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    1. A Study of Heating and Cooling of the ISM in NGC 1097 with Herschel-PACS and
    ... FIR) [C II]158 нјm and [O I]63 нјm lines and mid-infrared H2 emission lines as ... heating efficiency ([C II]158 нјm+[O I]63 нјm)/PAH in the ring about 50% lower than ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2012ApJ...751..144B.html -- 5.2 Кб -- 21.01.2016
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    2. Far-infrared line imaging of the starburst ring in NGC 1097 with the
    ... we map the important ISM cooling and diagnostic emission lines of [OI] 63 нјm, [OIII] 88 нјm, [NII] 122 нјm, [CII] 158 нјm and ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010A&A...518L..60B.html -- 5.0 Кб -- 21.01.2016
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    3. Figure 63
    ... Fig. 63 M = 10 6 M . M low = 1 M . Download here . Download here . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/starburst99/figs/fig63.html -- 2.6 Кб -- 21.08.1998
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    4. http://www.stsci.edu/institute/conference/acs_hls/clampin.pdf
    ... 159, 000 e- Dar k current at -82oC9. 5 e-/pi x/ hr Quantum Effici ency 250 n m 35% 300 n m 36% 350 n m 39% 400 n m 47% 500 n m 59% 600 n m 63% 700 n m 62% 800 n m 50% 900 n m 35% 1000 n m 14% Read Noi se (A-B) 4. 1 e-, 4.1 eRead Noi se (C-D) 4. 1 e-, 4 ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/acs_hls/clampin.pdf -- 1794.7 Кб -- 28.03.2006
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    5. http://www.stsci.edu/jwst/instruments/niriss/docarchive/NIRISS-pocket-guide.pdf
    ... Slitless Spectroscopy GR700XD grism + CLE AR · Two cross-dispersed orders · Spectral coverage 0.6 ­ 2.8 m · Resolving Power 1st order: 700 @ 1.25 µm 2nd order: 700 @ 0.63 µm The orders are broadened in the cross-dispersion direction by 20 ­25 pixels ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/instruments/niriss/docarchive/NIRISS-pocket-guide.pdf -- 1191.2 Кб
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    6. http://www.stsci.edu/hst/acs/documents/isrs/isr0709r.pdf
    ... 66.74804 67.29099 66.16063 65.95987 71.51536 63.45604 57.14285 59.26698 68.04175 58.16102 m ST F250W 14.7 15.0 15.6 15.8 15.9 ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/acs/documents/isrs/isr0709r.pdf -- 1316.8 Кб -- 19.11.2007
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    7. http://www.stsci.edu/~inr/nstarpap/paper2.ps
    ... The three new identifications are LP 993­116 (M V = 13.45), LHS 6167 (M V = 14.63) and G 161­71 (M V = 14.76). ... 2.08±0.42 2.06±0.24 · · · 25.9±3.3 6.76 11.63 N -- 15 -- Table 3---Continued NLTT (m­M)V-K (m­M)V-I (m­M)I-J (m­M)ph (m­M)# df ...
    [ Текст ]  Ссылки http://www.stsci.edu/~inr/nstarpap/paper2.ps -- 655.0 Кб -- 08.06.2007
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    8. http://www.stsci.edu/institute/conference/astro2020/images/Isaak_2020.pdf
    ... Water ices can only be directly detected through the 44/ 63µm emission features The predicted photospheric emission for an AO (Vega-like) star as a function of wavelength and distance from the Sun. ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/astro2020/images/Isaak_2020.pdf -- 1248.7 Кб -- 17.12.2007
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    9. http://www.stsci.edu/stsci/meetings/space_detectors/ircase.htm
    ... Finally, it could also find ice through its 63 m m emission feature, indicative of a zone responsible for comets. Figure 11 . 3. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/ircase.htm -- 36.1 Кб -- 30.08.2001
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    10. http://www.stsci.edu/hst/wfc3/documents/published/SPIE_MR.pdf
    ... Main performances requirements for the WFC3-1R detector were: 1. mean dark current <0.2e/s at 150K, 2. quantum efficiency >45% over the entire range 1.0-1.63µm, 3. readout noise <30 e- rms with correlated double sampling. ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/published/SPIE_MR.pdf -- 809.7 Кб -- 05.02.2013
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