeissig, S.R., Holleczek, B., Eisemann, N., Katalinic, A., Brenner, H., Asquez, R.A., Kumar, V., Ólafsdóttir, E.J., Tryggvadóttir, L., Comber, H., Walsh, P.M., Sundseth, H., Devigili, E., Mazzoleni, G., Giacomin, A., Bella, F., Castaing, M., Sutera, A., Gola, G., Ferretti, S., Serraino, D., Zucchetto, A., Lillini, R., Vercelli, M., Busco, S., Pannozzo, F., Vitarelli, S., Ricci, P., Pascucci, C., Autelitano, M., Cirilli, C., Federico, M., Fusco, M., Vitale, M.F., Usala, M., Cusimano, R., Mazzucco, W., Michiara, M., Sgargi, P., Maule, M.M., Sacerdote, C., Tumino, R., Di Felice, E., Vicentini, M., Falcini, F., Cremone, L., Budroni, M., Cesaraccio, R., Contrino, M.L., Tisano, F., Fanetti, A.C., Maspero, S., Candela, G., Scuderi, T., Gentilini, M.A., Piffer, S., Rosso, S., Sacchetto, L., Caldarella, A., La Rosa, F., Stracci, F., Contiero, P., Tagliabue, G., Dei Tos, A.P., Zorzi, M., Zanetti, R., Baili, P., Berrino, F., Gatta, G., Sant, M., Capocaccia, R., De Angelis, R., Liepina, E., Maurina, A., Smailyte, G., Agius, D., Calleja, N., Siesling, S., Visser, O., Larønningen, S., Møller, B., Dyzmann-Sroka, A., Trojanowski, M., Góźdż, S., Mężyk, R., Grądalska-Lampart, M., Radziszewska, A.U., Didkowska, J.A., Wojciechowska, U., Błaszczyk, J., Kępska, K., Bielska-Lasota, M., Kwiatkowska, K., Forjaz, G., Rego, R.A., Bastos, J., Silva, M.A., Antunes, L., Bento, M.J., Mayer-da-Silva, A., Miranda, A., Coza, D., Todescu, A.I., Valkov, M.Y., Adamcik, J., Safaei Diba, C., Primic-Žakelj, M., Žagar, T., Stare, J., Almar, E., Mateos, A., Quirós, J.R., Bidaurrazaga, J., Larrañaga, N., Díaz García, J.M., Marcos, A.I., Marcos-Gragera, R., Vilardell Gil, M.L., Molina, E., Sánchez, M.J., Franch Sureda, P., Ramos Montserrat, M., Chirlaque, M.D., Navarro, C., Ardanaz, E.E., Moreno-Iribas, C.C., Fernández-Delgado, R., Peris-Bonet, R., Galceran, J., Khan, S., Lambe, M., Camey, B., Bouchardy, C., Usel, M., Ess, S.M., Herrmann, C., Bulliard, J.L., Maspoli-Conconi, M., Frick, H., Kuehni, C.E., Schindler, M., Bordoni, A., Spitale, A., Chiolero, A., Konzelmann, I., Dehler, S.I., Matthes, K.L., Rashbass, J., Stiller, C., Fitzpatrick, D., Gavin, A., Bannon, F., Black, R.J., Brewster, D.H., Huws, D.W., White, C., Finan, P., Allemani, C., Bonaventure, A., Carreira, H., Coleman, M.P., Di Carlo, V., Harewood, R., Liu, K., Matz, M., Montel, L., Nikšić, M., Rachet, B., Sanz, N., Spika, D., Stephens, R., Peake, M., Chalker, E., Newman, L., Baker, D., Soeberg, M.J., Aitken, J., Scott, C., Stokes, B.C., Venn, A., Farrugia, H., Giles, G.G., Threlfall, T., Currow, D., You, H., Hendrix, J., Lewis, C., Matz, Melissa, Coleman, Michel P, Sant, Milena, Chirlaque, Maria Dolores, Visser, Otto, Gore, Martin, and Allemani, Claudia

Published
2017
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24. Worldwide comparison of ovarian cancer survival: Histological group and stage at diagnosis (CONCORD-2)

