Sat Apr 9 03:44:25 AST Number Name RA (Date) Dec (Date) Delt Diam BW S/Nday S/Nrun Runs Mag 0 2016_FG39 07 17 55.22 +35 16 17.9 0.012 .013 1. ... 25.207.8 20.2 0 2016_EH157 02 51 51.61 +27 54 56.9 0.068 .182 2. ... 60.0 23.3 0 2016_EV27 18 19 57.22 +28 02 58.8 0.045 .063 0. ... 3.0 10.2 6 Hebe 11 52 45.49 +16 49 51.1 1.990 217. ... 2.0 10.1 4 Vesta 02 51 6.19 +12 05 13.5 3.438 690. ... 77.0 19.6 40 Harmonia 08 53 45.31 +22 21 18.7 1.832 120. ... 3.0 12.7 0 2016_FX2 11 28 48.01 +01 53 9.7 0.074 .057 0. ...

... 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. ...

ALMA Memo 588, 1­15; (2009) Printed 24 July 2009 ALMA Memo #588 Inference of Coefficients for Use in Phase Correction II: Using the Observed Correlation Between Phase and Sky Brightness Fluctuations B. Nikolic Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge CB3 0HE, UK email ... Whatever the model is that is chosen, there will however be some errors which will limit the accuracy with which the phase correction coefficients are estimated. ... Springer 2009 ALMA Memo 588 ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . Meteor outburst predicted for 2014 May 24th, peak activity close to 07:00 UT. ... Table of 209P trail encounters in 2014 May . Comments on the data in the table . ... In this context "dust trail theory" refers to the fact that the set of meteoroids released from a parent comet during a single perihelion return stretch out into a dense, narrow dust trail during their early orbital evolution. ... 0.001 . ... 0.000 . ...

... 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. ...

... Based on fX / fO , LX , X-ray spectral hardness, and optical emission-line diagnostics, we have conservatively classified 36 normal galaxies and 71 AGNs. ... 2004). ... In x 3 we discuss normal galaxies in terms of their LX /LB evolution, log (N )-log (S ) relation, and X-ray luminosity function. ... Therefore, to further separate AGNs from normal galaxies, we use several diagnostics: the X-ray luminosity, X-ray to optical flux ratio, X-ray spectral hardness, and optical line ratios. ...

... 5-GHz total flux density . ... color gif | ... Correlated flux density (Jy) vs. projected baseline length plot . gif | ... flux density (Jy) . EW position (mas) . ... 0.7 . ... 2.3 and/or 8.4 GHz: multiple epoch 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 USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . ... 2000), ApJS, 131, 95-183 . ...

DS232A Dual RS-232 Transmitter/ Receiver www.dalsemi.com FEATURES Compatible with LT1181A and MAX232A High data rate - 250 kbits/sec under load 16-pin DIP or SOIC package 20-pin TSSOP package for height restricted applications Operate from single +5V power Meets all EIA-232E and ... industrial temperature range available (-40°C to +85°C) PIN ASSIGNMENT C1+ V+ C1C2+ C2VT2OUT R2IN 1 2 3 4 5 6 7 8 16 15 14 13 12 11 10 9 VCC GND T1OUT R1IN R1OUT T1IN T2IN R2OUT ... V CC is the +5-volt input. ...