The irregular galaxy Cassiopeia 1 – a new member of the Local group

A photometry in the V, R, I (Cousins) system has been performed for stars in the galaxy Cassiopeia 1. The resulting colour-agnitude (CM) diagram of Cas 1 reveals the existence of blue stars and the absence of red ones. From an analysis of the CM diagram of the galaxy it is concluded that A_v = 4.0 mag, and the distance modulus (m – M)_o = 24.5 mag, corresponding to a distance of 790 kpc. The visual magnitude of the galaxy is V = 14^m.62 (M_v = −13^m.8) and the colour index (V – R) = 0.89 mag. From the distance determination the galaxy Cassiopeia 1 is a member of the Local group.     

Photographic photometry for stellar statistics with Tautenburg Schmidt telescope

Photometric properties of deep Tautenburg Schmidt plates in the UBV system over the whole field and over a wide range of stellar magnitudes are discussed. Different reduction models based on the calibration curve alone and with additional terms containing colour and plate coordinates are considered. With the filter-emulsion combinations used the Johnson UBV system can be reproduced quite well by the Tautenburg telescope. The accuracy of photometric data can be improved if geometrical terms are taken into account. For deep plates with a significant effect of background nebulosity a supplementary term is to be included in the reduction model. The polynomial coefficients vary in dependence on spectral bands and individual properties of each plate.     

双因素判别分析胃癌组织与正常组织自体荧光光谱

通过对手术切除的37例胃癌患者的离体标本的自体荧光光谱检测,显示308nm,337nm激发光谱均呈双主峰结构,双主峰的比值均能区分胃癌与正常胃壁(P<0.001).分别用308nm,337nm激发荧光光谱单因素分析诊断胃癌的灵敏度、特异度、阳性预测值分别为88.8%,86.8%,86.4%和80.1%,72.1%,67.5%.对308nm及337nm激发荧光光谱双因素分析,癌诊断的灵敏度、特异度、阳性预测值分别为94.4%,92.1%,91.9%,其诊断正确符合率明显高于单因素分析的结果.研究表明,以308nm及337nm双波长激发检测胃壁浆膜,双因素判别算法可较好地区分胃癌,这种方法有望成为手术中快速识别胃癌在胃壁的浸润范围的有效方法.     

高浓度气体共振光声光谱信号饱和特性研究

采用恒流驱动耦合机械斩波技术在激光光声光谱装置上系统测量了5%—100%宽浓度范围甲烷气体的共振光声信号,发现在高浓度区共振光声信号呈现异常的饱和特征.基于气体吸收和光声光谱原理定量分析了光声信号饱和的主要原因及影响因素,研究表明,气体样本对入射光强吸收而导致的声源与本征共振模式的耦合系数改变是异常饱和的主要原因,并导出判定光声信号饱和深度的准则以用于判定高浓度气体饱和深度.     

基于阈值光电子-光离子符合技术的分子离子光谱和解离动力学研究

对电子和离子同时采用速度聚焦电场收集的阈值光电子-光离子符合成像谱仪能够有效提高电子的收集效率和能量分辨率.利用该符合成像谱仪,开展了Xe/Ar/Ne 惰性混合气体及NO 分子的阈值光电子谱、阈值光电子-光离子符合质谱和质量选择的符合光谱等实验研究,精确测量了NO 分子的电离势,并且获得了NO⁺离子振动态分辨的X¹Σ⁺,c³Π和B¹Π态光谱.还进一步研究了NO^{+ 相似文献}   

Coherent spectroscopy of a strongly driven triple quantum dot molecule

Based on a calculation model, we study the interference phenomena of serially coupled V-type and Λ-type triple quantum dots (CTQDs) driven simultaneously by a strong driving field and a weak probe field. Strongly depending on the configuration of the three-level CTQD, the probe absorption spectra, which are shown in the tunneling current, exhibit various quantum coherence properties. In the case where the two pairs of transitions of the CTQD have a small eigenfrequency difference Δω, the double-coupling effect of the driving field results in two Autler-Townes doublets and one weak Mollow triplet in one spectrum. With the value of Δω increasing, only one Autler-Townes splitting remains due to the single-coupling of the field. We also find that the effect of spontaneous emission of phonons may lead to an obvious background current, which can be used to distinguish which transition is driven by the driving field in experiment. The interesting quantum property of a CTQD revealed in our results suggests its potential applications in quantum modulators and quantum logic devices.     

