... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

Package . Class . ... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ... These links take you to the next or previous class, interface, package, or related page. ...

... HST . ... Data . ... HST Overview . Overview . ... Cycle 24 Announcement . ... Retrieving HST Data . ... Instruments . ... Grism Spectroscopy . ... UVIS Flats . ... Instrument Handbook . Data Handbook . ... The Wide Field Camera 3 (WFC3) is a fourth-generation UVIS/IR imager aboard the Hubble Space Telescope (HST). WFC3 was installed in May 2009 during HST servicing mission 4, and replaces the Wide Field Planetary Camera 2 (WFPC2). ... ISR 2016-09: WFC3 Cycle 22 Proposal 14007: UVIS Gain . ...

... A top-level object used to access Java classes from within JavaScript code. ... The java , netscape , and sun properties represent the packages java.*, netscape.*, and sun.* respectively. ... For example, you can access a constructor of the Frame class as follows: var theFrame = new Packages.java.awt.Frame(); For convenience, JavaScript provides the top-level netscape , sun , and java objects that are synonyms for the Packages properties with the same names. ... Any class in the Java package sun.* ...

. In this talk we will consider the following problem : which isogeny classes of abelian varieties over a finite field contain the Jacobian of a curves ? We will give the history of this question through the genus 1,2 and 3 cases. This will lead us naturally to a conjecture of Serre on non hyperelliptic genus 3 curves. Moreover we will give a complete answer for the case g=3 over F_2^(2n) . Go to the Laboratoire Poncelet home page. Site design by Paul Zinn-Justin

... Classes . ... Definition at line 87 of file SDSourceHandler.h . ... Definition at line 114 of file SDSourceHandler.h . ... Definition at line 137 of file SDSourceHandler.h . ... Definition at line 116 of file SDSourceHandler.h . ... Definition at line 139 of file SDSourceHandler.h . ... Definition at line 134 of file SDSourceHandler.h . ... Definition at line 117 of file SDSourceHandler.h . ... Definition at line 138 of file SDSourceHandler.h . ... Definition at line 131 of file SDSourceHandler.h . ...

Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... FieldConcatModel Class Reference . Allows for concatinating fields from a model for disply. ... QObject *parent=0) . ... columnCount (const QModelIndex &parent=QModelIndex()) const . ... rowCount (const QModelIndex &parent=QModelIndex()) const . ... This class allows a table model to concatinate fields for the purpose of display. ... home/aw/devel/stellarium/trunk/plugins/LogBook/src/models/ FieldConcatModel.hpp . ...

. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

... Obviously, to subclass GtkWidget , you will have to be familiar with the base class. ... typedef struct _GtkWidgetClass GtkWidgetClass; struct _GtkWidgetClass { GtkObjectClass parent_ class ; guint activate_signal; guint set_scroll_adjustments_signal; /* Basics */ void (* show) ( GtkWidget * widget ); void (* show_all) ( GtkWidget * widget ); void (* hide) ( GtkWidget * widget ); void (* hide_all) ( GtkWidget * widget ); void (* map) ( GtkWidget * widget ); void (* unmap) ( ...

... Home Observing Floyd Bennett Field . ... Lecture Series 2014-2015 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... The new observing location at Floyd Bennett Field is easy for people to find in the dark and will also be within walking distance of the Q35 bus. ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... NamespaceљList . NamespaceљMembers . ... computeObj . ... tcc.axis.computeObj Namespace Reference . ... Compute all computed obj fields from user-specified fields except path generator outputs. ... earth , . ... object data Input fields include all user inputs and current state Ouput fields include all computed fields . ... 3 bools) compute new position for (az, alt, rot) axis, if halted? . ... list tcc.axis.computeObj.__all__ = ["computeObj"] . ...

... Classes . ... Dust :: MMPUV . The radiation field published by Mezger, Mathis and Panagia. ... Inheritance diagram for Dust::MMPUV: . ... Collaboration diagram for Dust::MMPUV: . ... MMPUV (double chi) . These are the methods for the MMPUV class. virtual double . ... double . ... Returns the radiation field of Mezger, Mathis and Panagia ( 1982A&A... ... 372M ) as ammended in the 1983 paper. chi controls the scaling of the field. double Dust::MMPUV::operator() . ... The Specific Energy density. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... This course will provide an overview of some of what is now known about the presence of magnetic fields in stars. ... Lectures: eight lecture hours total, one per week, normally Tuesdays at 11:30 in the Library at Armagh, and Mondays 12 - 1 at QUB in the seminar room. ... Lecture 3, measuring stellar magnetic fields . Lecture 4, stellar magnetic fields and associated phenomena . ... Chapter 1 (Lectures 1 - 4) . ...

... In the presence of only uniform magnetic field B , the motion of a charged particle can be described with gyration about the guiding center and motion along the field line. ... In the precence of both magnetic and electric fields, the equation of motion for charged particle (mass m, charge q) is m d v /dt = q ( E + v x B ). ... Because v is independent of the mass and sign of the charge, it is the same for negatively and positively charged particles, and does not create electric current. ...

... Gallery . ... The Mt Bingar field station and the Catz teleтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . Title: The Mt Bingar field station and the Catz telescope . ... Katz 24" telescope at Stromlo, early 195тАж . Views: 2930 . Katz telescope . Views: 2842 . ... Views: 2691 . Bingar Field Station . Views: 2695 . ... Views: 2721 . ... Views: 2772 . ... Views: 2782 . ... Views: 2711 . ...

... Content Model: PCDATA (i.e. text and entities) . To let users enter more than one line of text, use the TEXTAREA element. ... The text up to the end tag is used to initialize the field's value. ... User agents should tolerate the same range of line terminators within the initialization text. In a typical rendering, the ROWS and COLS attributes determine the visible dimension of the field in characters. ... User agents should allow text to grow beyond these limits by scrolling as needed. ...

... 2 Magnetic Field . ... A magnetized bar has its power concentrated at two ends, its poles ; they are known as its north (N) and south (S) poles, because if the bar is hung by its middle from a string, its N end tends to point northwards and its S end southwards. ... That flow became known as an electric current . ... An electric current produced a magnetic force! ... The fundamental nature of magnetism was not associated with magnetic poles or iron magnets, but with electric currents . ...

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Next: The Evolution of Stars Up: NICMOS Science Previous: A Coronagraphic Search for . ... The NICMOS Parallel program . ... The Stellar Population . ... NICMOS Camera 3 is being used in parallel mode to observe galactic fields at both high and low galactic latitudes. ... Most of the fields are at high galactic latitude; as Figure 1 shows, only 8 pointings are within |b| = 10 o , i.e. the galactic disk. Figure 1: NICMOS parallel fields distribution in galactic latitude. ... Figure 6 ). ...

I-GALFA Survey Fields . ... Most I-GALFA fields are observed by ``nodding'' the telescope north and south along the meridian to trace out a zig-zag pattern on the sky as the Earth rotates. ... The I-GALFA fields fill the AO DEC range and overlap with each other by 20', with one field 3 degrees wide at the zenith and four others 9.3 degrees wide covering the rest of the survey. ... The LST range of each field is shown in blue. ... Field . ... The I-GALFA fields are shown in Galactic coordinates below. ...