... Posts tagged ?normal? ... Posted by hlee . ... Category: arXiv , Astro , Cross-Cultural , Frequentist , Methods , News , Quotes , Stat , Uncertainty | ... This paper might be an interest for those: Interval Estimation in Exponential Families by Brown, Cai,and DasGupta ; Statistica Sinica (2003), 13 , pp. ... The authors investigated issues in interval estimation of the mean in the exponential family, such as binomial, Poisson, negative binomial, normal, gamma, and a sixth distribution. ...

Hide Zen home . ... sncat2sntab.pl - convert old catalog to table sn . ... CREATE TABLE cats ( id integer PRIMARY KEY, name text ); -- a list of properties of galaxy CREATE TABLE properties ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy _property ( gid integer REFERENCES galaxy (id), pid integer REFERENCES properties(id), value float, UNIQUE( gid ,pid) ); CREATE t=# select * from galaxy; id | ...

Q. Why do I get a blank output page? ... One common example is when the ETC is asked to normalize the flux to a certain value when the flux in the input spectrum is zero. ... Q. If I am supplying my own user-input spectrum, does the spectrum have to cover the whole wavelength range of the observation? ... This was a limitation of the earlier version of the ETC; but the ETC has been enhanced so that the user-input spectrum does not have to cover the entire wavelength range of the observations. ...

... Time related attributes: . observation related: DATE_OBS and DURATION required by XMM-SOC-ICD-0006-SSC ([ 3 ]), write also DATE_END and OBSSTART , OBSSTOP . ... SAS_VERBOSITY should be set to `Sparse' (4) for normal processing and `Verbose' (5) for more detailed processing. Values of 6 and higher may yield quite a number of messages related to rejected events (MIPs) depending on CCD number and instrument mode. SAS_MEMORY_MODEL should be set to `high' for normal processing. ...

... of polarisations ( 1 = DAS inputs 1 and 2 are X, # 2 = DAS input 1 is X and 2 is Y) # # rest freq1 = Rest freq ( MHz ) in IF1 # # rest freq2 = Rest freq ( MHz ) in IF2 (set to 0.0 if no 2nd IF) # # BW1 = bandwidth of IF1 # # BW2 = bandwidth of IF2 (set to 0.0 if no 2nd IF) # # Time = Time needed ON SOURCE ( min ) # # Cor config = correlator config file # # No Avg = number of integrations to average before writing # # ... Pos time = (in min) Time spent at each position offset. ...

... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ... The derived temperature maps are quite similar to the ones obtained earlier with a different methods, the main differences occurring in the spot latitudes and relative strength of the spot structures....

... Day-by-day lines contain complete set and intended for those who have been there (I mean, in Kyoto :) . ... Large format is mainly for 1600x1200 screens and fast link (pictures are up to 150K in size). Normal is for typical 1024x768 screen (i.e. 15" monitors). ... Photos look incredible on it. ... Large . ... Normal . ... Thumbnails . ... Contents with thumbnails: Large | ... Nara, one of the historical cities of Japan . ... August 17, Sunday. ... Nara. ... return to photo album contents | ...

Arecibo Galaxy Environment Survey (AGES) Last Update: . ... 22/12/2006 . ... wapp.20061222.a2048.0001 Scan: AGES3193_p1_101, Got the telescope early, quickly added an extra scan. ... wapp.20061222.a2048.0009 Scan: TOGS calibration, . ... RM, WvD . ... wapp.20061223.a2048.0009 Scan: TOGS calibration, . TOGS had problems at the start. ... wapp.20061226.a2048.0002 Scan: TOGS calibration, . ... wapp.20061226.a2048.0010 Scan: TOGS calibration, . ... wapp.20061227.a2048.0008 Scan: TOGS calibration, . ...

... Data Handling and Products > Data Reduction FAQ > I derived quantities related to the performance of an instrument. How do I know whether these numbers are "normal"? ... Observing with ESO Telescopes . ... Instrument Pipelines . ... ESO-MIDAS . ... ESO Data . ... Related External Services . ... The quality control group at ESO monitors a variety of instrument parameters such as zeropoints, efficiencies, read-out noise, etc. ... http://www.eso.org/observing/dfo/quality/ <INSTRUMENT> /qc/qc1.html . ...

... mag . ... arcsec . ... deg . ... 2015-04-18 20:51:42 . ... Observation . site code . ... site name . Pulkovo . ... mag(J1+J3)-mag(J4) . ... sensor . ... sensor info . 0.533 arcsec/px, FOV = 35x23 arcmin . ...

