{"id":2428,"date":"2015-03-23T13:59:15","date_gmt":"2015-03-23T23:59:15","guid":{"rendered":"http:\/\/www.eaobservatory.org\/jcmt\/?page_id=2428"},"modified":"2017-01-25T13:23:26","modified_gmt":"2017-01-25T23:23:26","slug":"cfp15b","status":"publish","type":"page","link":"https:\/\/www.eaobservatory.org\/jcmt\/proposals\/cfp15b\/","title":{"rendered":"Call for Proposals &#8211; 15B"},"content":{"rendered":"<h3 style=\"text-align: center\">Semester 15B<\/h3>\n<hr size=\"4\" \/>\n<p><a name=\"submission\"><\/a><\/p>\n<h3>Submission Deadline:<\/h3>\n<h4 style=\"text-align: center\">For telescope time in<\/h4>\n<h4 style=\"text-align: center\">Semester 15B (1st August 2015\u00a0 &#8211; 31st January 2016)<\/h4>\n<h4 style=\"text-align: center\">the closing date for receipt of proposals is<\/h4>\n<h4 style=\"text-align: center\"><span style=\"color: red\">Friday 15 May 2015<\/span><\/h4>\n<h3 style=\"text-align: center\"><span style=\"color: red\">15:00 Hawaiian Standard Time<\/span><\/h3>\n<ul>\n<li>Applicants from the University of Hawaii may have a different deadline.<\/li>\n<\/ul>\n<hr size=\"4\" \/>\n<h3><span style=\"color: blue\">NEWS for 15B<\/span><\/h3>\n<ul>\n<li>This is the second semester for JCMT operating under the management of the East Asian Observatories, and again EAO invites observing proposals from users in its partner regions (China, Japan, South Korea, Taiwan), as well as from members of the contributing consortia in the UK and Canada. Proposals are not yet being invited from the wider &#8216;International&#8217; community. Click <span style=\"color: #3366ff\"><a style=\"color: #3366ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/proposals\/EAO_eligibility\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/proposals\/EAO_eligibility\/\" target=\"_blank\">here<\/a><\/span> to see if you are eligible to submit as PI.<\/li>\n<li>There is a limit of a maximum of 200 hours that may be requested per proposal and\u00a0each proposal should aim to be completed during the semester.<\/li>\n<li>Survey proposals (large programs spanning more than 200 hours and requiring more than one semester to complete) are not solicited in this Call. A separate Call for JCMT Surveys will be announced in mid-May and assessed separately. These programs will be considered for observing starting at a later date, to be announced in the survey call.<\/li>\n<li>The Time Allocation Committee for JCMT will assess each PI proposal for scientific merit and will rank and approve observing time accordingly.<\/li>\n<li>We encourage multi-national collaboration, and projects which request the heterodyne instruments and\/or weather bands 4 and 5. A description of how time will be distributed for collaborative projects is <a href=\"http:\/\/www.eaobservatory.org\/jcmt\/proposals\/collaborations\/\">here<\/a>.<\/li>\n<li>Proposal submission is via <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" href=\"http:\/\/northstar.eaobservatory.org\">Northstar<\/a><\/span> and applicants are requested to use the sections of the Northstar form regarding Flexible Observing to express\u00a0their willingness and ability to travel and observe.\u00a0If unable to travel themselves, applicants will be able to consult with the observatory to make alternative arrangements. As the JCMT operates flexible observing, it is important to note that data can be obtained for a project even without the P.I.\/observer&#8217;s attendance at the telescope.<\/li>\n<li>POL-2 and FTS-2 are <b>not<\/b> being offered in this <i>Call<\/i>.<\/li>\n<\/ul>\n<h3>Important Notes<\/h3>\n<ul>\n<li>There is only one &#8216;queue&#8217; in semester 15B &#8211; labelled &#8216;<i>International<\/i>&#8216; on the Northstar application form. The science and technical case should be limited to 2 pages; another page is available for figures &amp; tables.<\/li>\n<li>Applicants are urged to itemize explicitly, in the Technical section of the proposal, their inputs to their integration time calculations. Output from the SCUBA-2 ITC can\/should be copied&amp;paste-d. This will allow the assigned Technical Assessor to confirm the proposal&#8217;s feasibility.