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標(biāo)題: Titlebook: High Resolution Infrared Spectroscopy in Astronomy; Proceedings of an ES Hans Ulrich K?ufl,Ralf Siebenmorgen,Alan F. M. Moo Conference proc [打印本頁]

作者: iniquity 時(shí)間: 2025-3-21 17:51
書目名稱High Resolution Infrared Spectroscopy in Astronomy影響因子(影響力)

書目名稱High Resolution Infrared Spectroscopy in Astronomy影響因子(影響力)學(xué)科排名

書目名稱High Resolution Infrared Spectroscopy in Astronomy網(wǎng)絡(luò)公開度

書目名稱High Resolution Infrared Spectroscopy in Astronomy網(wǎng)絡(luò)公開度學(xué)科排名

書目名稱High Resolution Infrared Spectroscopy in Astronomy被引頻次

書目名稱High Resolution Infrared Spectroscopy in Astronomy被引頻次學(xué)科排名

書目名稱High Resolution Infrared Spectroscopy in Astronomy年度引用

書目名稱High Resolution Infrared Spectroscopy in Astronomy年度引用學(xué)科排名

書目名稱High Resolution Infrared Spectroscopy in Astronomy讀者反饋

書目名稱High Resolution Infrared Spectroscopy in Astronomy讀者反饋學(xué)科排名

作者: flaggy 時(shí)間: 2025-3-21 22:06
Conference proceedings 2005red spectrograph; VISIR features a high resolution spectroscopic mode. Together, the instruments combine the sensitivity of an 8m-telescope with the now well-established reliability of VLT-facility instruments. High resolution here means that lines in cool stellar atmospheres and H.II.-regions can b

作者: OPINE 時(shí)間: 2025-3-22 03:34

作者: Culmination 時(shí)間: 2025-3-22 07:03
Mid Infrared Spectroscopic Standards: Observations and Models,9). This allows us to demonstrate that the derived absolute calibration of the spectra is accurate to better than 5% in most cases. Our subsample of MIR calibration standards presented here shall become the primary calibrators of the VISIR instrument.

作者: 頭腦冷靜 時(shí)間: 2025-3-22 11:07

作者: FLAG 時(shí)間: 2025-3-22 13:23
Active Galaxies in the Mid Infrared: Ground-Based versus Space-Born Observations, emission is only detected in starbursts whereas PAH features are significantly reduced or completely absent in AGN. We find that the mid-infrared emission of Seyferts is dominated by a compact core while the starbursts are spatially resolved.

作者: 配置 時(shí)間: 2025-3-22 18:51

作者: intimate 時(shí)間: 2025-3-22 22:53
CRIRES: Context and Status,in the near infrared. This aspect in fact motivated the organization of this workshop to both explore the scientific prospects and prepare the ESO community for the use of the instrument in the not too distant future. Here I will summarize the main characteristics of the instrument and its development status.

作者: Basilar-Artery 時(shí)間: 2025-3-23 02:17
Improving the Accuracy of HCN/HNC Opacity Data and Accounting for Isotopomers,r ab initio counterparts. Thus improving the accuracy of many of the strongest HCN/HNC line frequencies. We propose to generate an approximate H.CN linelist using experimentally determined energy levels of H.CN with our HCN line intensities. Our preliminary results are presented here.

作者: BALK 時(shí)間: 2025-3-23 07:22

作者: Commodious 時(shí)間: 2025-3-23 15:19

作者: restrain 時(shí)間: 2025-3-23 21:32
SIFTIR: Spectro-Polarimetric Imaging Fourier Transform Spectrometer for the InfraRed,n with TNTCAM2 (Klebe et al. 1998), an imaging polarimeter. The FTS component will enhance TNTCAM2, giving the instrument a maximum resolution of 2000 at 10 .m. The FTS is capable of operating between 2–15 .m, but polarimetry for the instrument is limited to the 8–15 .m region due to waveplate/wiregrid characteristics.

