tricuspid-valve 发表于 2025-3-21 17:48:05
书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0163613<br><br> <br><br>书目名称Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0163613<br><br> <br><br>Liberate 发表于 2025-3-21 22:49:49
Some Quantitative Aspects of Galactic and Extragalactic Infrared Astronomy,Two types of infrared astrophysical problems have been intensively studied in recent years. The first is an investigation of primary coolants. The second is the nature of the diffuse extragalactic infrared background radiation.易改变 发表于 2025-3-22 03:37:17
http://reply.papertrans.cn/17/1637/163613/163613_3.png钢笔尖 发表于 2025-3-22 06:21:21
https://doi.org/10.1007/3-540-45573-6Cosmology; Dark Matter; Data Analysis; Galactic Structure; Infrared Astronomy; Stellar Structure; astronom谄媚于性 发表于 2025-3-22 09:43:29
http://reply.papertrans.cn/17/1637/163613/163613_5.png压倒 发表于 2025-3-22 14:15:20
http://reply.papertrans.cn/17/1637/163613/163613_6.png畸形 发表于 2025-3-22 17:52:48
http://reply.papertrans.cn/17/1637/163613/163613_7.pngAnhydrous 发表于 2025-3-22 22:12:23
http://reply.papertrans.cn/17/1637/163613/163613_8.png易怒 发表于 2025-3-23 02:25:07
Fluorescence methods in polymer science,1995 November 17 and ended its life in May, 1998. It operated in the 2.5 – 18 μm range, and was developed by the ISOCAM consortium lead by the French Service d’Astrophysique of CEA Saclay. This paper reviews different algorithms which can be used for the calibration and analysis of ISOCAM data.Mystic 发表于 2025-3-23 06:12:47
Michio Kurata,Walter H. Stockmayermmunity, covered the wavelength range from 2.5 – 240 μm at a wide variety of spectral and spatial resolutions and was operational between November 1995 and April 1998. The ISO data archive opened to the community in December 1998, at URL “www.iso.vilspa.esa.es”. The paper summarises the design and i