... We consider stars with a constant (solar) initial chemical composition. Before the Roche lobe overflow, the components evolve as single stars (see for details LPP96). ... If the mass transfer onto a normal star occurs on a time-scale ten time shorter than the thermal Kelvin-Helmholz time for this star or a compact star is engulfed by a giant companion (e.g. as a result of the kick), the common envelope (CE) stage of the binary evolution is set in (Paczynski 1976). ...

Next: Special problems Up: Reducing the observations Previous: Table file output . ... Rejected stars: These are marked with an asterisk (*) in the right margin when the residuals are listed. ... Some plots have fitted lines indicated by a series of dashes. The residual plots identify different stars with different symbols; these are given in the tables of residuals. ... Here, large fluctuations in sky brightness can occur, occasionally producing negative star intensities after sky subtraction. ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... suexec is used by the Apache HTTP Server to switch to another user before executing CGI programs. ... Since the HTTP daemon normally doesn't run as root , the suexec executable needs the setuid bit set and must be owned by root . ... For further information about the concepts and the security model of suexec please refer to the suexec documentation ( http://httpd.apache.org/docs/2.4/suexec.html ). ...

... We have measured this "redshift" for the pink black holes, and allowed for it in our calculations. ... We see this effect in the emission from gas around these pink black holes, but it is far too small an effect to account for the pinkness. Thus the swirling motions of gas around or into the black holes cannot produc the colour. ... At first we thought that these things were normal blue black holes hidden behind clouds of interstellar dust, that absorbed the blue light and made them appear pink. ...

... MIPT Solid State Physics Department . ... Interacting Electrons in Normal Metals . ... The course is an introduction to interacting Fermi-particle physics and intended for future experimentalists. ... Hartree-Fock approximation. ... Linear reaction function. Calculation of density-density reaction function. Relation of density-density reaction function to compressibility of Fermi liquid and thermodynamic state density. ... Density-density reaction function of free Fermi gas in long-wave limit. ...

The examples of the errors. ... Observations with ordinary values of the "Mean error of single observation" Obj Code DT RA (O-C) DEC (O-C) mag z h m s " ° ' " " ° 3907 761 1998 08 24.383673 3 17 44.739 0.28 +30 46 00.84 -0.08 15.8 18 3907 761 1998 08 24.409133 3 17 46.152 0.28 +30 46 10.85 0.12 15.8 11 3907 761 1998 08 25.392523 3 18 40.107 0.33 +30 52 27.69 0.04 15.4 15 Total mean value of 3 observations 0.297±0.017 0.027±0.058 Mean error of single observation 0.029 0.101 COMMENT. ...

Unno, W. Line Formation of a Normal Zeeman Triplet http://adsabs.harvard.edu/abs/1956PASJ.. ... 108U Moe, Olav Kjeldseth A Generalized Theory for Line Formation in a Homogeneous Magnetic Field http://adsabs.harvard.edu/abs/1968SoPh.. ... 24S Landi Degl'Innocenti, Egidio; Landi Degl'Innocenti, Maurizio Quantum Theory of Line Formation in a Magnetic Field http://adsabs.harvard.edu/abs/1972SoPh.. ... 235H Sazonov, V. N. Polarization in Zeeman-split absorption lines http://adsabs.harvard.edu/abs/1975SvA.. ...

... Все это просим направлять по адресу: 198904 С.-Петербург, Старый Петергоф, Библиотечная пл. 2, Астрономический институт СПбГУ или по электронной почте: viva@pobox.spbu.ru , krivov@astro.spbu.ru и dpa@astro.spbu.ru . Самый же простой вариант -- прислать сообщение прямо отсюда: . ... не обязательно) . ... Тип Вашего сообщения: . ... Текст Вашего сообщения: . ...

... The Secret of the Black Aurora . ... What causes black aurora? These gaps in normal bright aurora are frequently recorded but rarely questioned. ... Near a bright star, clouds of these dust particles scatter short wavelengths of visible starlight more readily than long wavelengths, producing lovely blue reflection nebulae. ... Inspection of NGC 6822 shows several bright star groups, including two dubbed Hubble-X and Hubble-V. Asteroid 1998 WT24 Passes Near Earth . ... Saturnian Aurora . ...

Supernova 2002dv and 2002eg in UGC 11486 . This page is devoted to information on Supernova 2002dv and Supernova 2002eg in UGC 11486 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . ... Ella Sanders discovered this one, the thrid double SN in four months, almost a stastical impossibility. ... SNWeb has a 2002dv page . ... Ella Sanders 2002eg images page 1 and 2002eg images page 2 . ... 2002/07/01.4 . ... Ella Sanders image . ...