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    <title>PFS-JIRA</title>
    <link>https://pfspipe.ipmu.jp/jira</link>
    <description>This file is an XML representation of an issue</description>
    <language>en-us</language>    <build-info>
        <version>8.3.4</version>
        <build-number>803005</build-number>
        <build-date>13-09-2019</build-date>
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<item>
            <title>[INSTRM-1022] Add Subaru-compliant spectroscopy cards</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/INSTRM-1022</link>
                <project id="10300" key="INSTRM">Instrument control development</project>
                    <description>&lt;p&gt;One of the requests from the&#160;PFSA01894911_20200619 comments was to add Subaru-specific spectroscopy cards:&lt;/p&gt;
&lt;div class=&quot;preformatted panel&quot; style=&quot;border-width: 1px;&quot;&gt;&lt;div class=&quot;preformattedContent panelContent&quot;&gt;
&lt;pre&gt;- Spectroscopy keywords
  All spec. keywords are missing in the present header
  While most of them are for slit spectroscopy and may be omitted for PFS,
  (-&amp;gt;needs to update Subaru rule. what other spec instruments do?)
  necessary information such as wavelength range and orientation of dispersion
  should be covered by some basic or instrument-dependent keywords

  WAVELEN
  WAV-MAX
  WAV-MIN
  SLIT
  SLTCPIX1
  SLTCPIX2
  SLT-LEN
  SLT-PA
  SLT-WID
  DISPAXIS
  DISPERSR
 &lt;/pre&gt;
&lt;/div&gt;&lt;/div&gt;
&lt;p&gt;&#160;&lt;/p&gt;

&lt;p&gt;DISPAXIS is easy and I&apos;ll do it right away: 1 for CCDs, 2 for NIR. Note that after DRP IRP the NIR exposures will probably be rotated to have dispersion along columns, to match the CCDs. So the DISPAXIS card would only be valid for raw data.&lt;/p&gt;

&lt;p&gt;I take it we can ignore all the SLit cards. For now, at least.&lt;/p&gt;

&lt;p&gt;For DISPRSR and the three WAV cards can we use names and values from the first measurement paper, which also show up in Yabe-san&apos;s curated tables in spt_exposureTimeCalculator? Those are for the full bandpass (not between the 50% levels of the dichroics, etc.), and will not be good to better than several nm:&lt;/p&gt;

&lt;p&gt;&#160;&lt;/p&gt;
&lt;div class=&apos;table-wrap&apos;&gt;
&lt;table class=&apos;confluenceTable&apos;&gt;&lt;tbody&gt;
&lt;tr&gt;
&lt;th class=&apos;confluenceTh&apos;&gt;Arm&lt;/th&gt;
&lt;th class=&apos;confluenceTh&apos;&gt;Wavelength range&lt;/th&gt;
&lt;th class=&apos;confluenceTh&apos;&gt;Central Wavelength&lt;/th&gt;
&lt;th class=&apos;confluenceTh&apos;&gt;Fringe frequency&lt;/th&gt;
&lt;/tr&gt;
&lt;tr&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;Blue&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;380-650 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;519 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;711 mm^-1&lt;/td&gt;
&lt;/tr&gt;
&lt;tr&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;Red&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;630-970 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;805 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;557 mm^-1&lt;/td&gt;
&lt;/tr&gt;
&lt;tr&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;NIR&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;940-1260 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;1107 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;570 mm^-1&lt;/td&gt;
&lt;/tr&gt;
&lt;tr&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;Med&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;710-885 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;799 nm&lt;/td&gt;
&lt;td class=&apos;confluenceTd&apos;&gt;1007 mm^-1&lt;/td&gt;
&lt;/tr&gt;
&lt;/tbody&gt;&lt;/table&gt;
&lt;/div&gt;


&lt;p&gt;In particular, for the WAVELEN card can we just use the central wavelength of the bandpass, or will we need to figure out which wavelength falls on the central row/column? The NAOJ examples have values down to 0.001 nm, which worries me&#160;&lt;/p&gt;

