... All exposures used the CASTLE Xenon source lamp, with a 5 µm pinhole used to provide an unresolved target. ... 2 ST-ECF Instrument Science Report WFC3-2005-17 Table 1. Log - June 2004, ambient tests. ...
... 2005 Herschel: A 3.5 m telescope at L2 HIFI: Heterodyne single pixel system 480 to 1250 & 1410 to 1910 GHz FWHP beamsize 12" to 45" SPIRE: Spectral and Photometric Imager Bands at 250, 360 & 520 micrometers FWHP beamsizes 17", 24", & 35" Field-of -View ...
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Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf -- 2622.1 Кб -- 04.09.2008 Похожие документы
... for details, F 0 = d F ~ Nl0 (T1 +T2 )cos((nlm -m)t+nlm )+(T3 +T4 +T5 )cos(nlm -m)t ... m cos r [ynlm (r )+ 2 m ynlm (r )] ~ 0 nlm l l d k=-l lmk (i)NlkPlk ()sin((nlm -m)t ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/daszynskaj.pdf -- 222.6 Кб -- 12.06.2006 Похожие документы
... by 3.5 1.75 by 3.5 1.75 by 3.5 Table 4: Some Characteristics of SPIRE Central Wavelength (m) 250 360 520 Pixel Size (") 12 18 24 Angular Resolution (") 17 24 35 Number of pixels 139 88 43 Field of View (') 4 by 8 4 by 8 4 by 8 9 Figure 3: The Hubble Deep ...
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... and Photometric Stability, ISR ACS 2002-004 KЭmmel, M., Larsen, S. S., & Walsh, J. R., 2005, Slitless Spectroscopy with the Advanced Camera for Surveys, 2005 HST Calibration Workshop, STScI (astro-ph/0512102) 17 ST-ECF Instrument Science Report ACS-2006 ...
... Summary of NIR grism calibrations during TV3 Test procedure IR14S01 IR14S02 IR14S03 IR14S04 IR16S10 IR16S60 Date 20082008200820082008200803 03 03 03 04 04 14/17/18 14/17 16 16 06 06 G G G G G G G rism 102 141 102 141 102 141 Purpose Flat field Flat field ...
... R. A. E. Fosbury 1 ST-ECF, Garching bei M?nchen, Germany, (rfosbury@eso.org) . ... J. Vernet ESO, Garching bei M?nchen, Germany . ... M. Villar-Mart?n Department of Physics & Astronomy, University of Sheffield, UK . ...
... At a distance of about 17,000 light years, this cluster is barely visible to the ... the active control of the 8.2-m mirror, the accuracy of the telescope motions, and ...