PSF-fitting techniques for crowded field 3D spectroscopy

From a historical point of view, it was only through the advent of the CCD as a linear, high dynamic range panoramic detector that it became possible to overcome the source confusion problem for stellar photometry, e.g., in star clusters or nearby galaxies. The ability of accurately sampling the point-spread-function (PSF) in two dimensions and to use it as a template for fitting severely overlapping stellar images is of fundamental importance for crowded-field photometry, and has thus become the foundation for the determination of accurate color-magnitude diagrams of globular clusters and the study of resolved stellar populations in nearby galaxies. Analogous to CCDs, the introduction of integral field spectrographs has opened a new avenue for crowded-field 3D spectroscopy, which benefits in the same way from PSF-fitting techniques as CCD photometry does. This paper presents first experience with sampling the PSF in 3D spectroscopy, reviews the effects of atmospheric refraction, discusses background subtraction problems, and presents several science applications as obtained from observations with the PMAS instrument at Calar Alto Observatory.     

荧光分光光度法测定海洋生物中的谷胱甘肽

对应用荧光分光光度法测定海洋生物中还原型谷胱甘肽(GSH)含量的方法进行了研究,并测定了分属于鱼、虾、贝、藻的10种海洋生物中谷胱甘肽的含量。利用邻苯二甲醛与GSH反应构成的荧光体系,在激发波长为365nm,发射波长为425nm的条件下,方法的回收率为99.22%~99.69%,变异系数为2.16%。应用此方法测得10种海洋生物中谷胱甘肽的含量为:红笛鲷(Lutjanussanguineus)0.399mg/g,银鲳(Pampusargenteus)0.352mg/g,大海鲢(Megalopscyrinoides)0.561mg/g,尖紫蛤(Sanguinolariaacuta)0.289mg/g,菲律宾蛤仔(Ruditapesphilippinarun)0.287mg/g,墨吉对虾(Penaeusmerguiensis)0.892mg/g,凡纳滨对虾(Litopenaeusvannamei)1.434mg/g,囊藻(Colpomeniasinu-ose)0.221mg/g,石莼(Ulvalactucal)0.727mg/g,马尾藻(Sargassummuticum)0.137mg/g。     

1–100 μm energy spectra and 2.3–4 μm spectrophotometry of MSC stars

The JHKL' photometry and 2.3–4 μm spectrophotometry of some M giants, S type stars and carbon stars are presented in this paper. It is found that in combination with IRAS data, the energy spectra in 1–100 μm of S type stars are intermediate between those of M giants and carbon stars, which are obviously different. The spectrophotometry in the near infrared shows that, besides carbon stars, which have HCN and C₂H₂ strong absorptions at 3.1 μm, some S type stars have the similar but weaker absorption in the same spectral region. However, no trace of any absorption at 3.1 μm can be seen in M giants. These results probably provide more evidence for the M-S-C sequence in the late stage of stellar evolution.     

氢化物原子荧光光度法测定地球化学样品中的微量铅

拟定了用铅空心阴极灯为激发光源,氢化物原子荧光光度法测定地球化学样品中微量铅的方法。在2％HCl-0.08％K_3[Fe(CN)_6]-2％KBH_4体系中,铅的测定灵敏度有明显地提高。该方法操作简便、快速、准确,检出限为8.89×10~(-9)g/ml,精密度为4.12％(n=11)。     

Spectral and Photoelectric Studies of the Herbig Ae/Be Star HD 259431

Spectral and photoelectric (ubvy, H, H) observations of the Herbig Ae/Be star HD 259431 are reported. It is found that as its brightness fades, this star becomes bluer in the Paschen continuum and the intensity and equivalent width of the hydrogen emission lines increase. The spectral observations reveal significant variations in the intensity of the Mg II 4481 Å photospheric absorption line. A rise and fall in the luminosity by 0^m.04 within a period of 5-7 minutes was recorded. Radical variations in the H lineshape ("double" "P Cyg") and flare activity are not only observed in this star, but also in a number of HAEBE stars. It is suggested that flare activity may initiate a change in the velocity gradient at the base of the wind and, thereby, induce "double P Cyg" or "P Cyg single" transitions. The nonradial pulsations of this star are also discussed.     

