... 3.6, 4.5, 5.8, and 8.0 µm) and MIPS (24, 70, and 160 µm) mosaics, obtained in May ... L(24 µm) (erg s-1) Conversely, the 8 µm luminosit y does not appear to be as closely ...
... There is significant diffuse emission in the IRAC 8 О?m band after starlight has been removed by scaling shorter wavelength ... shows spatially variable PAH emission demonstrates the complexity of interpreting diffuse 8 О?m emission in galaxies ...
... Evidence for a 3 10 8M Black Hole in NGC 7052 from HST Observations of the Nuclear Gas Disk. ... Models with a black hole of mass M = 3.3 +2.3 -1.3 10 8M provide an acceptable fit. ...
... PACOR BPatel · Fro m Ju n e 1 4 (8 a m ) to Ju n e 1 5 (8 a m ), Pacor-A received one event with fast-track o b se rva tio n s. · Th e d a ta w a s p ro ce sse d a n d d e live re d to O P U S w ith o u t a n y p ro b le m s. ...
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Ссылки http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/smov4notes/SMOVMeetingReportsOPUS_and_PACORfor15Jun09.pdf -- 27.4 Кб -- 23.06.2009 Похожие документы
... 2 May 30 P lo t o f a v e ra g e m a g d iffe re n c e fo r F 1 1 5 L P filte r o v e r tim e f o r 7 0 s ta rs in N G C 6 6 8 1 M ay 2 May 30 P lo t o f a v e ra g e m a g d iffe re n c e fo r F 1 2 5 L P filte r o v e r tim e f o r 7 0 s ta rs in N G C ...
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Ссылки http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/smov4notes/ACSSBCfirstUVcontamcheck31May09.pdf -- 427.0 Кб -- 03.06.2009 Похожие документы
... Welcome: Matt Mountain, STScI Director The Goals of this Year's Symposium Jason Kalirai and Massimo Robberto (STScI) 8:30-8:45 a.m. 8:45-9:00 a.m. Mike Fa ll The Formation of Stars and Stellar Populations The Formation of Stars Jonathan Tan (Univ. of ...
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Ссылки http://www.stsci.edu/institute/conference/spring2010/schedule.pdf -- 154.2 Кб -- 03.05.2010 Похожие документы
... in the spectral range 0.8<<1.8 µm. The F160W spectral element has been used in the ... in the spectral range 0.8<<1.8 µm. The lower panel shows the backround expressed in ...
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Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-13.pdf -- 63.7 Кб -- 25.09.2008 Похожие документы
... detector will be sensitive to wavelengths below 0.8 µm. This ISR gives the expected transmission of these glasses ... The WFC3 IR channel contains a HgCdTe detector for sensing light from 0.8 µm to 1.7 µm. This type of detector is grown on a ...
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Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2005-23.pdf -- 107.6 Кб -- 29.11.2007 Похожие документы
... at 3.6, 4.5, 5.8, 8.0 µm and with the Multiband Imaging Photometry for Spitzer (MIPS ... and the mosaicking was done 5.8 µm images suffered from poor dark subtraction be ...
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Ссылки http://www.stsci.edu/~kgordon/papers/PS_files/spitzer_newviews_m101.pdf -- 352.9 Кб -- 01.03.2005 Похожие документы