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Revision 92023-08-04 - MichaelCoughlin

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Submission of publications to the Publication Board

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  1. Does the manuscript cite Bellm et al. 2019, Graham et al. 2019, Dekany et al. 2020, Masci et al. 2019 and any additionally relevant instrument papers from the tables below (if it does not, please add the required citations): <yes|no>
  2. If you made use of SEDM data, did you acknowledge it (see 'Acknowledgement' section for the text) and cite Blagorodnova et al. 2018 and Rigault et al. 2019? (If you used IFU data after March 2020, cite Kim et al. 2022) <yes|no>
  3. If you made use of AMPEL, did you acknowledge it and cite Nordin et al 2019? <yes|no>
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  1. If you made use of Kowalski/Fritz, did you acknowledge it and cite van Der Walt et al. 2019 and Coughlin et al 2023? <yes|no>
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  1. If you made use of Kowalski/Fritz, did you acknowledge it and cite van Der Walt et al. 2019 and Coughlin et al 2023? <yes|no>
 
  1. Is this manuscript extremely time sensitive (if yes, please e-mail the Project Scientist directly)?: <no|yes>

Builders list

Revision 82023-05-23 - MichaelCoughlin

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  The ZTF forced-photometry service was funded under the Heising-Simons Foundation grant #12540303 (PI: Graham).
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-- Iva Kostadinova - 2021-05-18
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If you made use of Kowalski/Fritz, please add:

The Gordon and Betty Moore Foundation, through both the Data-Driven Investigator Program and a dedicated grant, provided critical funding for SkyPortal.

 

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Revision 72023-05-02 - MichaelCoughlin

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Submission of publications to the Publication Board

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  1. Have you made sure the standard acknowledgement is in your manuscript and up-to-date (if it does not, please add/update it): <yes|no>
  2. Does the manuscript cite Bellm et al. 2019, Graham et al. 2019, Dekany et al. 2020, Masci et al. 2019 and any additionally relevant instrument papers from the tables below (if it does not, please add the required citations): <yes|no>
  3. If you made use of SEDM data, did you acknowledge it (see 'Acknowledgement' section for the text) and cite Blagorodnova et al. 2018 and Rigault et al. 2019? (If you used IFU data after March 2020, cite Kim et al. 2022) <yes|no>
Changed:
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  1. If you made use of AMPEL, did you acknowledge it and cite Nordin et al 2019 and Soumagnac & Ofek 2019? <yes|no>
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  1. If you made use of AMPEL, did you acknowledge it and cite Nordin et al 2019? <yes|no>
  2. If you made use of Kowalski/Fritz, did you acknowledge it and cite van Der Walt et al. 2019 and Coughlin et al 2023? <yes|no>
 
  1. Is this manuscript extremely time sensitive (if yes, please e-mail the Project Scientist directly)?: <no|yes>

Builders list

Revision 62022-09-07 - MatthewGraham

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Submission of publications to the Publication Board

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Builders list

When a paper is submitted to the Publication Board for review, the lead author should also solicit from the leads of each of the listed subsystems (BuildersListLeads) the names to include. Builders must opt in and in doing so, it is understood that they will read the relevant parts of the paper. Not responding beyond a cutoff date will be taken to mean that the builder in question is not interested in being an author.

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Acknowledgement

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All ZTF papers should carry the following acknowledgements (any involving data taken prior to Dec 1, 2020):
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All ZTF papers should carry the following acknowledgments

If data is taken prior to Dec 1, 2020:

 

Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute of Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW.

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 If data is used taken after Dec 1, 2020:
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Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute of Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, France, the University of Warwick, the University of Bochum, and Northwestern University. Operations are conducted by COO, IPAC, and UW.
>
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Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute of Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, University of Warwick, Ruhr University Bochum and Northwestern University. Operations are conducted by COO, IPAC, and UW.

NOTE: If your paper uses data from a period both prior and after Dec 1, 2020, please combine the two acknowledgments in the following manner:

Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grants No. AST-1440341 and AST-2034437 and a collaboration including current partners Caltech, IPAC, the Weizmann Institute of Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, University of Warwick, Ruhr University Bochum, Northwestern University and former partners the University of Washington, Los Alamos National Laboratories, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW.

 

Additionally, if your paper includes data from SEDM, please add:

Revision 52022-06-01 - MatthewGraham

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META TOPICPARENT name="WebHome"

Submission of publications to the Publication Board

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  1. Have you invited eligible builders as co-authors (if yes, list which subsystems. If not, explain why not)?: <list invited subsystems>
  2. Have you made sure the standard acknowledgement is in your manuscript and up-to-date (if it does not, please add/update it): <yes|no>
  3. Does the manuscript cite Bellm et al. 2019, Graham et al. 2019, Dekany et al. 2020, Masci et al. 2019 and any additionally relevant instrument papers from the tables below (if it does not, please add the required citations): <yes|no>
Changed:
<
<
  1. If you made use of SEDM data, did you acknowledge it (see 'Acknowledgement' section for the text) and cite Blagorodnova et al. 2018 and Rigault et al. 2019? <yes|no>
>
>
  1. If you made use of SEDM data, did you acknowledge it (see 'Acknowledgement' section for the text) and cite Blagorodnova et al. 2018 and Rigault et al. 2019? (If you used IFU data after March 2020, cite Kim et al. 2022) <yes|no>
 
