Intravitreal ranibizumab for age-related macular degeneration : optical coherence tomography guided retreatment intervals and their intra- and inter-individual variability

Purpose: To determine whether the need for retreatment after an initial phase of 3 monthly intravitreal injections of ranibizumab shows an intra-individual regular rhythm and to what degree it varies between different patients. Methods: Prospective study with 42 patients with exudative AMD, treatment naïve. Loading dose of 3 monthly doses of ranibizumab (0,5 mg), followed by a 12 months pro re nata (PRN) regimen according to early exudative signs on HD-OCT Cirrus, Zeiss. The follow-up visits were intensified (week 4, 5, 6, 7, 8, 10, 12, 14, 16, 20, etc after each injection) in order to detect recurrences early, and injection followed within 3 days in cases of subretinal fluid, cysts, or central thickness increase of>50microns. Intervals were calculated between injections for the 12 month follow-up with PRN treatment. Variability was expressed as standard deviation (SD). Results: Visual acuity (VA) improved from a mean ETDRS score of 61.6 (SD 10.8) at baseline to 68.0 (SD 10.2) at month 3 and to 74.7(SD 9.0) at month 12. The 15 patients who have already completed the study showed maintenance of the VA improvement. Central foveal thickness improved from a mean value of 366 microns (baseline) to 253 microns (month 3), well maintained thereafter. Mean number of injections was 8.8 (SD 3.5,range 0-12) per 12 months of follow-up (after 3 doses), with mean individual treatment-recurrence (TR) intervals ranging from 28->365 days (mean 58). Intraindividual variability of TR intervals (SD) was 7.1 days as a mean value (range 1.7¡V22.6). It ranged within 20% of the mean intra-individual interval for 30 (91%) and within 15% for 21 patients (64%). The first interval was within 1 week of the mean intra-individual interval in 64% and within 2 weeks in 89% of patients. Conclusions: The majority of AMD patients showed a relatively stable rhythm for PRN injections of ranibizumab after initial loading phase, associated with excellent functional/anatomical results. The initial interval last loading dose-first recurrence may have a predictive value for further need of treatment, potentially facilitating follow-up and patient care.

Intravitreal ranibizumab for age-related macular degeneration - optical coherence tomography guided retreatment intervals and their intra- and inter-individual variability

PURPOSE:To determine whether the need for retreatment after an initial loading phase of 3 monthly intravitreal injections of ranibizumab shows an intra-individual regular rhythm and to what degree it varies between different patients.SETTING:Prospective mono-centre cohort study.METHODS:Prospective study with 42 patients with exudative age-related macular degeneration (AMD), treatment na?ve, giving informed consent. Loading dose of 3 monthly doses of ranibizumab (0,5mg), followed by a 12 months pro re nata (PRN) regimen according to early exudative signs on spectral domain optical coherence tomography (HD-OCT Cirrus Zeiss?, cube 512x126). The follow-up visits were intensified (week 4, 5, 6, 7, 8, 10, 12, 14, 16, 20, 24, etc after each injection) in order to detect exudative recurrences early, and injection followed within 3 days in cases of subretinal fluid, or intraretinal cysts, or central thickness increase of >50?m. Intervals were calculated between injections and the following recurrence was calculated for the 12 month follow-up with PRN treatment. Variability was expressed as standard deviation (SD). RESULTS Visual acuity (VA) improved from a mean ETDRS letter score of 61.6 (SD 10.8) at baseline to 68.0 (SD 10.2, +6.4 letters) at month 3 and increased further to 74.7 (SD 9.0, +13.1 letters from baseline) at month 12. The 15 patients who have completed the study by October 2010 showed maintenance of the VA improvement. Retinal thickness of the central foveal subfield improved from a mean value of 366?m(baseline) to 253?m(month 3), well maintained thereafter. Mean number of injections was 8.8 (SD 3.5) per 12 months of follow-up (after 3 loading doses), ranging from 0 to 12, with mean individual treatment-recurrence intervals ranging from 28 to >365 days (mean 58 days). Intraindividual variability of treatment-recurrence intervals, measured as SD of the individual intervals, was 7.1days as a mean value(range 1.7 ? 22.6 days) for the 33 patients with more than 1 injection during follow-up. SD was higher for longer intervals of an individual patient. It ranged within 20% of the mean intra-individual interval for 30 patients(91%) and within 15% for 21 patients(64%). The first interval was within 1 week of the mean intra-individual interval in 64% of patients and within 2 weeks in 89% of patients.CONCLUSIONS:The majority of AMD patients showed a relatively stable rhythm for PRN injections of intravitreal ranibizumab after initial loading phase, associated with excellent functional and anatomical results. The initial interval between last loading dose and first recurrence may have a predictive value for further need of treatment, therefore potentially facilitating follow-up and patient care.