Author

Bouzbid, S., Hamdi-Chérif, M., Zaidi, Z., Bah, E., Swaminathan, R., Nortje, S.H., El Mistiri, M.M., Bayo, S., Malle, B., Manraj, S.S., Sewpaul-Sungkur, R., Fabowale, A., Ogunbiyi, O.J., Bradshaw, D., Somdyala, N.I.M., Stefan, D.C., Abdel-Rahman, M., Jaidane, L., Mokni, M., Kumcher, I., Moreno, F., González, M.S., Laura, E.A., Espinola, S.B., Calabrano, G.H., Carballo Quintero, B., Fita, R., Garcilazo, D.A., Giacciani, P.L., Diumenjo, M.C., Laspada, W.D., Green, M.A., Lanza, M.F., Ibañez, S.G., Lima, C.A., Lobo de Oliveira, E., Daniel, C., Scandiuzzi, C., De Souza, P.C.F., Melo, C.D., Del Pino, K., Laporte, C., Curado, M.P., de Oliveira, J.C., Veneziano, C.L.A., Veneziano, D.B., Latorre, M.R.D.O., Tanaka, L.F., Azevedo e Silva, G., Galaz, J.C., Moya, J.A., Herrmann, D.A., Vargas, S., Herrera, V.M., Uribe, C.J., Bravo, L.E., Arias-Ortiz, N.E., Jurado, D.M., Yépez, M.C., Galán, Y.H., Torres, P., Martínez-Reyes, F., Pérez-Meza, M.L., Jaramillo, L., Quinto, R., Cueva, P., Yépez, J.G., Torres-Cintrón, C.R., Tortolero-Luna, G., Alonso, R., Barrios, E., Nikiforuk, C., Shack, L., Coldman, A.J., Woods, R.R., Noonan, G., Turner, D., Kumar, E., Zhang, B., McCrate, F.R., Ryan, S., Hannah, H., Dewar, R.A.D., MacIntyre, M., Lalany, A., Ruta, M., Marrett, L., Nishri, D.E., McClure, C., Vriends, K.A., Bertrand, C., Louchini, R., Robb, K.I., Stuart-Panko, H., Demers, S., Wright, S., George, J.T., Shen, X., Brockhouse, J.T., O'Brien, D.K., Ward, K.C., Almon, L., Bates, J., Rycroft, R., Mueller, L., Phillips, C., Brown, H., Cromartie, B., Schwartz, A.G., Vigneau, F., MacKinnon, J.A., Wohler, B., Bayakly, A.R., Clarke, C.A., Glaser, S.L., West, D., Green, M.D., Hernandez, B.Y., Johnson, C.J., Jozwik, D., Charlton, M.E., Lynch, C.F., Huang, B., Tucker, T.C., Deapen, D., Liu, L., Hsieh, M.C., Wu, X.C., Stern, K., Gershman, S.T., Knowlton, R.C., Alverson, J., Copeland, G.E., Rogers, D.B., Lemons, D., Williamson, L.L., Hood, M., Hosain, G.M., Rees, J.R., Pawlish, K.S., Stroup, A., Key, C., Wiggins, C., Kahn, A.R., Schymura, M.J., Leung, G., Rao, C., Giljahn, L., Warther, B., Pate, A., Patil, M., Schubert, S.S., Rubertone, J.J., Slack, S.J., Fulton, J.P., Rousseau, D.L., Janes, T.A., Schwartz, S.M., Bolick, S.W., Hurley, D.M., Richards, J., Whiteside, M.A., Nogueira, L.M., Herget, K., Sweeney, C., Martin, J., Wang, S., Harrelson, D.G., Keitheri Cheteri, M.B., Farley, S., Hudson, A.G., Borchers, R., Stephenson, L., Espinoza, J.R., Weir, H.K., Edwards, B.K., Wang, N., Yang, L., Chen, J.S., Song, G.H., Gu, X.P., Zhang, P., Ge, H.M., Zhao, D.L., Zhang, J.H., Zhu, F.D., Tang, J.G., Shen, Y., Wang, J., Li, Q.L., Yang, X.P., Dong, J., Li, W., Cheng, L.P., Chen, J.G., Huang, Q.H., Huang, S.Q., Guo, G.P., Wei, K., Chen, W.Q., Zeng, H., Demetriou, A.V., Pavlou, P., Mang, W.K., Ngan, K.C., Kataki, A.C., Krishnatreya, M., Jayalekshmi, P.A., Sebastian, P., Sapkota, S.D., Verma, Y., Nandakumar, A., Suzanna, E., Keinan-Boker, L., Silverman, B.G., Ito, H., Nakagawa, H., Hattori, M., Kaizaki, Y., Sugiyama, H., Utada, M., Katayama, K., Narimatsu, H., Kanemura, S., Koike, T., Miyashiro, I., Yoshii, M., Oki, I., Shibata, A., Matsuda, T., Nimri, O., Ab Manan, A., Bhoo-Pathy, N., Tuvshingerel, S., Chimedsuren, O., Al Khater, A.H.M., Al-Eid, H., Jung, K.W., Won, Y.J., Chiang, C.J., Lai, M.S., Suwanrungruang, K., Wiangnon, S., Daoprasert, K., Pongnikorn, D., Geater, S.L., Sriplung, H., Eser, S., Yakut, C.I., Hackl, M., Mühlböck, H., Oberaigner, W., Zborovskaya, A.A., Aleinikova, O.V., Henau, K., Van