作者: progestogen 時(shí)間: 2025-3-23 22:55

作者: ingestion 時(shí)間: 2025-3-24 03:33

作者: 低能兒 時(shí)間: 2025-3-24 10:16
CRIRES: Context and Status,ower of 10. from 1 to 5 .m. It will complement the comparable resolution provided by UVES at visible and ultraviolet wavelengths. Many new scientific prospects will also be opened up by the availability of this new capability for high sensitivity observations at high spectral and spatial resolution

作者: 帳單 時(shí)間: 2025-3-24 14:43
Science Highlights from 4 Years of NIRSPEC on the Keck II Telescope,ensively and successfully over the last four years. In high-resolution mode (R?~?20,000–30,000), NIRSPEC science includes studies of comets and solar system bodies, abundance studies in red giants, the kinematics of the population of stars near the Galactic Center, protostars and disks, low-mass spe

作者: 綠州 時(shí)間: 2025-3-24 15:33

作者: 過濾 時(shí)間: 2025-3-24 22:26
High Resolution Mid-Infrared Spectroscopy of Star and Planet Forming Regions with TEXES,rption and emission toward several embedded young stars. Here, we concentrate on observations of C.H., HCN, SiO, and H. toward the KL region in Orion, with some discussion of molecules observed toward NGC 7538 IRS1. High spectral, and in some cases spatial, resolution is found to be necessary to det

作者: Inflated 時(shí)間: 2025-3-25 01:08

作者: 小歌劇 時(shí)間: 2025-3-25 05:17
,Atomic Data in the 1–5 Micron Region: Present Status,the CRIRES region (1–5 .m). There is a clear distinction between the atomic lines that will appear in absorption in stellar spectra and in emission in nebular spectra. For abundance analyses different classes of lines can be defined on the basis of the energy level structure, either along particular

作者: 不利 時(shí)間: 2025-3-25 11:12
High-Resolution Spectroscopy on the Milliarcsecond Scale,illiarcsecond scale. This enables completely new observational approaches to many open problems in stellar and circumstellar astrophysics. Fiber coupling of the output from a relatively simple beam combiner to existing spectrographs offers a cost-effective way to implement interferometric high-resol

作者: 合同 時(shí)間: 2025-3-25 14:05

作者: Mri485 時(shí)間: 2025-3-25 19:28

作者: Invertebrate 時(shí)間: 2025-3-25 22:09
T-ReCS and Michelle: The Mid-Infrared Spectroscopic Capabilities of the Gemini Observatory,llow observers the unique opportunity to apply to one observatory for all-sky spectroscopic access in the mid-infrared with the light gathering power of 8-meter telescopes. Gemini South has recently commissioned the Thermal-Region Camera and Spectrograph (T-ReCS) and is now available to perform queu

作者: 褲子 時(shí)間: 2025-3-26 00:30
Improving the Accuracy of HCN/HNC Opacity Data and Accounting for Isotopomers, the inherent accuracy problems of ab initio data. The band centres of some overtone bands deviate by up to 10 cm. from experimental values. To improve the quality of many of our line frequencies we are in the process of substituting the available experimentally determined HCN energy levels for thei

作者: 一再困擾 時(shí)間: 2025-3-26 04:35
SIFTIR: Spectro-Polarimetric Imaging Fourier Transform Spectrometer for the InfraRed,ith which to diagnose grain characteristics. We are currently developing an instrument that will employ a Fourier transform spectrometer in conjunction with TNTCAM2 (Klebe et al. 1998), an imaging polarimeter. The FTS component will enhance TNTCAM2, giving the instrument a maximum resolution of 2000

作者: MEEK 時(shí)間: 2025-3-26 11:46
Mid Infrared Spectroscopic Standards: Observations and Models,MI2 instrument at the ESO/La Silla observatory. The low resolution spectra (R?≈?160) were analyzed with an optimal extraction procedure specifically designed for TIMMI2 spectroscopy. The wavelength calibration was done using atmospheric lines. Our analysis package is based on IDL and will be made av

作者: Feigned 時(shí)間: 2025-3-26 15:49
GIANO: An Ultra-Stable IR Echelle Spectrometer for the TNG Telescope,dial velocity measurements. It also includes polarimetric capabilities and a low resolution mode that make it a very versatile, common user instrument which will be permanently mounted and available at one of the Nasmyth foci of the Telescopio Nazionale Galileo (TNG) located at Roque de Los Muchacho

作者: 分貝 時(shí)間: 2025-3-26 19:42

作者: 是貪求 時(shí)間: 2025-3-26 23:32

作者: capsule 時(shí)間: 2025-3-27 04:46

作者: Ringworm 時(shí)間: 2025-3-27 06:41

作者: 側(cè)面左右 時(shí)間: 2025-3-27 13:27
John H. Black savings. Despite this, there is no comprehensive description of fund manager behaviour, much less a matching theory. This is troubling because one of the most economically significant puzzles in finance is why experienced, well-resourced fund managers cannot outperform the market..Applied Investmen

作者: Intruder 時(shí)間: 2025-3-27 13:38

作者: Compassionate 時(shí)間: 2025-3-27 21:01

作者: MOTIF 時(shí)間: 2025-3-28 01:25

作者: Truculent 時(shí)間: 2025-3-28 03:11
Alistair C.H. Glassening why, where and how the theory fails to explain what hap.Institutions now dominate trading in equities around the world. Mutual funds are the most prominent, and doubly important as custodians of retirement savings. Despite this, there is no comprehensive description of fund manager behaviour, m

作者: rods366 時(shí)間: 2025-3-28 09:52

作者: Anterior 時(shí)間: 2025-3-28 11:03

作者: 恫嚇 時(shí)間: 2025-3-28 15:50

作者: 母豬 時(shí)間: 2025-3-28 21:12

作者: indignant 時(shí)間: 2025-3-29 02:29

作者: 充滿裝飾 時(shí)間: 2025-3-29 06:59
Katelyn N. Allers,Daniel T. Jaffe,John H. Lacy,Matthew J. Richterning why, where and how the theory fails to explain what hap.Institutions now dominate trading in equities around the world. Mutual funds are the most prominent, and doubly important as custodians of retirement savings. Despite this, there is no comprehensive description of fund manager behaviour, m

作者: FIG 時(shí)間: 2025-3-29 08:11
James M. De Buizer,R. Scott Fisher savings. Despite this, there is no comprehensive description of fund manager behaviour, much less a matching theory. This is troubling because one of the most economically significant puzzles in finance is why experienced, well-resourced fund managers cannot outperform the market..Applied Investmen

作者: COMA 時(shí)間: 2025-3-29 13:27

作者: 群島 時(shí)間: 2025-3-29 18:36
Colby Jurgenson,Robert Stencelof the most visible and respected Canadian psychologists worldwide. In light of his upcoming retirement in December 2006, the Festschrift will recognize Dr. Yuille’s achievements in the areas of eyewitness memory research (i.e., pioneering a new research paradigm that grants better validity), invest

作者: ticlopidine 時(shí)間: 2025-3-29 20:34
Katrin K?mpgen,Ralf Siebenmorgenof the most visible and respected Canadian psychologists worldwide. In light of his upcoming retirement in December 2006, the Festschrift will recognize Dr. Yuille’s achievements in the areas of eyewitness memory research (i.e., pioneering a new research paradigm that grants better validity), invest

作者: 懶鬼才會衰弱 時(shí)間: 2025-3-30 02:57

作者: 凹處 時(shí)間: 2025-3-30 08:02

作者: pus840 時(shí)間: 2025-3-30 10:36

作者: occurrence 時(shí)間: 2025-3-30 16:21

作者: 使人入神 時(shí)間: 2025-3-30 16:54
https://doi.org/10.1007/b96749Active Galaxies; Astronomical Observation; High Resolution Infrared Spectroscopy; Interstellar Medium; P

作者: leniency 時(shí)間: 2025-3-30 21:18
The High-Resolution Frontier in Infrared Spectroscopy,rophysics. A few examples are discussed, including isotope abundances in rapidly evolving stars, absorption spectroscopy of interstellar clouds, and terrestrial remote sensing with astronomical facilities.

作者: 抵押貸款 時(shí)間: 2025-3-31 02:17

作者: Heart-Rate 時(shí)間: 2025-3-31 05:02
High-Resolution Spectroscopy on the Milliarcsecond Scale,illiarcsecond scale. This enables completely new observational approaches to many open problems in stellar and circumstellar astrophysics. Fiber coupling of the output from a relatively simple beam combiner to existing spectrographs offers a cost-effective way to implement interferometric high-resolution spectroscopy at the VLTI.

作者: 慎重 時(shí)間: 2025-3-31 11:27