Comparación de grosor macular y grado de miopía en grupo de pacientes de la Fundación Oftalmológica Nacional

OBJETIVOS: Comparar las medidas de grosor macular, medido por HD-OCT Cirrus®, en pacientes de la Fundación Oftalmológica Nacional con miopía baja y alta. MÉTODOS: Estudio transversal analítico, en el que se incluyeron pacientes con miopía alta, definida como defecto esférico mayor a – 6.0 dioptrías (D), y pacientes con miopía baja, definida como defecto esférico entre -1.00 D y -6.00 D; a los que se le realizó mapa de grosores maculares con el HD-OCT Cirrus®, y se compararon las medias de los grosores (1, 3 y 6 mm). RESULTADOS: Un total de 128 ojos de pacientes entre 12 y 80 años fueron incluidos; 64 ojos en grupo de miopes bajos y 64 ojos en grupo de miopes altos. La media de edad fue: 37.3 y 38.4 años, y el defecto esférico promedio fue de 2.2 D y 11.5 D, respectivamente. El promedio de grosores en mácula interna (319.9 vs. 307.87 micras, P=0.002), y mácula externa (276.08 vs. 270.23 micras, P=0.047) fue significativamente mayor en el grupo de miopía baja que en el de miopía alta. Sin embargo la media del grosor macular central (1 mm) no tuvo diferencia (261.25 vs. 262 micras P=0.891). CONCLUSIÓN: Este estudio muestra que el grosor macular de 3 y 6 mm centrales es más delgado en miopes altos, pero en 1 mm central es similar que en miopes bajos. En los pacientes estudiados no se encontró diferencia en grosores maculares según género o subgrupos de edad.

Effect of Disease Severity on the Performance of Cirrus Spectral-Domain OCT for Glaucoma Diagnosis

PURPOSE. To evaluate the effect of disease severity on the diagnostic accuracy of the Cirrus Optical Coherence Tomograph (Cirrus HD-OCT; Carl Zeiss Meditec, Inc., Dublin, CA) for glaucoma detection. METHODS. One hundred thirty-five glaucomatous eyes of 99 patients and 79 normal eyes of 47 control subjects were recruited from the longitudinal Diagnostic Innovations in Glaucoma Study (DIGS). The severity of the disease was graded based on the visual field index (VFI) from standard automated perimetry. Imaging of the retinal nerve fiber layer (RNFL) was obtained using the optic disc cube protocol available on the Cirrus HD-OCT. Pooled receiver operating characteristic (ROC) curves were initially obtained for each parameter of the Cirrus HD-OCT. The effect of disease severity on diagnostic performance was evaluated by fitting an ROC regression model, with VFI used as a covariate, and calculating the area under the ROC curve (AUCs) for different levels of disease severity. RESULTS. The largest pooled AUCs were for average thickness (0.892), inferior quadrant thickness (0.881), and superior quadrant thickness (0.874). Disease severity had a significant influence on the detection of glaucoma. For the average RNFL thickness parameter, AUCs were 0.962, 0.932, 0.886, and 0.822 for VFIs of 70%, 80%, 90%, and 100%, respectively. CONCLUSIONS. Disease severity had a significant effect on the diagnostic performance of the Cirrus HD-OCT and thus should be considered when interpreting results from this device and when considering the potential applications of this instrument for diagnosing glaucoma in the various clinical settings. (Invest Ophthalmol Vis Sci. 2010;51:4104-4109) DOI:10.1167/iovs.094716

Sensitivity and specificity of machine learning classifiers for glaucoma diagnosis using Spectral Domain OCT and standard automated perimetry