Eycken, L., Dimitrova, N., Valerianova, Z., Šekerija, M., Zvolský, M., Engholm, G., Storm, H., Innos, K., Mägi, M., Malila, N., Seppä, K., Jégu, J., Velten, M., Cornet, E., Troussard, X., Bouvier, A.M., Faivre, J., Guizard, A.V., Bouvier, V., Launoy, G., Arveux, P., Maynadié, M., Mounier, M., Fournier, E., Woronoff, A.S., Daoulas, M., Clavel, J., Le Guyader-Peyrou, S., Monnereau, A., Trétarre, B., Colonna, M., Cowppli-Bony, A., Molinié, F., Bara, S., Degré, D., Ganry, O., Lapôtre-Ledoux, B., Grosclaude, P., Estève, J., Bray, F., Piñeros, M., Sassi, F., Stabenow, R., Eberle, A., Erb, C., Nennecke, A., Kieschke, J., Sirri, E., Kajueter, H., Emrich, K., Zeissig, S.R., Holleczek, B., Eisemann, N., Katalinic, A., Brenner, H., Asquez, R.A., Kumar, V., Ólafsdóttir, E.J., Tryggvadóttir, L., Comber, H., Walsh, P.M., Sundseth, H., Devigili, E., Mazzoleni, G., Giacomin, A., Bella, F., Castaing, M., Sutera, A., Gola, G., Ferretti, S., Serraino, D., Zucchetto, A., Lillini, R., Vercelli, M., Busco, S., Pannozzo, F., Vitarelli, S., Ricci, P., Pascucci, C., Autelitano, M., Cirilli, C., Federico, M., Fusco, M., Vitale, M.F., Usala, M., Cusimano, R., Mazzucco, W., Michiara, M., Sgargi, P., Maule, M.M., Sacerdote, C., Tumino, R., Di Felice, E., Vicentini, M., Falcini, F., Cremone, L., Budroni, M., Cesaraccio, R., Contrino, M.L., Tisano, F., Fanetti, A.C., Maspero, S., Candela, G., Scuderi, T., Gentilini, M.A., Piffer, S., Rosso, S., Sacchetto, L., Caldarella, A., La Rosa, F., Stracci, F., Contiero, P., Tagliabue, G., Dei Tos, A.P., Zorzi, M., Zanetti, R., Baili, P., Berrino, F., Gatta, G., Sant, M., Capocaccia, R., De Angelis, R., Liepina, E., Maurina, A., Smailyte, G., Agius, D., Calleja, N., Siesling, S., Visser, O., Larønningen, S., Møller, B., Dyzmann-Sroka, A., Trojanowski, M., Góźdż, S., Mężyk, R., Grądalska-Lampart, M., Radziszewska, A.U., Didkowska, J.A., Wojciechowska, U., Błaszczyk, J., Kępska, K., Bielska-Lasota, M., Kwiatkowska, K., Forjaz, G., Rego, R.A., Bastos, J., Silva, M.A., Antunes, L., Bento, M.J., Mayer-da-Silva, A., Miranda, A., Coza, D., Todescu, A.I., Valkov, M.Y., Adamcik, J., Safaei Diba, C., Primic-Žakelj, M., Žagar, T., Stare, J., Almar, E., Mateos, A., Quirós, J.R., Bidaurrazaga, J., Larrañaga, N., Díaz García, J.M., Marcos, A.I., Marcos-Gragera, R., Vilardell Gil, M.L., Molina, E., Sánchez, M.J., Franch Sureda, P., Ramos Montserrat, M., Chirlaque, M.D., Navarro, C., Ardanaz, E.E., Moreno-Iribas, C.C., Fernández-Delgado, R., Peris-Bonet, R., Galceran, J., Khan, S., Lambe, M., Camey, B., Bouchardy, C., Usel, M., Ess, S.M., Herrmann, C., Bulliard, J.L., Maspoli-Conconi, M., Frick, H., Kuehni, C.E., Schindler, M., Bordoni, A., Spitale, A., Chiolero, A., Konzelmann, I., Dehler, S.I., Matthes, K.L., Rashbass, J., Stiller, C.A., Fitzpatrick, D., Gavin, A., Bannon, F., Black, R.J., Brewster, D.H., Huws, D.W., White, C., Finan, P., Allemani, C., Bonaventure, A., Carreira, H., Coleman, M.P., Di Carlo, V., Harewood, R., Liu, K., Matz, M., Montel, L., Nikšić, M., Rachet, B., Sanz, N., Spika, D., Stephens, R., Peake, M., Chalker, E., Newman, L., Baker, D., Soeberg, M.J., Aitken, J., Scott, C., Stokes, B.C., Venn, A., Farrugia, H., Giles, G.G., Threlfall, T., Currow, D., You, H., Hendrix, J., Lewis, C., Matz, Melissa, Coleman, Michel P, Carreira, Helena, Salmerón, Diego, Chirlaque, Maria Dolores, and Allemani, Claudia

