Hide Zen home . ... SAI CAS . ... More information: cas=# select sn_name,snt.name, gal_type, gal_type_code, gal_type_code_prec, coalesce((sndist(s)).reldist,0) as rd from sn.sn_cat s, sn.sntypes snt where s.sn_type = snt.id and sn_name='1997C'; sn_name | ... Top 10 relative distances: cas=# select sn_name,snt.name, gal_type, gal_type_code, gal_type_code_prec, coalesce((sndist(s)).reldist,0) as rd from sn.sn_cat s, sn.sntypes snt where s.sn_type = snt.id order by rd desc limit 10; sn_name | ...

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. You can define a file or directory by its location in relation to your current directory . The pathname is given as / (slash) separated list of the directories on the route to the file (or directory) from your current directory. A .. (dot dot) is used to represent the directory immediately above the current directory. In all shells except the Bourne shell, the ~ (tilde) character can be used as shorthand for the full pathname to your home directory. Examples . Did You Know? .

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• Examples of using relative pathnames
• UNIXhelp Glossary - "R"

... A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. The text of the "outer" box (at the end of line 1, halfway into line 2, and halfway into line 3) is shifted upward 12px. The text of the "inner" box, thought shifted upward as well, has been relatively positioned so that it lies in its normal flow position at the end of line 2. ... The lines, as they appear in the image, contain: Start 1 Beginning of body contents. 2 of outer contents. Inner contents. ...

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• Dynamic HTML in Communicator
• Frequency/duration relation.

We investigate the relative importance of starbursts and active galactic nuclei (AGN) in nuclear activities of ultraluminous infrared galaxies (ULIRGs) based on chemodynamical simulations combined with spectrophotometric synthesis codes. We numerically investigate both the gas accretion rates (ARs; m acc ) on to supermassive black holes (SMBHs) and the star formation rates (SFRs; m sf ) in ULIRGs formed by gas-rich galaxy mergers and thereby discuss what powers ULIRGs. ...

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• Integer Indices are 0-relative
• WCSLIB: FITS-WCS and related software

UFO Forum Message . Forums: . ... Post . ... It Really Is Relative . ... Post Message | ... If you are on the Earth the moon does not rotate around its own axis. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... Near, far field and the sky ovverlap at 100 km . Relative strengths of linefeed/yagi sidelobe detections . ... 18 Amin . ... Diameter=(K*lambda)/hpbw (where k depends on the edge taper .. typically k=1.2) The hpbws are different for the linefeed and yagi so their illumination patterns are different. ... At this height, the linefeed is still in the near field while the yagi is in the far field. The angles and distances of the two beams at 100 km are shown below (assuming the far field.. ...

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• http://www.naic.edu/~phil/rfi/fm/fcc_73.317_fmstations.pdf
• http://www.naic.edu/~phil/talks/fast06/talk.pag8
• http://www.naic.edu/~phil/software/datataking/vxworks/help.pnt

Start Data Acquisition - Selected Wavelengths - 22/Apr/2014 16:16:05.216 Observation Type - Target Images - 22/Apr/2014 16:16:05.231 22/Apr/2014 16:16:07.269 Begin Iteration #1 of 2 - Number of Frames : 17 - 22/Apr/2014 16:16:07.286 Filter : 6563 (Position 3) | ... Acquisition Time : 22/Apr/2014 16:16:07.422 | ... ExpTime (sec) : 0.030 | Stokes : I Filter : 6563 (Position 3) | ... Stokes : I Begin Iteration #2 of 2 - Number of Frames : 17 - 22/Apr/2014 16:16:10.023 Filter : 6563 (Position 3) | ...

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• http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2014.1.05/22Apr2014/spectral/GridImages/20140422_162144/log_20140422_162144.txt
• http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2014.1.05/22Apr2014/spectral/TargetImages/20140422_160644/log_20140422_160644.txt
• http://www.arcetri.astro.it/~gcauzzi/SOLARNET/24_april_2014/ibis/GridImages/20140424_181027/log_20140424_181027.txt

... The map shows the distances of the three clumps of galaxies from each other relative to the radio galaxy USS1558-003 located at (0,0). More specifically, the horizontal and vertical axes show relative distances in right ascensions and declinations in arcminute units with respect to the radio galaxy. ... The black dots are all galaxies selected in this field. Magenta dots show old, passively evolving galaxies. ... Large gray circles show the three clumps of galaxies. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE697A649-B990-4F0C-9693-88E72FFCBA78%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B77327F29-F48C-4D4D-964C-0E617716857B%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB971CE61-C842-4AD9-B7FA-6EC8D4E1B573%7D

... In Spiral . Between spiral . ... Center of vortices . ... to density exterema . ...