PURPOSE: To evaluate the sensitivity and specificity of machine learning classifiers (MLCs) for glaucoma diagnosis using Spectral Domain OCT (SD-OCT) and standard automated perimetry (SAP). METHODS: Observational cross-sectional study. Sixty two glaucoma patients and 48 healthy individuals were included. All patients underwent a complete ophthalmologic examination, achromatic standard automated perimetry (SAP) and retinal nerve fiber layer (RNFL) imaging with SD-OCT (Cirrus HD-OCT; Carl Zeiss Meditec Inc., Dublin, California). Receiver operating characteristic (ROC) curves were obtained for all SD-OCT parameters and global indices of SAP. Subsequently, the following MLCs were tested using parameters from the SD-OCT and SAP: Bagging (BAG), Naive-Bayes (NB), Multilayer Perceptron (MLP), Radial Basis Function (RBF), Random Forest (RAN), Ensemble Selection (ENS), Classification Tree (CTREE), Ada Boost M1(ADA),Support Vector Machine Linear (SVML) and Support Vector Machine Gaussian (SVMG). Areas under the receiver operating characteristic curves (aROC) obtained for isolated SAP and OCT parameters were compared with MLCs using OCT+SAP data. RESULTS: Combining OCT and SAP data, MLCs' aROCs varied from 0.777(CTREE) to 0.946 (RAN).The best OCT+SAP aROC obtained with RAN (0.946) was significantly larger the best single OCT parameter (p<0.05), but was not significantly different from the aROC obtained with the best single SAP parameter (p=0.19). CONCLUSION: Machine learning classifiers trained on OCT and SAP data can successfully discriminate between healthy and glaucomatous eyes. The combination of OCT and SAP measurements improved the diagnostic accuracy compared with OCT data alone.

The impact of topical prostaglandin analogs on the biomechanical properties of the cornea in patients with open angle glaucoma