  1. If you made use of AMPEL, did you acknowledge it and cite Nordin et al 2019 and Soumagnac & Ofek 2019? <yes|no>
  2. Is this manuscript extremely time sensitive (if yes, please e-mail the Project Scientist directly)?: <no|yes>

Revision 42022-03-06 - IvaKostadinova

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Submission of publications to the Publication Board

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 All ZTF papers should carry the following acknowledgements (any involving data taken prior to Dec 1, 2020):
Changed:
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Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW.
>
>
Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute of Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW.
 

If data is used taken after Dec 1, 2020:

Changed:
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<
Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, France, the University of Warwick, the University of Bochum, and Northwestern University. Operations are conducted by COO, IPAC, and UW.
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Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute of Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, France, the University of Warwick, the University of Bochum, and Northwestern University. Operations are conducted by COO, IPAC, and UW.
 

Additionally, if your paper includes data from SEDM, please add:

Revision 32021-12-08 - MatthewGraham

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Submission of publications to the Publication Board

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 If data is used taken after Dec 1, 2020:
Changed:
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Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, and IN2P3, France. Operations are conducted by COO, IPAC, and UW.
>
>
Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, France, the University of Warwick, the University of Bochum, and Northwestern University. Operations are conducted by COO, IPAC, and UW.
 

Additionally, if your paper includes data from SEDM, please add:

Revision 22021-09-27 - StevenStetzler

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Submission of publications to the Publication Board

Revision 12021-05-18 - IvaKostadinova

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META TOPICPARENT name="WebHome"

Submission of publications to the Publication Board

To submit a paper for review by the Publication Board, add the draft PDF to the relevant section on this page and e-mail the following check-list with your answers to ztf-pubboard@lists.astro.caltech.edu

Pre-submission check-list (please copy and paste it into your e-mail, with answers):

  1. Is the paper ready to be submitted to the journal (all sections finished, checked for typos, no remaining TBDs, etc.; if no, stop and finalize it before submitting to the PubBoard): <yes|no>
  2. Have you attached the PDF of your manuscript to this page, and added a row in the appropriate table below (if no, stop and attach/add it): <yes|no>
  3. Have you attached the PDF of your manuscript to this e-mail (if no, stop and attach it): <yes|no>
  4. Has the manuscript been shared with all co-authors (if no, stop and share with co-authors): <yes|no>
  5. Do you have permission to use all data used in the manuscript? E.g. if relying on follow-up data found on the Marshal (or other collaboration tools or mailing lists) co-authorship must be offered to the people/groups who originated them: <yes|no>
  6. Has the manuscript been shared with and approved by the relevant Science Working Group?: <yes|no>
  7. Does the PDF come with line numbers (if no, please add them ( see here how) unless it's extremely difficult to do so): <yes|no>
  8. Have you invited eligible builders as co-authors (if yes, list which subsystems. If not, explain why not)?: <list invited subsystems>
  9. Have you made sure the standard acknowledgement is in your manuscript and up-to-date (if it does not, please add/update it): <yes|no>
  10. Does the manuscript cite Bellm et al. 2019, Graham et al. 2019, Dekany et al. 2020, Masci et al. 2019 and any additionally relevant instrument papers from the tables below (if it does not, please add the required citations): <yes|no>
  11. If you made use of SEDM data, did you acknowledge it (see 'Acknowledgement' section for the text) and cite Blagorodnova et al. 2018 and Rigault et al. 2019? <yes|no>
  12. If you made use of AMPEL, did you acknowledge it and cite Nordin et al 2019 and Soumagnac & Ofek 2019? <yes|no>
  13. Is this manuscript extremely time sensitive (if yes, please e-mail the Project Scientist directly)?: <no|yes>

Builders list

When a paper is submitted to the Publication Board for review, the lead author should also solicit from the leads of each of the listed subsystems (BuildersListLeads) the names to include. Builders must opt in and in doing so, it is understood that they will read the relevant parts of the paper. Not responding beyond a cutoff date will be taken to mean that the builder in question is not interested in being an author.

Acknowledgement

All ZTF papers should carry the following acknowledgements (any involving data taken prior to Dec 1, 2020):

Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW.

If data is used taken after Dec 1, 2020:

Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, and IN2P3, France. Operations are conducted by COO, IPAC, and UW.

Additionally, if your paper includes data from SEDM, please add:

SED Machine is based upon work supported by the National Science Foundation under Grant No. 1106171

If your analysis has made use of the forced photometry service, please add:

The ZTF forced-photometry service was funded under the Heising-Simons Foundation grant #12540303 (PI: Graham).

-- Iva Kostadinova - 2021-05-18

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