Published
2017
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29. The coupling between tropical meteorology, aerosol lifecycle, convection, and radiation, during the Cloud, Aerosol and Monsoon Processes Philippines Experiment (CAMP2Ex)

Author

Reid, J. S., primary, Maring, H. B., additional, Narisma, G. T., additional, van den Heever, S., additional, Di Girolamo, L., additional, Ferrare, R., additional, Lawson, P., additional, Mace, G. G., additional, Simpas, J. B., additional, Tanelli, S., additional, Ziemba, L., additional, van Diedenhoven, B., additional, Bruintjes, R., additional, Bucholtz, A., additional, Cairns, B., additional, Cambaliza, M. O., additional, Chen, G., additional, Diskin, G. S., additional, Flynn, J. H., additional, Hostetler, C. A., additional, Holz, R. E., additional, Lang, T. J., additional, Schmidt, K. S., additional, Smith, G., additional, Sorooshian, A., additional, Thompson, E. J., additional, Thornhill, K. L., additional, Trepte, C., additional, Wang, J., additional, Woods, S., additional, Yoon, S., additional, Alexandrov, M., additional, Alvarez, S., additional, Amiot, C. G., additional, Bennett, J. R., additional, Brooks, M.,, additional, Burton, S. P., additional, Cayanan, E., additional, Chen, H., additional, Collow, A., additional, Crosbie, E., additional, DaSilva, A., additional, DiGangi, J. P., additional, Flagg, D. D., additional, Freeman, S. W., additional, Fu, D., additional, Fukada, E., additional, Hilario, M. R. A., additional, Hong, Y., additional, Hristova-Veleva, S. M., additional, Kuehn, R., additional, Kowch, R. S., additional, Leung, G. R., additional, Loveridge, J., additional, Meyer, K., additional, Miller, R. M., additional, Montes, M. J., additional, Moum, J. N., additional, Nenes, Thanos, additional, Nesbitt, S. W., additional, Norgren, M., additional, Nowottnick, E. P., additional, Rauber, R. M., additional, Reid, E. A., additional, Rutledge, S., additional, Schlosser, J. S., additional, Sekiyama, T. T., additional, Shook, M. A., additional, Sokolowsky, G. A., additional, Stamnes, S. A., additional, Tanaka, T. Y., additional, Wasilewski, A., additional, Xian, P., additional, Xiao, Q., additional, Xu, Zhuocan, additional, and Zavaleta, J., additional

Published
2023
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30. Different types of visual cells in the photoreceptor layer of the retinae of the treeshrew (Tupaia belangeri chinensis) as revealed by scanning microscopy.

Author

Cheng, R. S. Y., Wai, M. S. M., Leung, G. C. T., Chow, T. C. H., Sze-To, W. W., Yew, D. T., Cheng, Rufina S Y, Leung, Gigi C T, and Chow, Tony C H

Abstract

The retinae of treeshrew have never been evaluated by scanning electron microscopic studies. This work described the visual cells in the photoreceptor layer of the retinae of treeshrew (Tupaia belangeri chinensis) living on the high plateau of Yunnan, China, via scanning electron microscopy. Results indicated five different types of cones morphologically, in which two of those have shown oil droplet like structures in their inner segments. To our knowledge, no prior studies have reported oil droplets in the visual cells of higher mammals, only in lower vertebrate and primitive mammals. In addition, this study revealed one type of degenerative visual cell without outer segments. The findings signal the needs for additional studies to understand the physiological functions and phylogenetic relationships of the diversity of visual cells in this group of mammal. [ABSTRACT FROM AUTHOR]

Published
2023
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41. Perspectives on Family Health, Happiness and Harmony (3H) among Hong Kong Chinese People: A Qualitative Study

Author

Lam, W. W. T., Fielding, R., McDowell, I., Johnston, J., Chan, Sophia, Leung, G. M., and Lam, T. H.