Justification: Le glaucome entraîne une perte progressive de la vision causée par la détérioration du nerf optique. Le glaucome est répandu dans le monde et cause la cécité dans environ sept millions de personnes. Le glaucome touche plus de 400 000 Canadiens et sa prévalence augmente avec le vieillissement de la population.1,2 Il s'agit d'une maladie chronique surnoise dont les symptômes se manifestent uniquement lors des stades avancés et qui peuvent mener à la cécité. Présentement, le seul moyen possible d’arrêter la progression du glaucome au stade initial est de diminuer la pression intra-oculaire (PIO). Les analogues de prostaglandines (APG) topiques sont fréquemment utilisées comme traitement de première ligne. Cependant, la recherche démontre que cette classe de médicaments peut changer certaines propriétés de la cornée, et possiblement influencer la mesure de la PIO.3 Objectif: À déterminer si l'utilisation d'APG affecte les propriétés biomécaniques de la cornée. La conclusion sera basée sur l'analyse intégrée des résultats obtenus de l'analyseur Reichert oculaire Réponse (ORA), la tonométrie par applanation de Goldmann (TAG) et la pachymétrie ultrasonographique. Le deuxième objectif potentiel de cette étude est de déterminer la corrélation, le cas échéant, entre les propriétés biomécaniques de la cornée, l'épaisseur de la cornée centrale (ECC) et la PIO chez les patients subissant un traitement d’APG topique. L'hypothèse principale de cette étude est que l’APG influence les propriétés de la cornée telles que l'épaisseur centrale, l'élasticité et la résistance. Patients et méthodes : Soixante-dix yeux de 35 patients, âgés de 50-85 ans, atteints de glaucome à angle ouvert (GAO) et traités avec APG topique ont été examinés. Seulement les sujets avec une réfraction manifeste entre -6,00 D et +4,25 D ont été inclus. Les critères d'exclusion sont: patients avec n'importe quelle autre maladie de la cornée de l’œil, telles que la dystrophie endothéliale de Fuch’s et kératocône, ou tout antécédent de traumatisme ou d'une chirurgie de la cornée, ainsi que le port de lentilles de contact. Nous avons demandé aux patients atteints du glaucome qui ont des paramètres stables et qui utilisent l’APG dans les deux yeux de cesser l’APG dans l'œil moins affecté par la PIO, et de continuer l’utilisation d’APG dans l'œil contralatéral. Le meilleur œil est défini comme celui avec moins de dommage sur le champ visuel (CV) (déviation moyenne (DM), le moins négatif) ou une PIO maximale historique plus basse si la DM est égale ou encore celui avec plus de dommage sur la tomographie par cohérence optique (TCO, Cirrus, CA) ou la tomographie confocale par balayage laser (HRT, Heidelberg, Allemagne). Toutes les mesures ont été prises avant la cessation d’APG et répétées 6 semaines après l’arrêt. Les patients ont ensuite recommencé l’utilisation d’APG et toutes les mesures ont été répétées encore une fois après une période supplémentaire de 6 semaines. Après commencer ou de changer le traitement du glaucome, le patient doit être vu environ 4-6 semaines plus tard pour évaluer l'efficacité de la goutte.4 Pour cette raison, on été décidé d'utiliser 6 semaines d'intervalle. Toutes les mesures ont été effectuées à l’institut du glaucome de Montréal par le même technicien, avec le même équipement et à la même heure de la journée. L'œil contralatéral a servi comme œil contrôle pour les analyses statistiques. La tonométrie par applanation de Goldmann a été utilisée pour mesurer la PIO, la pachymétrie ultrasonographique pour mesurer l'ECC, et l’ORA pour mesurer les propriétés biomécaniques de la cornée, incluant l'hystérèse cornéenne (HC). L’hypothèse de l'absence d'effet de l'arrêt de l’APG sur les propriétés biomécaniques a été examiné par un modèle linéaire à effets mixtes en utilisant le logiciel statistique R. Les effets aléatoires ont été définies à deux niveaux: le patient (niveau 1) et l'œil de chaque patient (niveau 2). Les effets aléatoires ont été ajoutés au modèle pour tenir compte de la variance intra-individuelle. L’âge a également été inclus dans le modèle comme variable. Les contrastes entre les yeux et les temps ont été estimés en utilisant les valeurs p ajustées pour contrôler les taux d'erreur internes de la famille en utilisant multcomp paquet dans R. Résultats: Une augmentation statistiquement significative due l 'HC a été trouvée entre les visites 1 (sur APG) et 2 (aucun APG) dans les yeux de l'étude, avec une moyenne (±erreur standard) des valeurs de 8,98 ± 0,29 mmHg et 10,35 ± 0,29 mmHg, respectivement, correspondant à une augmentation moyenne de 1,37 ± 0,18 mmHg (p <0,001). Une réduction significative de 1,25 ± 0,18 mmHg (p <0,001) a été observée entre les visites 2 et 3, avec une valeur moyenne HC finale de 9,09 ± 0,29 mmHg. En outre, une différence statistiquement significative entre l’oeil d’étude et le contrôle n'a été observée que lors de la visite 2 (1,01 ± 0,23 mmHg, p <0,001) et non lors des visites 1 et 3. Une augmentation statistiquement significative du facteur de résistance conréen (FRC) a été trouvée entre les visites 1 et 2 dans les yeux de l'étude, avec des valeurs moyennes de 10,23 ± 0,34 mmHg et 11,71 ± 0,34 mmHg, respectivement. Le FRC a ensuite été réduit de 1,90 ± 0,21 mmHg (p <0,001) entre les visites 2 et 3, avec une valeur moyenne FRC finale de 9,81 ± 0,34 mmHg. Une différence statistiquement significative entre l’oeil d’étude et le contrôle n'a été observée que lors de la visite 2 (1,46 ± 0,23 mmHg, p <0,001). Une augmentation statistiquement significative de l'ECC a été trouvée entre les visites 1 et 2 dans les yeux de l'étude, avec des valeurs moyennes de 541,83 ± 7,27 µm et 551,91 ± 7,27 µm, respectivement, ce qui correspond à une augmentation moyenne de 10,09 ± 0,94 µm (p <0,001). L'ECC a ensuite diminué de 9,40 ± 0,94 µm (p <0,001) entre les visites 2 et 3, avec une valeur moyenne finale de 542,51 ± 7,27 µm. Une différence entre l’étude et le contrôle des yeux n'a été enregistré que lors de la visite 2 (11,26 ± 1,79 µm, p <0,001). De même, on a observé une augmentation significative de la PIO entre les visites 1 et 2 dans les yeux de l'étude, avec des valeurs moyennes de 15,37 ± 0,54 mmHg et 18,37 ± 0,54 mmHg, respectivement, ce qui correspond à une augmentation moyenne de 3,0 ± 0,49 mmHg (p <0,001). Une réduction significative de 2,83 ± 0,49 mmHg (p <0,001) a été observée entre les visites 2 et 3, avec une valeur moyenne de la PIO finale de 15,54 ± 0,54 mmHg. L’oeil de contrôle et d’étude ne différaient que lors de la visite 2 (1,91 ± 0,49 mmHg, p <0,001), ce qui confirme l'efficacité du traitement de l’APG. Lors de la visite 1, le biais de la PIO (PIOcc - PIO Goldmann) était similaire dans les deux groupes avec des valeurs moyennes de 4,1 ± 0,54 mmHg dans les yeux de contrôles et de 4,8 ± 0,54 mmHg dans les yeux d’études. Lors de la visite 2, après un lavage de 6 semaines d’APG, le biais de la PIO dans l'œil testé a été réduit à 1,6 ± 0,54 mmHg (p <0,001), ce qui signifie que la sous-estimation de la PIO par TAG était significativement moins dans la visite 2 que de la visite 1. La différence en biais PIO moyenne entre l'étude et le contrôle des yeux lors de la visite 2, en revanche, n'a pas atteint la signification statistique (p = 0,124). On a observé une augmentation peu significative de 1,53 ± 0,60 mmHg (p = 0,055) entre les visites 2 et 3 dans les yeux de l'étude, avec une valeur de polarisation finale de la PIO moyenne de 3,10 ± 0,54 mmHg dans les yeux d'études et de 2,8 ± 0,54 mmHg dans les yeux de contrôles. Nous avons ensuite cherché à déterminer si une faible HC a été associée à un stade de glaucome plus avancé chez nos patients atteints du glaucome à angle ouvert traités avec l’APG. Lorsque l'on considère tous les yeux sur l’APG au moment de la première visite, aucune association n'a été trouvée entre les dommages sur le CV et l'HC. Cependant, si l'on considère seulement les yeux avec un glaucome plus avancé, une corrélation positive significative a été observée entre la DM et l'HC (B = 0,65, p = 0,003). Une HC inférieure a été associé à une valeur de DM de champ visuelle plus négative et donc plus de dommages liés au glaucome. Conclusions : Les prostaglandines topiques affectent les propriétés biomécaniques de la cornée. Ils réduisent l'hystérèse cornéenne, le facteur de résistance cornéen et l'épaisseur centrale de la cornée. On doit tenir compte de ces changements lors de l'évaluation des effets d’APG sur la PIO. Plus de recherche devrait être menées pour confirmer nos résultats. De plus, d’autres études pourraient être réalisées en utilisant des médicaments qui diminuent la PIO sans influencer les propriétés biomécaniques de la cornée ou à l'aide de tonomètre dynamique de Pascal ou similaire qui ne dépend pas des propriétés biomécaniques de la cornée. En ce qui concerne l'interaction entre les dommages de glaucome et l'hystérésis de la cornée, nous pouvons conclure qu' une HC inférieure a été associé à une valeur de DM de CV plus négative. Mots Clés glaucome - analogues de prostaglandines - hystérèse cornéenne – l’épaisseur de la cornée centrale - la pression intraoculaire - propriétés biomécaniques de la cornée.