<\/li>\n<li>We encourage use of the <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" href=\"http:\/\/www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca\/en\/jcmt\/\">CADC<\/a><\/span> database to check for previous observations that might satisfy your program needs (see p8 of the talk given at the <a title=\"http:\/\/www.eaobservatory.org\/JCMT\/workshops\/Jan-2015\/JCMT-ideas-to-data-1.pdf\" href=\"http:\/\/www.eaobservatory.org\/JCMT\/workshops\/Jan-2015\/JCMT-ideas-to-data-1.pdf\"><span style=\"color: #0000ff\">January workshops<\/span><\/a> and our <a href=\"http:\/\/www.eaobservatory.org\/jcmt\/science\/archive\/\"><span style=\"color: #0000ff\">JSA<\/span><\/a> pages).<\/li>\n<li>JCMT normally operates a 12-hour night, running from approximately 7:30pm to 7:30am HST.\u00a0 <a title=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/a-semester\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/a-semester\/\"><span style=\"color: #0000ff\">Table A<\/span><\/a> and <a title=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/b-semester\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/b-semester\/\"><span style=\"color: #0000ff\">Table B<\/span><\/a> show source transit times during (roughly) the first and seconds halves of the year.<\/li>\n<li>Your proposal must specify the weather conditions (read <i>opacity<\/i>) that it requires or can tolerate.<br \/>\nThe amount of time available per weather\/opacity band <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/weather-bands#opacity\">varies through the year<\/a><\/span>.<\/li>\n<li>A summary of the telescope and its operations was given at the <a title=\"http:\/\/www.eaobservatory.org\/jcmt\/help\/workshops\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/help\/workshops\/\"><span style=\"color: #0000ff\"> <b>January Workshops<\/b><\/span><\/a><\/li>\n<\/ul>\n<hr \/>\n<h3><div id=\"toc_container\" class=\"no_bullets\"><p class=\"toc_title\">Contents<\/p><ul class=\"toc_list\"><li><a href=\"#Available_Instrumentation_and_Observing_Modes\"><span class=\"toc_number toc_depth_1\">1<\/span> Available Instrumentation and Observing Modes<\/a><\/li><li><a href=\"#Calculating_Integration_Times\"><span class=\"toc_number toc_depth_1\">2<\/span> Calculating Integration Times<\/a><\/li><li><a href=\"#Proposal_Submission\"><span class=\"toc_number toc_depth_1\">3<\/span> Proposal Submission<\/a><\/li><li><a href=\"#Flexible_Scheduling\"><span class=\"toc_number toc_depth_1\">4<\/span> Flexible Scheduling<\/a><\/li><li><a href=\"#The_JCMT_Users_e-mail_exploder\"><span class=\"toc_number toc_depth_1\">5<\/span> The JCMT Users e-mail exploder:<\/a><\/li><\/ul><\/div>\n<\/h3>\n<h3><span id=\"Available_Instrumentation_and_Observing_Modes\">Available Instrumentation and Observing Modes<\/span><\/h3>\n<p>The current status and availability of the JCMT instrument suite is <a title=\"Instrumentation\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\">here.<\/a><\/p>\n<p><b>Continuum Receivers<\/b> &#8211;<\/p>\n<ul>\n<li><span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/continuum\/scuba-2\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/continuum\/scuba-2\/\">SCUBA-2<\/a><\/span> (simultaneous 450\u00b5m &amp; 850\u00b5m imaging)<\/li>\n<\/ul>\n<p><b>Heterodyne Receivers<\/b> &#8211;<a title=\"Heterodyne Receivers\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/\"> <span style=\"color: #0000ff\">General\u00a0overview<\/span><\/a><\/p>\n<ul>\n<li><span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/rxa\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/rxa\/\"> RxA3<\/a><\/span> (211-272 GHz) &#8211; has a single receptor.<\/li>\n<li><span style=\"color: #0000ff\"> <a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/harp\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/harp\/\"> HARP<\/a><\/span> (325-375 GHz) &#8211; is a 16-element B-band array.<\/li>\n<\/ul>\n<p><b>Heterodyne Backend<\/b><\/p>\n<ul>\n<li><b>ACSIS<\/b> &#8211; <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/acsis\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/acsis\/\"> Available bandwidths, spectral resolutions and backend modes<\/a><\/span>.