Multivariate analysis of fluorescence and source identification of dissolved organic matter in Jiaozhou Bay, China

Hierarchical clustering analysis and principal component analysis (PCA) methods were used to assess the similarities and dissimilarities of the entire Excitation-emission matrix spectroscopy (EEMs) data sets of samples collected from Jiaozhou Bay, China. The results demonstrate that multivariate analysis facilitates the complex data treatment and spectral sorting processes, and also enhances the probability to reveal otherwise hidden information concerning the chemical characteristics of the dissolved organic matter (DOM). The distribution of different water samples as revealed by multivariate results has been used to track the movement of DOM material in the study area, and the interpretation is supported by the results obtained from the numerical simulation model of substance tracing technique, which show that the substance discharged by Haibo River can be distributed in Jiaozhou Bay.     

兴凯湖沉积物磁化率和色度反映的28kaBP以来区域古气候环境演化

对兴凯湖长269 cm的沉积岩心的研究结果显示:沉积物的色度和磁化率特征可以较好地反映区域气候环境变化。沉积物明度分别与红度、磁化率、黏土和有机质含量之间及磁化率与黏土之间有很好的相关性;红度高值与明度低值对应暖湿气候环境,磁化率低值反映沉积物较粗的较低湖面,对应冷干气候。28480~26160 cal.aBP,湖区处于温湿气候时期;22880~18170 cal.aBP,岩心孢粉浓度很低,流域处于末次盛冰期疏桦林草原环境;18170~12650 cal.aBP处于Bφlling/Older Dryas/Allerφd暖期。岩心深度90~78 cm段,对应于新仙女木期;11500~4570 cal.aBP,进入全新世暖期,其中8000~5000 cal.aBP,本区处于全新世大暖期(气候适宜期);4570~1470 cal.aBP气候变为凉干;1470 cal.aBP以来,流域又变为暖湿气候环境,同时,人类活动逐渐增强造成水土流失加剧。     

Spectroscopic study of the peculiar galaxy UGC 5119

We present the results of our study of the stellar kinematics in the elliptical galaxy UGC 5119, which has previously been suspected to be a polar-ring galaxy. We have detected a rapidly rotating disk in the central region (r ≤ 3.2 kpc) of the galaxy’s main body and found a radial velocity gradient along its minor axis (in the putative ring). We conclude that UGC 5119 is a medium-luminosity elliptical galaxy with a rapidly rotating disk component and a stellar (probably polar) ring. We have calculated the Lick indices of the Hβ, Mggb, Fe 5270, and Fe 5335 absorption lines and compared them with evolutionary synthesis models. Differences in the [Mg/Fe] ratios, metallicities, and ages of the stars have been found: the young stellar population with a solar [Mg/Fe] ratio and a high metallicity dominates in the circumnuclear region (r ≤ 1 kpc), while the old one with a low metal abundance dominates in the ring.     

Fabry-Perot spectroscopy in space science

The paper describes use of Fabry-Perot (fp) systems in spectroscopic studies of astronomy and earth’s upper atmosphere. Factors influencing the resolution, luminosity and instrumental line shape offp spectrometer are discussed and the need for their optimization is emphasised, if desired luminosity gain is to be realised in practice. Use offp as imaging spectrometer, scanning spectrometer and as a narrow band filter are illustrated. Tandemfp systems are briefly dealt with.