Element Dichroic Focussing Optic 1 Degree of Freedom x y x y z x y z z x y x y z x y z x y x y z z FM1 Focussing Optic 2 FM2 CCD Error budget OAP Layout DT Layout DLT Layout Zoom Layout 0.040 0.052 0.047 0.066 0.044 0.058 0.045 0.071 0.50 µm 0.47 µm 0.47 µm 0.33µm 0.39 µm 0.42 µm 0.35 µm 0.28µm 70µm 140 µm 140 µm 55µm ...

ZSS 70 12:02:56 -61:39:03 new-HIZSS070 #FR Clipped rms: 0.0478 Jy #FN ( 46 out of 69 channels) #MC xaxis: optical #MX Maximum: 0.627 Jy at 1451.328 km/s #MN Minimum: - 0.057 Jy at 1704.609 km/s #NP Number of spectral points: 23 #CL Clipping inside range ( 0.000 , 0.000 ) Jy Moment: 0 1 2 #MM 93.693 1536.687 66.887 Robust moments: 0 1 2 #MR 93.862 1533.874 59.465 units : Jy km/s km/s km/s Width maximiser: 50% 20% #MXC Line centre : 1539.984 ...

... XMM­Newton CCF Release XMM­ CCF ­REL­289 Page: 3 R1o1 R1o2 R2o1 R2o2 target rev ObsID ADU CTI nT nB nT nB ADU CTI nT nB nT nB PKS2155­304 1543 0411780301 0021 0009 234478 9090 48046 2991 0024 0010 242547 8289 41591 2502 0022 0010 232217 9133 45119 2921 0025 0011 239168 8343 39316 2469 Mkn421 1640 0560980101 0021 0009 854199 28212 198595 10399 0024 0010 880754 28080 170938 8179 0022 ... The ADU and CTI columns indicate the ADUCONV and CTI CCF version numbers. ...

... Chandra Survey . ... Optical Database . ... The R (1200 sec total exposure time), I (540 sec), and Halpha (4500 sec) images show a source at RA(J2000)=17h 49m 55.34s, Dec(J2000)=-29d 19m 19.7s. At an offset of 0.16", this is consistent with the Chandra position. ... Given the error on the Faulkes position (0.3"), and the absence of other sources in the Mosaic and Faulkes images within 1.8" of the Chandra position, we consider our Mosaic source and the proposed optical counterpart to be the same. ...

... One striking feature is a small source of almost pure H 2 line emission, which is located near one of the compact sources in Orion reported by O'Dell and collaborators (HST-18 = 203-504). ... H-H objects, Proplyds, Orion Bar, H 2 . ... We obtained a series of images across the bright rim of the Orion Bar near the peaks of mm-wave molecular line emission with NICMOS cameras 1-3 (NIC1, NIC2, NIC3) in several filters on 1998 February 18. ... The suggestion of an H-H object does not seem compelling. ...

Astronomy Astrophysics manuscript no. aa10321 August 19, 2008 c ESO 2008 Quasi-Hilda Comet 147P /Kushida-Muramatsu Another long temporary satellite capture by Jupiter K. Ohtsuka1 , T. Ito2 , M. Yoshikawa3 , D. J. Asher4 , and H. Arakida 1 2 3 4 5 5 Tokyo Meteor Network, Daisawa 1­27­5, Setagaya ... Every case has been associated with a QHC: 82P/Gehrels 3; 111P/Helin-Roman-Crockett; P/1996 R2 (Lagerkvist); and the possibly QHC-derived D/1993 F2 (Shoemaker-Levy 9, SL9). ... Comets or asteroids? ...

Inscrivez-vous †а la newsletter | ... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualit†йs . des reportages . ... les plus belles images de l'Univers d†йcrypt†йes pour vous . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil Challenge Photo Portfolio . ... Publi par M. Chr†йtien . Publi par A. Lepanot . ...

... Optical design . ... TDI OPTICAL SUMMARY . ... Tr: 0.00 ' 4760A fb=-0.361 h= - 0.000 eps ,z=0.018 0.018 Tr: 30.00' 4760A fb=-0.088 h= -108.452 eps ,z=0.015 0.015 Tr: 45.00' 4760A fb= 0.052 h= -162.685 eps ,z=0.013 0.013 Tr: 60.00' 4760A fb=-0.084 h= -216.913 eps ,z=0.010 0.010 Tr: 70.00' 4760A fb=-0.458 h= -253.069 eps ,z=0.011 0.011 Tr: 73.00' 4760A fb=-0.632 h= -263.918 eps ,z=0.011 0.011 Tr: 82.00' 4760A fb=-1.380 h= -296.474 eps ,z=0.015 0.015 Tr: 90.00' 4760A fb=-2.399 h= -325.431 ...

... T A B * * Extinction table for AAO. ... SET .Z.LABEL = "Extinction" * 3200 1.084 3250 0.948 3300 0.858 3350 0.794 3400 0.745 3450 0.702 3500 0.665 3571 0.617 3636 0.575 3704 0.532 3862 0.460 4036 0.396 4167 0.352 4255 0.325 4464 0.279 4566 0.259 4785 0.234 5000 0.203 5263 0.188 5556 0.177 5840 0.166 6056 0.160 6436 0.123 6790 0.098 7100 0.094 7550 0.080 7780 0.076 8090 0.080 8370 0.077 8708 0.057 9832 0.080 10256 0.050 10400 0.051 10610 0.053 10796 0.056 10870 0.064 ...

... Uniquely heavy t = 1.4 GeV .. ... Identify heavy-quark signals with Mcorr Flavor tagging heavy-quark 22000 1200 20000 18000 1000 16000 14000 800 12000 600 10000 8000 400 6000 4000 2000 0 0 1 2 3 4 5 6 7 0 0 uds-quark b c uds 200 2 4 6 8 10 12 14 PT corrected mass( GeV ) # of significant tracks in jet b efficiency = 67% purity = 95% efficiency = 67% purity = 97% : PT corrected mass 1.8 GeV uds: Nsig = 0 efficiency = 87% purity = 79% c+b: PT corrected mass 0.5 GeV Reconstructed W with 2 ...

... Nikolaev 2.8 USNO 104 Italy, San 0.40 21 x 21' 2.5 10 32 0.253 0.436 Marccello 2.0 GSC 106 Slovenia, 0.36 36 x 36' 2.0 2235 9264 0.307 0.295 Crni vrh 2.4 USNO 113 Germany , 0.50 13 x 10' 2 42 283 0.260 0.319 Schonbrunn 2.3 USNO 114 213 1172 0.260 0.222 118 Slovakia, 0.57 14 x 10' 1.7 7 42 0.165 0.077 Modra 3.3 USNO 130 Italy, 0.4 15 x 10' 1.0 9 36 0.284 0.275 Lumezzane 1.8 ... 1.8 UCAC A24 New Millennium 0.36 12 x 12' 1.4 86 399 0.341 0.284 Obs., ... 3.5 UCAC H15 ISON-NM Obs., ...

... 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...