iniquity 发表于 2025-3-21 17:51:44
书目名称High Resolution Infrared Spectroscopy in Astronomy影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0426479<br><br> <br><br>书目名称High Resolution Infrared Spectroscopy in Astronomy读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0426479<br><br> <br><br>flaggy 发表于 2025-3-21 22:06:58
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 bOPINE 发表于 2025-3-22 03:34:00
http://reply.papertrans.cn/43/4265/426479/426479_3.pngCulmination 发表于 2025-3-22 07:03:06
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.头脑冷静 发表于 2025-3-22 11:07:36
http://reply.papertrans.cn/43/4265/426479/426479_5.pngFLAG 发表于 2025-3-22 13:23:37
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.配置 发表于 2025-3-22 18:51:49
http://reply.papertrans.cn/43/4265/426479/426479_7.pngintimate 发表于 2025-3-22 22:53:56
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.Basilar-Artery 发表于 2025-3-23 02:17:31
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.BALK 发表于 2025-3-23 07:22:59
http://reply.papertrans.cn/43/4265/426479/426479_10.png