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• Related usefull links
• Optimization of spectroscopic observations

... 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....

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... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Nuclear activity and environment Effect of environment on AGN is not completely clear yet. ... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Effect of the mass Mass slices ­ optical and radio AGN overall interaction one-on-one interaction relative location 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Stratified study Stratifed study that considers several strata of mass. ...

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• Determination of the relative orientation between radio and dynamical reference
• Some notes on Python relevant to ALMA and ALMA data reduction Bojan Nikolic web
• ALMA-related software engineering topics Bojan Nikolic web pages (r. 329)

... The first column shows the kinematical diagrams, where is the angle between the line of sight on the object and the vector of rotation about Z -axis, and V S is objects line-of-sight velocity relative to an observer at rest at the position of the Sun. The straight lines are regression fits, whose slopes yield the subsystem’s rotation rate. The second column shows the relations between metallicity and distance from the Galactic plane. ... privious figure | next figure . ...

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• Vladimir Marsakov Abstracts
• Doclad, figures
• Population of Galactic globular clusters, figures

... Annals of the Cape observatory. ... 1906QB4_C22v12_____ Informations. relative to: J1-Io: 362, J2-Europe: 246, J3-Ganymede: 130 reference frame: astrometric centre of frame: topocentre epoch of equinox: date time scale: Cape sideral time reduction: no information coordinates: apparent distance, position angle diff. refraction: removed receptor: heliometer telescope: Refractor, F = 2.5 m, D = 17.8 cm observers: Cookson B. data included in standard data file: no Comments. no information Format. ...

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• jg0009
• jg0026
• ji0009

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Time profiles of the mean seasonal and annual relative humidity at Armagh at 09.00 GMT . ... Though a relative humidity series, like all other meteorological series, is essentially local, it will contain elements of variability which derive from a wider region. ... Data: Wet and dry bulb thermometer readings have been recorded daily at Armagh Observatory since 1838. ... Extended abstract in PDF format . ...

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• Armagh Astropark: The Planets
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• SETTING THE SCENE (II)

... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to E-ELT Armazones . ... Green ESO . ... Survey Telescopes . ... Star Clusters . ... Stars@ESO . ... Astronomers have detected a new faint companion to the star HD 3651, already known to host a planet. ... The separations (top) and position angles (bottom) of the companion with respect to the host star is shown here over a three year period. ... Related releases: . ...

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• Location of ESO HQ Relative to Munich | ESO
• Relative Changes with Redshift of the Fine Structure Constant | ESO
• Relative Sizes of the Alpha Centauri Components and other Objects (artistтАЩs

... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Celestial Mechanics
• General Astrometry
• General Astrophysics

The Mars Flag has a different design on the reverse side. obverse side of flag . ... The orbit lines on the obverse cross the Sun on the lower half of the flag and appear to go behind the Sun on the upper half of the flag. The reverse side has the orbits lines continuing around the Sun on the upper half of the flag. ... The Mars Flag reverse side is a continuation of the obverse side and not just a different design on the back and not a mirror image of the obverse. Main Flag Background Color . ...

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• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
• ASP: Sharing the Universe
• ASP: AstroCappella - A Musical Exploration of the Universe

I revisit the Cepheid-distance determination to the nearby spiral galaxy M101 (Pinwheel Galaxy), in light of several recent investigations questioning the shape of the interstellar extinction curve. I find that the (steeper) extinction curve of Fitzpatrick Massa (2007) is slightly favoured relative to the vastly more cited curve of Cardelli et al. (1989), and this consequently increases the inferred distance modulus by ~0.06 mag. ...

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• Observational Techniques: Computer Notes
• Proposed Facility
• Worked Example 02

The geocentric angular distance between magnetic footprints of two satellites in the same time is considered as a criterion of the magnetic conjugations. The situation is identified, as a magnetic conjugation in case as the relative angular distance of the mentioned magnetic footprints is less then 5 deg. ... The output file with name 'xy.cng' contains the information about X and Y satellites magnetic conjugations as a function of the Universal time. ... See the output file description ...

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• mcfile
• INTERBALL IB_TAIL April 2000 during operation scheduling
• IB_AUR February 1997 during operations scheduling

... Mindful of these biases, I can now explore the relations between the measured rotation periods and various other observables. The hypothesis behind monitoring stellar variability is that active stars have asymmetric spot distributions on their photospheres. ... They found that only stars with rotation periods greater than seven days show variations greater than 0.4 magnitudes at I. Bouvier et al . ... 1993a) demonstrated a relation between X--ray flux and spectral type in ZAMS stars. ...

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• The AstroStat Slog relations
• The AstroStat Slog Blog Archive News and related stories
• List of Related Documents