Extended Figures

Capture extended figures using a <fig> element with a @fig-type attribute of value extended.

Capture each of the individual image files in <graphic> elements.

The <fig> must contain the following as children of the <caption> element:
  • The linking text that appears in the print version in a <p> element with a @content-type attribute of value print.
  • The linking text that appears in the online version in a <p> element with a @content-type attribute of value online.

Optionally an <inline-supplementary-material> may be used as a child of <caption> to capture the file name of the tar of the figure set (see Inline Supplementary Data).

Example

<fig fig-type="extended" id="apjaa6032f4" position="float">
  <label>Figure 4.</label>
  <caption id="apjaa6032fc4">
    <p>Globally integrated infrared/submillimeter spectral energy
    distributions for all the galaxies in the KINGFISH/SINGS sample,
    sorted by R.A. The following symbols are used: filled circles
    (<italic>Herschel</italic>), triangles (<italic>GALEX</italic>,
    2MASS, and <italic>WISE</italic>), open circles
    (<italic>Spitzer</italic> and <italic>Planck</italic>), and squares
    (<italic>BVR</italic>
    <sub>C</sub>
    <italic>I</italic>
    <sub>C</sub> and <italic>ugriz</italic> and SCUBA). Arrows indicate
    5<italic>σ</italic> upper limits (and lower limits in the case of
    NGC 3034). The solid curve is the sum of a 5000 K stellar blackbody
    (short dashed) along with models of dust emission from PDRs (dotted;
    <italic>U</italic> > <italic>U</italic>
    <sub>min</sub>) and the diffuse interstellar medium (long dashed;
    <italic>U</italic> = <italic>U</italic>
    <sub>min</sub>). The fitted parameters from these Draine &amp; Li
    (<xref ref-type="bibr" rid="apjaa6032bib16">2007</xref>) 3.6–500
    <italic>μ</italic>m model fits are listed within each panel along
    with the reduced <italic>χ</italic>
    <sup>2</sup> (see Section <xref ref-type="sec" rid="apjaa6032s4-2">4.2</xref> for details). While the plotted data are corrected for
    Galactic extinction, the fluxes tabulated in Table <xref ref-type="table" rid="apjaa6032t2">2</xref> are not corrected. The
  uncertainties are smaller than the symbols plotted. There are no SED
  fits in cases where the far-infrared photometry provides only
  limits.</p>
    <p content-type="print">(An extended version of this figure is available in the <ext-link xlink:href="https://doi.org/10.3847/1538-4357/aa6032">online article</ext-link>.)</p>                          
    <p content-type="online">
      <inline-supplementary-material>(An extended
    version of this figure is
    available.)</inline-supplementary-material>
    </p>
    <p content-type="numparts">1 of 9 images.</p>
  </caption>
  <graphic content-type="print" id="apjaa6032f4_eps" xlink:href="apjaa6032f4.eps"/>
  <graphic content-type="online" id="apjaa6032f4_lr" xlink:href="apjaa6032f4_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_a_lr" xlink:href="apjaa6032f4_a_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_b_lr" xlink:href="apjaa6032f4_b_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_c_lr" xlink:href="apjaa6032f4_c_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_d_lr" xlink:href="apjaa6032f4_d_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_e_lr" xlink:href="apjaa6032f4_e_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_f_lr" xlink:href="apjaa6032f4_f_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_g_lr" xlink:href="apjaa6032f4_g_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_h_lr" xlink:href="apjaa6032f4_h_lr.jpg"/>
  <graphic content-type="online" id="apjaa6032f4_i_lr" xlink:href="apjaa6032f4_i_lr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_a_hr" xlink:href="apjaa6032f4_a_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_b_hr" xlink:href="apjaa6032f4_b_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_c_hr" xlink:href="apjaa6032f4_c_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_d_hr" xlink:href="apjaa6032f4_d_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_e_hr" xlink:href="apjaa6032f4_e_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_f_hr" xlink:href="apjaa6032f4_f_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_g_hr" xlink:href="apjaa6032f4_g_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_h_hr" xlink:href="apjaa6032f4_h_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_i_hr" xlink:href="apjaa6032f4_i_hr.jpg"/>
  <graphic content-type="high" id="apjaa6032f4_hr" xlink:href="apjaa6032f4_hr.jpg"/>
</fig>