... Sfit . ... In addition, the variety of possible forms in which observed spectra might be presented (LORES normalised, HIRES fluxed, OPTICAL, ULTRAVIOLET), it is demanding to ensure every mode is operational at once. ... SLV . CHISQ . LORES . ... AMOEBA . ... GENETIC . ... HIRES . ... FLX . ...

VERSION DATE DESCRIPTION 1.0 2011-10-10 created 1.0.1 2011-10-14 improvements for multiple raw_type definitions; match rule includes PRO.CATG 1.0.2 2011-10-21 added : comments; improved check for multiple cell entries; dfosRLSmassage.py for option -C 1.0.3 2011-11-25 slightly changed handling of validity_date for CALSELECTOR 1.1 2011-12-12 added : support for CALSELECTOR validity 1.2 2012-01-10 ...

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Irvin M. Winer . ... Weather . ... Temperature ( F) . ... 0.00 . ... AAG IR Sky Temperature ( C) . ... AAG Adjusted IR Sky Temperature ( C) . ... AAG Ambient Temperature ( C) . ... AAG Temperature Split ( C) . ... 39321 D,01/23,01:10:10, 67, 20,25.43,270, 8, 38, 0.00, 6.18, 63,!251 at 2016.04.09 19:45:25 . ... S-cmd: "(null)" at 2016.04.09 19:45:25 . ... Page last updated on: February 16, 2016 . ... 2013 Winer Observatory. ...

The input data used to compute model 16 (.ps) ( .pdf ) . ... pointing error for the sources taken with model16 ( .pdf ) Background. ... The model is fit to the raw errors. ... Fig. 1 plots the residuals versus za for the azimuth and za errors. ... Fig. 2 plots the azimuth and za (raw Errors - ( model + encoderTable) ) residuals versus za. Fig. 3 plots the azimuth and za (raw Errors - (model + encoder table) residuals versus azimuth. Fig. 4 plots the za and azimuth residual errors by source. ...

... ATNF Colloquium . Linking AGN and host galaxy formation . ... It also confirms previous result that strong AGNs are usually hosted by galaxies with young stellar population. Yet different from [OIII] narrow line emission, the IR torus emission is found to be associated with excessive number of close companions when the clustering effect of host star formation is carefully controlled, showing evidence of direct AGN-host connection via galaxy interactions. ... today * ATNF | ...

NAUTICAL ASTRONOMICAL ALMANAC for 2005-2006 (in Russian) . ... The Institute of Applied Astronomy of the Russian Academy of Sciences submits the next issue of тАЬThe Nautical Astronomical Almanac for the years 2005-2006тАЭ (NAA-2) biennial. NAA-2 is based on тАЬ The Nautical Astronomical Yearbook тАЭ (NAY) also prepared by IAA RAS. ... The structure of тАЬThe Nautical Astronomical Almanac for the years 2005-2006тАЭ has not undergone essential changes in comparison with the previous issue of NAA-2. ...

... To execute a user--written MIDAS application program љ (coded in FORTRAN or C), employ the command RUN . The command RUN MYPROG or RUN myprog will execute myprog.exe in a subprocess like any other MIDAS command. ... Program bestfilt just needs the names of the input and output image which are obtained inside the program from the keywords IN_A and OUT_A . ... MIDAS procedure bestfilt.prg . ... RUN BESTFILT ! ... Together with the MIDAS command CREATE/COMMAND BESTFILT/IMAGE @@ bestfilt . ...

We use the near-infrared BrнЕ hydrogen recombination line as a reference star formation rate (SFR) indicator to test the validity and establish the calibration of the Herschel/PACS 70 нјm emission as a SFR tracer for sub-galactic regions in external galaxies. ... We use the extinction corrected BrнЕ emission to derive the SFR(70) calibration for H II regions in these two galaxies. ...

... Includes filters to display : All files, only files with different/dubious longname, only files with a longfilename or only files that have been selected for placement: /pub/os2/util/disk Your name: Keith Merrington Email address: k.merington@gmail.com Program contact name: (same) Program contact email: (same) Program URL: (none) Would you like the contact email address included in listings? yes Operating System/Version: Warp - eCs 2.0 Additional requirements: Replaces: LONGFILEUTILITY0_81,zip ...

... The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL