HIP 356 07:44:14 -35:48:53 new #FR Clipped rms: 0.0130 Jy #FN ( 56 out of 86 channels) #MC xaxis: optical #MX Maximum: 0.185 Jy at 2775.752 km/s #MN Minimum: - 0.026 Jy at 3058.186 km/s #NP Number of spectral points: 30 #CL Clipping inside range ( 0.000 , 0.000 ) Jy Moment: 0 1 2 #MM 26.370 2861.643 95.721 Robust moments: 0 1 2 #MR 26.653 2838.198 85.425 units : Jy km/s km/s km/s Width maximiser: 50% 20% #MXC Line ...

... Multiwavelength Milky Way . Our solar system consists of an average star we call the Sun , the planets Mercury , Venus , Earth , Mars , Jupiter , Saturn , Uranus , Neptune , and Pluto . ... The whole solar system, together with the local stars visible on a clear night, orbits the center of our home galaxy, a spiral disk of 200 billion stars we call the Milky Way . ... The terrestrial planets are the four innermost planets in the solar system, Mercury , Venus , Earth and Mars . ... Earth's) . ...

... 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. ...

Delay Line Pipes & Supports Design Description v1.0 INT-406-VEN-0115.doc Y Z MRO Delay Line Delay Line Pipes and Supports Design Description Document No. ... 8 2.1.4 End Sections and End Plates .. ... A depiction of the pipes and supports at the BCA end of the delay line is shown in Figure 1. ... 9 Delay Line Pipes & Supports Design Description v1.0 INT-406-VEN-0115.doc End Plate Limit target Plate End Section O-ring B1 M5 M6 M4 B2 M1 M2 Buffer Assembly M3 S1 S2 S3 S4 Figure 4 BCA End Plate. ...

... 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. ...

Next: Status and Goals of Up: NICMOS Data Calibration and Previous: NICMOS Data Calibration and . ... CALNICB Processing . ... Combining NUMITER Images . ... The Space Telescope Science Institute (STScI) data reduction and calibration pipeline for the Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) is composed of two major tasks, CALNICA and CALNICB. ... NICMOS, calibration, pipeline, software . ... CALNICB combines images into mosaics and also removes background signal from the images. ...

... Tonight's Sky . ... Star Atlas . ... Astronomy for Kids . ... The violent birth of neutron stars . ... NEUTRON STARS . ... Supernovae are also the birthplaces of neutron stars, those extraordinarily exotic, compact, stellar remnants in which about 1.5 times the mass of our Sun is compressed to a sphere with the diameter of Munich. ... These neutrinos are produced and radiated in tremendous numbers at the extreme temperatures and densities in the collapsing stellar core and nascent neutron star. ...

... Printed in U.S.A. The Hipparcos and Tycho Photometric System Passbands MICHAEL S. BESSELL Research School of Astronomy and Astrophysics, Institute of Advanced Studies, The Australian National University, Private Bag, Weston Creek P.O., ACT 2611, Australia ; bessell=mso.anu.edu.au Received 2000 March 6 ; accepted 2000 April 17 ABSTRACT. Hipparcos and T ycho magnitudes have been extracted for many of the E-region standard stars. ... B [V regression for the E-region stars. ...

The Use of Neutrals for an Improvement of Higgs BR A Review of and an Update on Higgs BR Jan Strube, Jeffrey J. Early and James E. Brau jstrube@darkwing.uoregon.edu University of Oregon ALCPG Victoria LCWS, 2004 ­ p.1/18 Overview Review of previous analyses Battaglia (Tesla TDR) Potter, Brau, et al. ... JLC) Presentation of new approach ALCPG Victoria LCWS, 2004 ­ p.2/18 Battaglia - 1999 s =350 GeV, mH =120 GeV Two studies (cut-based): 1. CDR Ver texer 2. ...

Optical and UV Spectrophotometric Standard Stars . ... Two papers detail the observations: the first is devoted to wavelengths from 3300 to 7550A (Hamuy et al., ... -------------------------------------------------------- 718 Xi2 Cet B9 III -O.107 -0.056 4.279 -0.023 -0.063 1544 Pi2 Ori Al V 0.01 4.355 0.014 0.039 3454 Eta Hya B3 V -0.743 -0.200 4.295 -0.083 -0.200 4468 Theta Crt B9.5 V -0.18 -0.07 4.700 -O.023 -0.063 4963 ...

... 02138, U.S.A. Prepared using the Tamkin Foundation Computer Network MPC@CFA.HARVARD.EDU URL http://www.cfa.harvard.edu/iau/mpc.html 2008 YK2 Observations: K08Y02K * K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K K08Y02K Observer L. Buzzi. 0.60-m f/4.64 reflector + CCD. ... 704 Lincoln Laboratory ETS, New Mexico. ...

General Forum Message . ... Antigravitational Non-local Spacetime Experiment . ... Hence it can be known that in the antigravitational field the spacetime location of an object is varying. ... In the experiments described in Section 2 below, the scraps serve as the observers. ... The scraps used in Experiment 2 are two other scraps. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... 5-GHz total flux density . ... 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) . ... Other VLBI references . 2.3 and/or 8.4 GHz: VLBI images are available in the USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . 15 GHz: VLBI images are available in the VLBA 2-cm survey (Kellermann et al. ...

... 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. ...

... GRIN lenses for telecommunication optics applications ? GTC (gradient telecom) lenses. ... GTC lenses are used in different fiber-optic devices: collimators, couplers, isolators and WDM etc . ... 2.Diameter . GTC lenses diameters are 1.0 mm, 1.8 mm, 3.0 mm and 4.0mm. ... 1.0 mm -3.0 mm diam GTC lenses are supplied in 0.22P, 0.23P, 0.25P, 0.27P and 0.29P length. 4.0 mm diam GTC lenses are supplied in 0.11P length. ... GTC . ... 3 scratches with 5mkm max width and 200mkm max length are allowed . ...