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181. http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_012.pdf
... The NICMOS target acquisition allows the user to acquire a point source and position it into the coronagraphic hole. ... FSW - Target Location Prop.ID (visit) 7226 (03) 7226 (04) 7226 (13) 7226 (14) 7226 (57) 7226 (58) 7226 (61) 7226 (62) 7227 (07) 7227 (08) 7227 (17) 7227 (18) 7227 (45) 7227 (46) 7227 (49) 7227 (50) 7227 (57) 7227 (58) 7227 (59) 7227 (60) 7233 (05) 7233 (06) 7233 (13) 7233 (32) 7233 (33) 7329 (61) 7329 (81)* X-center ( ...
[ Текст ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_012.pdf -- 308.2 Кб -- 12.02.2002
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182. Accuracy of World positional CCD observations of the numbered minor planets
... For reliable estimation of the accuracy of asteroid CCD observations we usually consider from ten or more various NUMBERED MINOR PLANETS (NMPs) observed during several nigths per month (more then 50 positions). ... They can be considered as an indicator of accuracy of the CCD positional observations with given MPC code. ... For any NUMBERED minor planet the (O-C) values must be zero if the errors of observations and the errors of its theory are absent. ...
[ Сохраненная копия ]  Ссылки http://www.accuracy.puldb.ru/METHOD.HTM -- 21.2 Кб -- 05.12.2007
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183. http://xmm.vilspa.esa.es/calibration/ept/fluxChandra/SAS7.1_CIAO4.0-3.4.2/0124930301_3168B.txt
FIT aciss-heg+1 aciss-heg-1 aciss-leg+1 aciss-leg-1 aciss-meg+1 aciss-meg-1 combined hrci-leg +... hrci-leg -... hrcs-leg +... hrcs-leg -... m1 m2 pn r1 r2 0.15-0.33 0 0 0 2.547e-05 0 0 7.082e-02 0 0 0 0 6.699e-02 8.478e-02 6.485e-02 2.136e+01 6.000e-02 0.33-0.54 0 0 0 1.646 0 0 2.399 0 0 0 0 ... .925 2.916 2.862 2.834 3.003 0.50-2.00 0 0 0 0.83220.01240 0 0 0.734820.01240 0 0 0 0 0.86940.01240 0.64940.01240 0.662370.01240 0.0000.01240 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/ept/fluxChandra/SAS7.1_CIAO4.0-3.4.2/0124930301_3168B.txt -- 2.0 Кб -- 04.02.2015
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184. http://www.winer.org/Downloads/astro-ph-KELT-3b.pdf
... Table 1 lists all RV data for KELT-3 , and Figure 2 shows 20 TA B L E 1 RV O B S E RVAT I O N S O F K E LT- 3 BJD RV RV errora Source (TDB) (m s-1 ) (m s-1 ) 2455983.672916 -319 25 TRES 2455990.777987 -66 14 TRES 2456000.473809 -31 27 FIES 2456001.465355 103 20 FIES 2456002.514673 -259 20 FIES 2456003.552533 90 16 FIES 2456004.432251 0 16 FIES 2456018.656206 -324 14 TRES 2456019.709404 4 19 TRES 2456020.710562b -125 18 ... Both observations were able to resolve KELT-3 from...
[ Текст ]  Ссылки http://www.winer.org/Downloads/astro-ph-KELT-3b.pdf -- 1862.3 Кб -- 06.12.2013
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185. http://star.arm.ac.uk/preprints/2015/670.pdf
... 000, 1­18 (2014) Printed 1 June 2015 A (MN L TEX style file v2.2) On the calibration of the relation b etween geometric alb edo and p olarimetric prop erties for the asteroids A. Cellino1, S. Bagnulo2, R. Gil-Hutton3, P. Tanga4, M. Canada-Assandri3, ~ 5 and E. F. Tedesco 1 2 3 4 5 INAF - Osservatorio Astrofisico di Torino, I-10025 Pino Torinese, Italy. ... The task of determining the alb edo based on available phase-p olarization curves is imp ortant in asteroid science. ...
[ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2015/670.pdf -- 710.6 Кб -- 01.06.2015
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186. http://hea-www.harvard.edu/~pgreen/HRCULES/table2.ps
TABLE 2 Partial correlations All data (including upper limits) Detections only Line logW – vs. log L 2500 logW – vs. log z logW – vs. log L 2500 logW – vs. log z P ae P ae P ae P ae LBQS Sample Fe UV 0.177 ­0.033 !0.005 ­0.123 0.175 ­0.983 0.175 ­0.983 Lyfi+OVI .. ... C III] 0.066 0.060 0.011 ­0.091 .. ... 18:6 Subsample Fe UV 0.177 ­0.033 !0.005 ­0.123 0.244 ­0.030 0.208 ­0.037 Lyff !0.005 0.379 !0.005 ­0.446 !0.005 0.161 !0.005 ­0.258 Si IV + OIV] .. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/HRCULES/table2.ps -- 68.2 Кб -- 27.12.2000
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187. Siding Spring Survey NEA discoveries 2007
NEA discoveries made with the Uppsala Schmidt (E12) and ANU 40-inch (413) Status as at 2010 Sep 14 Atens Designation q Q a e i H opps Date last obs 2007 VL243 0.262 1.668 0.965 0.729 43.3 17.8 2 E12 2008 Nov. ... 15 PHA 0.019 2007 TD 0.321 1.059 0.690 0.535 3.5 24.4 ( 7d) E12 2007 Oct. ... 15 2007 XH16 0.908 1.466 1.187 0.235 27.4 19.7 (193d) E12 2008 June 18 PHA 0.015 2007 WW4 0.594 3.598 2.096 0.717 10.4 19.5 ( 45d) E12 2008 Jan. ... 2007 GS3 0.924 1.198 1.061 0.129 15.1 19.4 2 E12 2008 Nov. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/e12-2007.htm -- 6.4 Кб -- 14.09.2010
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188. J0057+3021
... 5-GHz total flux density . ... 0.017 * = the position has been determined to an accuracy of 10 mas from the VLBApls data . VLBApls image at 5 GHz . color gif | contour gif | ... Correlated flux density (Jy) vs. projected baseline length plot . gif | ... flux density (Jy) . EW position (mas) . ... major axis (mas) . minor axis (mas) . position angle ( ) . ... 2.0 0.3 . ... 5 GHz: see Gurvits et al. ... VLBApls reference: Fomalont et al. ... VLBApls home page . ...
[ Сохраненная копия ]  Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0057+3021.htm -- 3.7 Кб -- 08.05.2001
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189. Satellites of the Giant Planets
... Amalthea 181400 0.389 0.003 168 E.E. Barnard (1892) XIV Thebe 221900 1.070 0.018 98 S.P. Synnott/Voyager 1 (1980) I Io 421800 0.036 0.000 3643 Galileo (1610) II Europa 671100 0.467 0.000 3122 Galileo (1610) III Ganymede 1070400 0.172 0.001 5262 Galileo (1610) IV Callisto 1882700 0.307 0.007 4821 Galileo (1610) XVIII Themisto S/ 2000 J1#1 7507000 43.08 0.242 9 S.S . Sheppard et al ( 2000 , ... 2002, IAUC 8213) #1: Jupiter satellite S/2000 J1 (Themisto) = S/1975 J1. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~pfreire/space/satellites.html -- 18.0 Кб -- 27.01.2008
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190. field details
. *********** FIELD 1 ************* . *********** FIELD 2 ************* . *********** FIELD 3 ************* . *********** FIELD 4 ************* . *********** FIELD 5 ************* . *********** FIELD 6 ************* . *********** FIELD 7 ************* . *********** FIELD 8 ************* . *********** FIELD 9 ************* . *********** FIELD 10 ************* . *********** FIELD 11 ************* . *********** FIELD 12 ************* . *********** FIELD 13 ************* . *********** FIELD 14 ************* .
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19960410_OpticalDesign/field_details.html -- 120.2 Кб -- 19.05.1998
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191. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 337, 275­292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
[ Текст ]  Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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192. http://www.stsci.edu/hst/acs/analysis/STECF/isr/isr0603.pdf
ST-ECF Instrument Science Report ACS-2006-03 Wavelength and Flux calibration of the ACS/HRC PR200L prism S. S. Larsen, J. Walsh and M. KЭmmel, March 2006 ABSTRACT Wavelength- and flux calibrations are presented for the ACS/HRC PR200L slitless spectroscopy mode. ... Wavelength solutions for the PR200L prism. ... Wavelength. ... 12 ST-ECF Instrument Science Report ACS-2006-03 Figure 7: Comparison of the aXe-extracted prism spectra of the two flux standards with the reference spectra. ...
[ Текст ]  Ссылки http://www.stsci.edu/hst/acs/analysis/STECF/isr/isr0603.pdf -- 788.6 Кб -- 02.12.2010
[ Текст ]  Ссылки http://www.stecf.org/documents/isr/isr0603.pdf -- 559.5 Кб -- 11.05.2006
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