\n<ul>\n<li>The ACSIS correlating spectrometer is a highly flexible backend; it was designed to work with HARP, but it works with all our heterodyne receivers.<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>Several <a title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/observing-modes\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/observing-modes\/\"><span style=\"color: #0000ff\">modes of heterodyne observing<\/span><\/a> and several switching schemes are supported.<\/p>\n<p>See also the Instrumentation summary from the <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" href=\"http:\/\/www.eaobservatory.org\/JCMT\/workshops\/Jan-2015\/JCMT-Instruments.pdf\"> <b>January Workshops<\/b><\/a><\/span><\/p>\n<hr \/>\n<h3><\/h3>\n<h3><span id=\"Calculating_Integration_Times\">Calculating Integration Times<\/span><\/h3>\n<p>Integration time calculators or formulae are available, for<\/p>\n<ul>\n<li>Heterodyne receivers : <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/itc\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/itc\/\">HITEC<\/a><\/span> (the <b>H<\/b>eterodyne <b>I<\/b>ntegration <b>T<\/b>im<b>E C<\/b>alculator),<\/li>\n<li><span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/continuum\/scuba-2\/itc\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/continuum\/scuba-2\/itc\/\">SCUBA-2<\/a><\/span> (<span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/continuum\/scuba-2\/time-and-sensitivity\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/continuum\/scuba-2\/time-and-sensitivity\/\"> Formulae<\/a><\/span>)<\/li>\n<\/ul>\n<p>They should be used to calculate the integration time needed to reach a given RMS per channel or beam or output-map pixel as a function of receiver, frequency, observing mode, elevation and sky opacity.<\/p>\n<p>The JCMT Observing Tool (<span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/omp\/observing-tool\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/observing\/omp\/observing-tool\/\">JCMTOT<\/a><\/span>) gives equivalent results for all instruments.<\/p>\n<ul>\n<li><b>Overheads for pointing, focussing, and calibrations should not be added to the time request. These activities will be accounted for separately. <\/b>Calibration observations (eg. focus, pointing, flux calibrators) and other unavoidable overheads (eg receiver tuning) are no longer charged to science projects and instead are charged to an observatory accounting code. There is therefore no need for applicants to provide calibration overhead estimates in their proposals.The observatory will perform regular and appropriate calibration observations to ensure that all science data obtained are sensibly calibrated.\n<ul>\n<li><span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/\"> Spectroscopically<\/a><\/span>, this involves observations of one of our <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/calibration\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/calibration\/\"> Spectral Line Standards<\/a><\/span> at one of about ten different <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/calibration\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/heterodyne\/calibration\/\"> standard line frequencies <\/a><\/span>. If your programme frequency is one of these, then you&#8217;re decidely in luck. In any case, the calibration allows you to assess the performance of the instrument. We will perform such an observation at least once per programme unless a previous calibration is still appropriate, and more often if circumstances change or if more than a couple of hours pass.<\/li>\n<li>For continuum work, continuum calibrators will be observed at both operational wavelengths of SCUBA-2 (450\u00b5m, 850\u00b5m) at appropriate times and airmass to meet the general needs of the science programmes.<\/li>\n<\/ul>\n<p>If a proposal demands more unusual or more frequent calibrations then this needs to be clearly stated in the proposal and the time for these calibrations requested explicitly. If you have queries about what our default calibrations might be or what extra overheads are generated by your calibration requirements please get in touch with us.