Cambios maculares y de capa de fibras nerviosas ganglionares posterior a la vitrectomía pars plana y sus factores pronósticos en la fundación oftalmológica nacional

OBJETIVOS: Determinar los factores pronóstico, cambios maculares morfológicos y de capa de fibras nerviosas ganglionares posterior a vitrectomía pars plana, en la Fundación Oftalmológica Nacional. MATERIALES Y MÉTODOS: Estudio longitudinal de antes y después (3y6 meses) de la vitrectomía pars plana (VPP) en pacientes con membrana epirretiniana, agujero macular, síndrome de tracción vítreo macular y opacidades vítreas no-inflamatorias. Se realizó seguimiento clínico y con tomografía de coherencia óptica. RESULTADOS: Grupo de 60 pacientes (mujeres 65.0%), edad promedio 65.45+9.49años y tiempo de enfermedad promedio 23+29.79meses. Las indicaciones de VPP (n=60ojos) fueron agujero macular (38.3%) y membrana epirretiniana (36.7%). Se encontró diferencia significativa entre grosor del complejo capa de células ganglionares (CCG)+capa plexiforme interna (CPI) inicial y 3 meses (p=0.039), correlación entre grosor del complejo CCG+CPI al tercer y sexto mes (r=0.704,p<0.001) y grosor del complejo CCG+CPI al tercer mes con grosor foveal central (CFT) al tercer y sexto mes (r=–0.594,p<0.001 y r=–0.595,p=0.001). Mayores de 65años tenían menor grosor de CFNG a 6meses (r=-0.528,p=0.007). El grosor de CFNG promedio y la presencia de la zona elipsoide inicial fueron factores pronósticos de buena agudeza visual al tercer mes de VPP (r2=0.414,p=0.018, y r2=0.414,p=0.010). CONCLUSIÓN: El grosor de CFNG y la presencia de la zona elipsoide inicial tienen alta capacidad predictiva de buena agudeza visual al tercer mes de VPP, y, correlación inversa entre grosor del complejo CCG+CPI con CFT al tercer y sexto mes de VPP.