原子吸收分光光度法快速测定铬铁矿中钙、镁、锰

通过在标液中加入相应的Sr来消除离子干扰,采用原子吸收分光光度法快速测定CaO、MgO、MnO的含量,方法经国家标准物质验证,其RSD<2%(n=6)。其结果与标准值相符。方法达到了准确、简便、快速、实用性强。     

对磺基苯偶氮变色酸分光光度法测定岩石样品中的氟

采用对磺基苯偶氮变色酸分光光度法对岩石样品中氟的含量进行测定。确定的最佳测定条件为:测定波长570 nm,放置2 h后测定,盐酸介质浓度0.84 mol/L,显色剂用量5.0 mL。氟离子浓度在0~1.4 mg/L时符合比尔定律,方法检出限为0.06μg/g。以岩石标准物质代替氟标准溶液制作标准曲线,可有效降低杂质元素的干扰。对国家一级标准物质和日本玄武岩标准物质6次测定的相对标准偏差(RSD)为2.37%~6.32%。     

钛磁铁矿的制备及其异相Fenton反应催化性能

在水相中合成了钛磁铁矿（Fe3-xTixO4）,并用XRD、MSssbauer、TG-DSC和SEM等手段对合成的Fe3-xTixO4进行了表征。结果表明,合成的Fe3-xTixO4为立方晶系尖晶石结构,样品中的钛离子都已经进入其晶格中;钛掺杂有抑制钛磁铁矿进一步向钛磁赤铁矿转化和稳定尖晶石结构的作用。此外,以亚甲基蓝降解为探针反应,考察了钛磁铁矿异相Fenton反应的催化性能。实验表明,钛含量较高的钛磁铁矿是一种性能优越的异相Fenton反应催化剂。     

爱沙尼亚干酪根催化降解生烃过程及动力学研究

以爱沙尼亚油页岩干酪根为对象,利用热模拟实验方法和化工催化原理,考察了不同介质对干酪根热解生烃过程的影响,从热解生烃量、生烃组成特征及生烃动力学等方面进行了探讨。结果表明:膏岩对干酪根的生烃具有明显催化作用,碳酸盐岩对干酪根的生烃具有一定反催化作用,各种盐类对干酪根的生烃量影响较小。干酪根热解动力学研究表明,生烃动力学参数表观活化能E与视频率因子A两者之间不是独立变化的,而是具有一定的关系,即:E与lnA之间服从直线关系(R=0.99),这些认识对于深入探讨爱沙尼亚油页岩干酪根的化学结构、建立热解动力学模型具有一定的参考价值。     

溴邻苯三酚红-丁基罗丹明B高灵敏分光光度法测定微量钛的研究

在乳化剂ＯＰ和聚乙烯醇ＰＶＡ－１２４存在下,于０．０２ｍｏｌ／ＬＨ２ＳＯ４介质中,Ｔｉ（Ⅳ）与溴邻苯三酚红（ＢＰＲ）和丁基罗丹明Ｂ（ＢＲＢ）产生高灵敏协同显色反应。配合物λｍａｘ＝５９６ｎｍ,ε为１．５０×１０５Ｌ·ｍｏｌ－１·ｃｍ－１,钛的质量浓度在０～４８０μｇ／Ｌ符合比尔定律,配合物的组成为ｎＴｉ∶ｎＢＰＲ∶ｎＢＲＢ＝１∶２∶２。考察了共存离子的干扰情况。结合阴离子交换树脂分离富集,方法用于地质样品中微量钛的测定,结果与标准值相符,其ＲＳＤ（ｎ＝５）小于２％。