&lt;p&gt;We need some convention for DISPRSR. A proposal, based on the NAOJ example would be &quot;VPH_$fringesPerMm_$centralWave&quot;? Add &quot;low&quot; vs &quot;high&quot; for red? I.e &quot;VPH_711_519nm&quot; or &quot;VPH_low_557_805nm&quot;? The red medium assembly is slightly different (adds prisms) but does it matter?&lt;/p&gt;

&lt;p&gt;&#160;&lt;/p&gt;</description>
                <environment></environment>
        <key id="14527">INSTRM-1022</key>
            <summary>Add Subaru-compliant spectroscopy cards</summary>
                <type id="3" iconUrl="https://pfspipe.ipmu.jp/jira/secure/viewavatar?size=xsmall&amp;avatarId=10518&amp;avatarType=issuetype">Task</type>
                                            <priority id="10000" iconUrl="https://pfspipe.ipmu.jp/jira/images/icons/priorities/medium.svg">Normal</priority>
                        <status id="10002" iconUrl="https://pfspipe.ipmu.jp/jira/images/icons/statuses/generic.png" description="The issue is resolved, reviewed, and merged">Done</status>
                    <statusCategory id="3" key="done" colorName="green"/>
                                    <resolution id="10000">Done</resolution>
                                        <assignee username="cloomis">cloomis</assignee>
                                    <reporter username="cloomis">cloomis</reporter>
                        <labels>
                            <label>FITS</label>
                            <label>SPS</label>
                    </labels>
                <created>Mon, 22 Jun 2020 21:33:43 +0000</created>
                <updated>Tue, 16 Feb 2021 18:25:58 +0000</updated>
                            <resolved>Tue, 16 Feb 2021 17:59:41 +0000</resolved>
                                                                    <component>ics_ccdActor</component>
                    <component>ics_hxActor</component>
                        <due></due>
                            <votes>0</votes>
                                    <watches>1</watches>
                                                                <comments>
                            <comment id="18450" author="cloomis" created="Mon, 8 Feb 2021 21:06:06 +0000"  >&lt;p&gt;Since DISPRSR is just a string but might be generated or parsed I went for f&quot;VPH_&lt;/p&gt;
{arm}
&lt;p&gt;_&lt;/p&gt;
{int(fringePerMm)}
&lt;p&gt;_&lt;/p&gt;
{int(wavemid)}
&lt;p&gt;nm&quot;. &lt;/p&gt;

&lt;p&gt;A complete example for a blue exposure:&lt;/p&gt;

&lt;div class=&quot;preformatted panel&quot; style=&quot;border-width: 1px;&quot;&gt;&lt;div class=&quot;preformattedContent panelContent&quot;&gt;
&lt;pre&gt;DISPAXIS=                    2 / Dispersion axis (along columns)
DISPRSR = &apos;VPH_b_711_519nm&apos;      / Disperser name (arm_fringe/mm_centralNm)
WAV-MIN =                 380. / [nm] Blue edge of the bandpass
WAV-MAX =                 650. / [nm] Red edge of the bandpass
WAVELEN =                 519. / [nm] Middle of the bandpass
&lt;/pre&gt;
&lt;/div&gt;&lt;/div&gt;

&lt;p&gt;Is that OK, &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/secure/ViewProfile.jspa?name=furu&quot; class=&quot;user-hover&quot; rel=&quot;furu&quot;&gt;Hisanori Furusawa&lt;/a&gt;?&lt;/p&gt;</comment>
                            <comment id="18525" author="cloomis" created="Tue, 16 Feb 2021 17:59:41 +0000"  >&lt;p&gt;pfs_utils merged at b534453, tagged 5.2.6&lt;br/&gt;
ics_ccdActor merged at 847ffee, tagged 1.6.15&lt;/p&gt;</comment>
                    </comments>
                <issuelinks>
                            <issuelinktype id="10003">
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                                            <outwardlinks description="relates to">
                                        <issuelink>
            <issuekey id="13202">INSTRM-578</issuekey>
        </issuelink>
            <issuelink>
            <issuekey id="14528">INSTRM-1023</issuekey>
        </issuelink>
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