Corneal Biomechanics, Retinal Nerve Fiber Layer, and Optic Disc in Children

Purpose: To evaluate the possible associations between corneal biomechanical parameters, optic disc morphology, and retinal nerve fiber layer (RNFL) thickness in healthy white Spanish children. Methods: This cross-sectional study included 100 myopic children and 99 emmetropic children as a control group, ranging in age from 6 to 17 years. The Ocular Response Analyzer was used to measure corneal hysteresis (CH) and corneal resistance factor. The optic disc morphology and RNFL thickness were assessed using posterior segment optical coherence tomography (Cirrus HD-OCT). The axial length was measured using an IOLMaster, whereas the central corneal thickness was measured by anterior segment optical coherence tomography (Visante OCT). Results: The mean (±SD) age and spherical equivalent were 12.11 (±2.76) years and −3.32 (±2.32) diopters for the myopic group and 11.88 (±2.97) years and +0.34 (±0.41) diopters for the emmetropic group. In a multivariable mixed-model analysis in myopic children, the average RNFL thickness and rim area correlated positively with CH (p = 0.007 and p = 0.001, respectively), whereas the average cup-to-disc area ratio correlated negatively with CH (p = 0.01). We did not observe correlation between RNFL thickness and axial length (p = 0.05). Corneal resistance factor was only positively correlated with the rim area (p = 0.001). The central corneal thickness did not correlate with the optic nerve parameters or with RNFL thickness. These associations were not found in the emmetropic group (p > 0.05 for all). Conclusions: The corneal biomechanics characterized with the Ocular Response Analyzer system are correlated with the optic disc profile and RNFL thickness in myopic children. Low CH values may indicate a reduction in the viscous dampening properties of the cornea and the sclera, especially in myopic children.

Avaliação da reprodutibilidade das medidas da camada de fibras nervosas retiniana e da cabeça do nervo óptico pela tomografia de coerência óptica

OBJETIVO: Determinar a reprodutibilidade da espessura da camada de fibras nervosas da retina peripapilar e dos parâmetros da cabeça do nervo óptico em olhos normais, utilizando a tomografia de coerência óptica de domínio espectral (SD-OCT). MÉTODOS: Trinta e quatro olhos de 34 indivíduos saudáveis foram incluídos no estudo. O protocolo do cubo do disco óptico 200x200 do OCT Cirrus foi utilizado para gerar 3 imagens de cada olho para avaliar a reprodutibilidade. O coeficiente de correlação intraclasse (ICC) foi calculado para as medidas da espessura da camada de fibras nervosas da retina e da cabeça do nervo óptico. RESULTADOS: A correlação foi excelente para todas as medidas da espessura da camada de fibras nervosas da retina (ICC entre 0,87 e 0,98). O mesmo ocorreu com os parâmetros da cabeça do nervo óptico que, com exceção da razão E/D vertical (ICC 0,56), apresentou ICC entre 0,83 e 0,99. CONCLUSÃO: As medidas de espessura da camada de fibras nervosas da retina peripapilar e os parâmetros da cabeça no nervo óptico demonstraram uma excelente reprodutibilidade com o OCT Cirrus, indicando que este aparelho poderá ser uma ferramenta útil no estudo do glaucoma. Este estudo apresenta algumas limitações, como o pequeno número de casos avaliados, sendo necessários maiores estudos para corroborar nossos achados.

Comparison of central macular thickness (CMT) measurement between time domain and spectral domain (SD) optical coherence tomography (OCT) and reproducibility of SD OCT in active neovascular AMD

