<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>Transition probabilities for [Ni I] and [Ni II] lines.</title>
	<altname type="ADC">J/A+AS/119/99</altname>
		<altname type="CDS">J/A+AS/119/99</altname>
		<altname type="brief">[Ni I] &amp; [Ni II] transition probabilities</altname>
	<reference>
		<source>
<journal>
	<title>Transition probabilities for [Ni I] and [Ni II] lines.</title>
	<author>
			<initial>P</initial>
			<lastName>Quinet</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Le Dourneuf</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>119</volume>
	<pageno>99</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996A&amp;AS..119...99Q</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Atomic_physics.html">Atomic physics</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="atomic_data.html">atomic data</keyword>
			<keyword xlink:href="Ni_I.html">Ni I</keyword>
			<keyword xlink:href="Ni_II.html">Ni II</keyword>
			<keyword xlink:href="transition_probabilities.html">transition probabilities</keyword></keywords>
	<descriptions>
				<description>
				<para>
    New radiative transition probabilities have been calculated for
    forbidden lines of astrophysical interest in Ni I and Ni II. The
    accuracy of the transition probability scales is established on the
    basis of two independent calculations performed with the approximately
    relativistic Hartree-Fock (HFR) and SUPERSTRUCTURE (SST) codes. Both
    physical models take into account the most important configuration
    interaction (CI) and relativistic effects.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table7">
	<title>Radiative transition probabilities, Aki in s-1,
                                 as obtained with HFR and SST for forbidden
                                 lines of Ni I.</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Multiplet</name>
			<definition>Multiplet designation</definition>
			<units>---</units></field>
		<field>
			<name>J-J'</name>
			<definition>J-J'</definition>
			<units>---</units></field>
		<field>
			<name>Lambda</name>
			<definition>Predicted wavelengths from observed
                                    energy levels: see note
	<footnote footnoteId="???"><para>number=1</para>
			<para>Predicted wavelengths are deduced from the observed energy levels
           (Litzen et al. 1993). They are given in air above 200nm and in
           vacuum below 200nm.</para></footnote></definition>
			<units>0.1nm</units></field>
		<field>
			<name>Type</name>
			<definition>Type of transition</definition>
			<units>---</units></field>
		<field>
			<name>Aki(HFR)</name>
			<definition>HFR transition probabilities</definition>
			<units>s-1</units></field>
		<field>
			<name>n_Aki(HFR)</name>
			<definition>Comment on the HFR A-value: see note
	<footnote footnoteId="???"><para>number=2</para>
			<para>* Cancellation effects present.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Aki(SST)</name>
			<definition>SST transition probabilities</definition>
			<units>s-1</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table8">
	<title>Radiative transition probabilities, Aki in s-1,
                                 as obtained with HFR and SST for forbidden
                                 lines of Ni II.</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Multiplet</name>
			<definition>Multiplet designation</definition>
			<units>---</units></field>
		<field>
			<name>2J-2J'</name>
			<definition>2J-2J'</definition>
			<units>---</units></field>
		<field>
			<name>Lambda</name>
			<definition>Predicted wavelengths from observed
                                     energy levels: see note
	<footnote footnoteId="???"><para>number=1</para>
			<para>Predicted wavelengths are deduced from the observed energy levels
          (Sugar and Corliss 1985). They are given in air above 200nm and in
          vacuum below 200nm.</para></footnote></definition>
			<units>0.1nm</units></field>
		<field>
			<name>n_Lambda</name>
			<definition>Comment on the wavelength: see note
	<footnote footnoteId="???"><para>number=2</para>
			<para>+ Calculated HFR wavelength.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Type</name>
			<definition>Type of transition</definition>
			<units>---</units></field>
		<field>
			<name>Aki(HFR)</name>
			<definition>HFR transition probabilities</definition>
			<units>s-1</units></field>
		<field>
			<name>n_Aki(HFR)</name>
			<definition>Comment on the HFR A-value: see note
	<footnote footnoteId="???"><para>number=3</para>
			<para>* Cancellation effects present.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Aki(SST)</name>
			<definition>SST transition probabilities</definition>
			<units>s-1</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Mar</month><day>25</day></date><acknowledgement>Pascal Quinet &lt;pascal@simpa3.univ-rennes1.fr></acknowledgement></ingest>
		</history>
	<identifier>J_A+AS_119_99.xml</identifier></dataset>