Abstract

Family harmony, an important Confucian ideal in Chinese society is believed to determine family happiness and therefore health, but is this accurate? This is a qualitative study of 41 Hong Kong Chinese family members. Individual recorded interviews were thematically analysed describing perceived interactions between harmony, happiness and health. Family harmony comprised four components: communication, mutual respect, lack of conflict and family time [notably "Gou tong" (in Cantonese [?])--opportunity and willingness to spend time together--requiring good interpersonal communication, emphasized by female respondents]. Lack of conflict was emphasized, while diverse values, parenting styles and financial difficulties were common causes of conflict. Respect required reciprocity. Family happiness comprised four elements: family harmony, an important pre-requisite; mutual caring and supportive orientation; sense of security emphasizing financial security in middle-class versus sense of togetherness in lower social class groups and contentment. Healthy families were harmonious; "typical" (children/two-parent/two-grandparent); happy; caring and respectful, with individual health and healthy behaviours. Family harmony, happiness and health are interrelated and built on a communicative, respectful, caring and contented set of attitudes, in particular allowing for family time. Harmony is apparently a core element of good family functioning.

Published
2012
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42. Hong Kong Chinese Community Leaders' Perspectives on Family Health, Happiness and Harmony: A Qualitative Study

Author

Chan, Sophia S. C., Viswanath, K., Au, Doreen W. H., Ma, C. M. S., Lam, W. W. T., Fielding, R., Leung, G. M., and Lam, Tai-Hing

Abstract

This paper examines the views of Hong Kong community leaders on the underlying issues that affect family health, happiness and harmony (3Hs) in Hong Kong. Using a community reconnaissance method, a series of individual in-depth interviews with 26 leaders that represent neighbourhoods of diverse socio-economic status (SES) from June to August 2008 were conducted. Participants considered that changing family structure, economic situation and strong work ethic are the most salient factors that affect family 3Hs. The deprived comprehensive social security assistance recipients, single-parent families and migrant women were considered to be the most vulnerable groups to breakdown in family 3Hs and particularly, they lack family resources. Families from different SES have to overcome different challenges in order to achieve and sustain family 3Hs. Leaders from low SES neighbourhood were concerned more about providing tangible help such as child care facilities to improve family resources, whereas leaders from high SES neighbourhood focused more on preventive interventions such as education on relationship skills to achieve better family well-being. The findings offer insights in designing effective social marketing education campaigns and family-friendly workplace policy to promote social harmony through the maintenance of 3Hs families.

Published
2011
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45. A Screen for Identifying Maladaptive Internet Use

Author

Chow, Siu L., Leung, G. M., and Ng, Cecilia

Abstract

A screening tool (in Chinese) for maladaptive internet use was developed in two stages. Thirty-five factors were first extracted from data obtained from 378 adolescents with a 179-item questionnaire. Nine higher-order factors were then obtained from 35 factors. A 26-item screen that measures both endogenous and exogenous factors was constructed on the basis of the nine higher-order factors. The screen's split-half validity and concurrent criterion-related validity were ascertained with a new sample of 3,523 adolescents. The screen may be used to classify adolescent internet-users into four categories. Its endogenous part may be used to identify potential problem internet users.

Published
2009
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48. Infectivity, Transmission, and Pathology of Human-Isolated H7N9 Influenza Virus in Ferrets and Pigs

Author

Zhu, H., Wang, D., Kelvin, D. J., Li, L., Zheng, Z., Yoon, S.-W., Wong, S.-S., Farooqui, A., Wang, J., Banner, D., Chen, R., Zheng, R., Zhou, J., Zhang, Y., Hong, W., Dong, W., Cai, Q., Roehrl, M. H. A., Huang, S. S. H., Kelvin, A. A., Yao, T., Zhou, B., Chen, X., Leung, G. M., Poon, L. L. M., Webster, R. G., Webby, R. J., Peiris, J. S. M., Guan, Y., and Shu, Y.

Published
2013
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49. The value of values in climate science

Author

Pulkkinen, Karoliina, Undorf, S., Bender, F., Wikman-Svahn, Per, Doblas-Reyes, F., Flynn, C., Hegerl, G. C., Jönsson, A., Leung, G. -K, Roussos, J., Shepherd, T. G., Thompson, E., Pulkkinen, Karoliina, Undorf, S., Bender, F., Wikman-Svahn, Per, Doblas-Reyes, F., Flynn, C., Hegerl, G. C., Jönsson, A., Leung, G. -K, Roussos, J., Shepherd, T. G., and Thompson, E.

Abstract

QC 20220919

Published
2022
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