Purpose: To evaluate the reproducibility of Cirrus-SD OCT measurements and to compare central macular thickness (CMT) measurements between TD-Stratus and SD-Cirrus OCT in patients with active exudative AMD. Methods: Consecutive case series of patients with active exudative AMD seen in the Medical Retina Department. Patients underwent 1 scan with Stratus (macular thickness map protocol) and 5 scans with Cirrus (Macular Cube protocol) at the same visit by the same experienced examiner. To be included, patients best-corrected visual acuity (BCVA) had to be >20/200 while all scans had to be of sufficient quality, well-centered and at least one Cirrus scan with CMT >300 microns. The repeatability of the SD Cirrus was estimated by using all 5 CMT measurements and the mean of the Cirrus measurements was compared with the CMT obtained by TD Stratus. Results: Cirrus OCT demonstrated high intraobserver repeatability at the central foveal region (ICC 96%). The mean of the CMT measurements was 321microns for Stratus and 387 microns for Cirrus. The average difference was 65m (SD=30). The coefficient of concordance between Stratus and Cirrus CMT measurements was rho=0,749 with a high precision and a moderate accuracy. The equation of the line of regression between Stratus and meanCirrus is given by the following: M_stratus = 0,848 x m_cirrus - 4,496 (1).Conclusions: The Cirrus macular cube protocol allows reproducible CMT measurements in patients with active exudative AMD. In cases of upgrading from TD to SD use and vice versa, there is the possibility to predict the measurements by using the equation (1). These real life data and conclusions can help in improving our clinical management of patients with neovascular AMD.

Structure-function Relationships Using the Cirrus Spectral Domain Optical Coherence Tomograph and Standard Automated Perimetry

Purpose: To evaluate the relationship between glaucomatous structural damage assessed by the Cirrus Spectral Domain OCT (SDOCT) and functional loss as measured by standard automated perimetry (SAP). Methods: Four hundred twenty-two eyes (78 healthy, 210 suspects, 134 glaucomatous) of 250 patients were recruited from the longitudinal Diagnostic Innovations in Glaucoma Study and from the African Descent and Glaucoma Evaluation Study. All eyes underwent testing with the Cirrus SDOCT and SAP within a 6-month period. The relationship between parapapillary retinal nerve fiber layer thickness (RNFL) sectors and corresponding topographic SAP locations was evaluated using locally weighted scatterplot smoothing and regression analysis. SAP sensitivity values were evaluated using both linear as well as logarithmic scales. We also tested the fit of a model (Hood) for structure-function relationship in glaucoma. Results: Structure was significantly related to function for all but the nasal thickness sector. The relationship was strongest for superotemporal RNFL thickness and inferonasal sensitivity (R(2) = 0.314, P < 0.001). The Hood model fitted the data relatively well with 88% of the eyes inside the 95% confidence interval predicted by the model. Conclusions: RNFL thinning measured by the Cirrus SDOCT was associated with correspondent visual field loss in glaucoma.

Effects Of Misalignments In The Retinal Nerve Fiber Layer Thickness Measurements With Spectral Domain Optical Coherence Tomography.

Purpose. To investigate misalignments (MAs) on retinal nerve fiber layer thickness (RNFLT) measurements obtained with Cirrus(©) SD-OCT. Methods. This was a retrospective, observational, cross-sectional study. Twenty-seven healthy and 29 glaucomatous eyes of 56 individuals with one normal exam and another showing MA were included. MAs were defined as an improper alignment of vertical vessels in the en face image. MAs were classified in complete MA (CMA) and partial MA (PMA), according to their site: 1 (superior, outside the measurement ring (MR)), 2 (superior, within MR), 3 (inferior, within MR), and 4 (inferior, outside MR). We compared RNFLT measurements of aligned versus misaligned exams in all 4 sectors, in the superior area (sectors 1 + 2), inferior area (sectors 3 + 4), and within the measurement ring (sectors 2 + 3). Results. RNFLT measurements at 12 clock-hour of eyes with MAs in the superior area (sectors 1 + 2) were significantly lower than those obtained in the same eyes without MAs (P = 0.043). No significant difference was found in other areas (sectors 1 + 2 + 3 + 4, sectors 3 + 4, and sectors 2 + 3). Conclusion. SD-OCT scans with superior MAs may present lower superior RNFLT measurements compared to aligned exams.