<\/li>\n<\/ul>\n<hr \/>\n<p>&nbsp;<\/p>\n<h3><span id=\"Proposal_Submission\">Proposal Submission<\/span><\/h3>\n<p><span style=\"color: #0000ff\">Northstar<\/span> is now available for submissions. All users are advised to <a href=\"http:\/\/northstar.eaobservatory.org\/\"><b>register, check and\/or update their accounts<\/b><\/a>. As mentioned in our <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" title=\"http:\/\/www.eaobservatory.org\/jcmt\/proposals\/northstar\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/proposals\/northstar\/\"> Help page<\/a><\/span>, you may, at first, have to accept the server certificate to gain access to Northstar. Except for the University of Hawaii, all proposals should be submitted<\/p>\n<p style=\"text-align: center\"><span style=\"color: #0000ff\"><a style=\"color: #0000ff\" href=\"http:\/\/northstar.eaobservatory.org\/\">HERE<\/a><\/span>.<\/p>\n<p>If you already have a Northstar account you can login now! &#8211; new users should first register. Applicants should avoid using font sizes that are excessively <span style=\"font-size: x-large\">small<\/span>.<\/p>\n<p>&nbsp;<\/p>\n<p><em>It is important that all applicants (PI &amp; CoIs) and their <strong>national affiliations<\/strong> are listed on the proposal, so that an assessment can be made of how much observing time is being used by each partner organization. We suggest that you edit your Northstar profile to include, eg<br \/>\n<\/em><\/p>\n<p><em>\u00a0\u00a0\u00a0\u00a0\u00a0 REMARK : Affiliation = China (or Japan or Taiwan or South Korea or UK or Canada)<br \/>\n<\/em><\/p>\n<hr \/>\n<h3><\/h3>\n<h3><span id=\"Flexible_Scheduling\">Flexible Scheduling<\/span><\/h3>\n<p>The overall philosophy of observing at JCMT is to match observing programmes to the weather. A summary was given at the <span style=\"color: #0000ff\"><a style=\"color: #0000ff\" href=\"http:\/\/www.eaobservatory.org\/JCMT\/workshops\/Jan-2015\/JCMT-Operations.pdf\"> <b>January Workshops<\/b><\/a><\/span> and new guidelines will appear here soon.<\/p>\n<hr \/>\n<h3><\/h3>\n<h3><span id=\"The_JCMT_Users_e-mail_exploder\">The JCMT Users e-mail exploder:<\/span><\/h3>\n<p>From time to time, subscribers to the &#8216;jcmt_users&#8217; email list will receive notices on the status of the JCMT, call for proposals, etc. To subscribe, please send email to <span style=\"color: #ff00ff\">jcmt_users+subscribe@eaobservatory.org<\/span> (no particular Subject or content is required).<\/p>\n<hr size=\"4\" \/>\n<h3>And Finally:<\/h3>\n<p>If you&#8217;ve read all this and still have questions about the scheduling, the submission deadlines, the procedures, etc &#8211; please contact the <a title=\"http:\/\/www.eaobservatory.org\/jcmt\/help\/\" href=\"http:\/\/www.eaobservatory.org\/jcmt\/help\/\">helpdesk<\/a> &#8211; or <a href=\"mailto:i.coulson@eaobservatory.org\">me<\/a>.<\/p>\n<p>Iain Coulson<br \/>\nJCMT Scheduler<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Semester 15B Submission Deadline: For telescope time in Semester 15B (1st August 2015\u00a0 &#8211; 31st January 2016) the closing date for receipt of proposals is Friday 15 May 2015 15:00 Hawaiian Standard Time Applicants from the University of Hawaii may have a different deadline. NEWS for 15B This is the\u2026 <a class=\"continue-reading-link\" href=\"https:\/\/www.eaobservatory.org\/jcmt\/proposals\/cfp15b\/\">Continue reading<\/a><\/p>\n","protected":false},"author":7,"featured_media":0,"parent":192,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/2428"}],"collection":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/users\/7"}],"replies":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/comments?post=2428"}],"version-history":[{"count":31,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/2428\/revisions"}],"predecessor-version":[{"id":6429,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/2428\/revisions\/6429"}],"up":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/192"}],"wp:attachment":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/media?parent=2428"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}