The qWR star HD 45166 - II. Fundamental stellar parameters and evidence of a latitude-dependent wind

Context. The enigmatic object HD 45166 is a qWR star in a binary system with an orbital period of 1.596 day, and presents a rich emission-line spectrum in addition to absorption lines from the companion star (B7 V). As the system inclination is very small (i = 0.77 degrees +/- 0.09 degrees), HD 45166 is an ideal laboratory for wind-structure studies. Aims. The goal of the present paper is to determine the fundamental stellar and wind parameters of the qWR star. Methods. A radiative transfer model for the wind and photosphere of the qWR star was calculated using the non-LTE code CMFGEN. The wind asymmetry was also analyzed using a recently-developed version of CMFGEN to compute the emerging spectrum in two-dimensional geometry. The temporal-variance spectrum (TVS) was calculated to study the line-profile variations. Results. Abundances and stellar and wind parameters of the qWR star were obtained. The qWR star has an effective temperature of T(eff) = 50 000 +/- 2000 K, a luminosity of log(L/L(circle dot)) = 3.75 +/- 0.08, and a corresponding photospheric radius of R(phot) = 1.00 R(circle dot). The star is helium-rich (N(H)/N(He) = 2.0), while the CNO abundances are anomalous when compared either to solar values, to planetary nebulae, or to WR stars. The mass-loss rate is. M = 2.2 x 10(-7) M(circle dot) yr(-1), and the wind terminal velocity is v(infinity) = 425 km s(-1). The comparison between the observed line profiles and models computed under different latitude-dependent wind densities strongly suggests the presence of an oblate wind density enhancement, with a density contrast of at least 8: 1 from equator to pole. If a high velocity polar wind is present (similar to 1200 km s(-1)), the minimum density contrast is reduced to 4:1. Conclusions. The wind parameters determined are unusual when compared to O-type stars or to typical WR stars. While for WR stars v(infinity)/v(esc) > 1.5, in the case of HD 45166 it is much smaller (v(infinity)/v(esc) = 0.32). In addition, the efficiency of momentum transfer is eta = 0.74, which is at least 4 times smaller than in a typical WR. We find evidence for the presence of a wind compression zone, since the equatorial wind density is significantly higher than the polar wind. The TVS supports the presence of such a latitude-dependent wind and a variable absorption/scattering gas near the equator.

A binary engine fuelling HD 87643's complex circumstellar environment Determined using AMBER/VLTI imaging

Context. The star HD 87643, exhibiting the ""B[e] phenomenon"", has one of the most extreme infrared excesses for this object class. It harbours a large amount of both hot and cold dust, and is surrounded by an extended reflection nebula. Aims. One of our major goals was to investigate the presence of a companion in HD87643. In addition, the presence of close dusty material was tested through a combination of multi-wavelength high spatial resolution observations. Methods. We observed HD 87643 with high spatial resolution techniques, using the near-IR AMBER/VLTI interferometer with baselines ranging from 60 m to 130 m and the mid-IR MIDI/VLTI interferometer with baselines ranging from 25 m to 65 m. These observations are complemented by NACO/VLT adaptive-optics-corrected images in the K and L-bands, and ESO-2.2m optical Wide-Field Imager large-scale images in the B, V and R-bands. Results. We report the direct detection of a companion to HD 87643 by means of image synthesis using the AMBER/VLTI instrument. The presence of the companion is confirmed by the MIDI and NACO data, although with a lower confidence. The companion is separated by similar to 34 mas with a roughly north-south orientation. The period must be large (several tens of years) and hence the orbital parameters are not determined yet. Binarity with high eccentricity might be the key to interpreting the extreme characteristics of this system, namely a dusty circumstellar envelope around the primary, a compact dust nebulosity around the binary system and a complex extended nebula suggesting past violent ejections.

The B0.5 IVe CoRoT target HD 49330 II. Spectroscopic ground-based observations

Context. We present spectroscopic ground-based observations of the early Be star HD 49330 obtained simultaneously with the CoRoT-LRA1 run just before the burst observed in the CoRoT data. Aims. Ground-based spectroscopic observations of the early Be star HD 49330 obtained during the precursor phase and just before the start of an outburst allow us to disantangle stellar and circumstellar contributions and identify modes of stellar pulsations in this rapidly rotating star. Methods. Time series analysis (TSA) is performed on photospheric line profiles of He I and Si III by means of the least squares method. Results. We find two main frequencies f1 = 11.86 c d(-1) and f2 = 16.89 c d(-1) which can be associated with high order p-mode pulsations. We also detect a frequency f3 = 1.51 c d(-1) which can be associated with a low order g-mode. Moreover we show that the stellar line profile variability changed over the spectroscopic run. These results are in agreement with the results of the CoRoT data analysis, as shown in Huat et al. (2009). Conclusions. Our study of mid-and short-term spectroscopic variability allows the identification of p-and g-modes in HD 49330. It also allows us to display changes in the line profile variability before the start of an outburst. This brings new constraints for the seimic modelling of this star.