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1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are | ||||||||
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(1.2) Long acknowledgement statement (optional) (can be used in all scientific articles or papers appearing in scientific, technical or professional journals instead of the short statement) | ||||||||
Changed: | ||||||||
< < | "This work was supported by the GROWTH (Global Relay of Observatories Watching Transients Happen) project funded by the National Science Foundation under PIRE Grant No 1545949. GROWTH is a collaborative project among California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), Liverpool John Moores University (UK)." | |||||||
> > | "This work was supported by the GROWTH (Global Relay of Observatories Watching Transients Happen) project funded by the National Science Foundation under PIRE Grant No 1545949. GROWTH is a collaborative project among California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Indian Institute of Technology Bombay (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), Liverpool John Moores University (UK)." | |||||||
(1.3) Important Note: When the published work is entirely or partly conducted by GROWTH team members from Japan, India and Taiwan or it uses data obtained by one or more of the GROWTH facilities in these countries, the following acknowledgement statements should be added to the short and long statement listed above: | ||||||||
Line: 73 to 73 | ||||||||
(3) Boilerplate text (to be used in non-scientific publications like press releases, interviews, featured stories, etc) | ||||||||
Changed: | ||||||||
< < | “GROWTH is a collaborative project in astronomy set out to explore cosmic transients - energetic flashes of light that are millions to billions of times the brightness of the sun caused by exotic cosmic events like explosive deaths of massive stars, white dwarf detonations, exotic neutron star or black hole mergers. Led by Caltech, twelve partner institutions from around the world have created a collaborative network of observatories to effectively beat sunrise and keep our "eyes" fixed on these short-lived cosmic events by switching observations from one location to the next as the earth rotates. These extended initial observations in the first 24 hours after a cosmic transient is detected will help us localize the primary source of gravitational wave, identify the long sought cosmic location of heavy element production, track and analyze small near-earth asteroids and much more. GROWTH is jointly funded by the National Science Foundation under the PIRE program and national funding provided by partner institutions in Japan, Taiwan and India. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.” | |||||||
> > | “GROWTH is a collaborative project in astronomy set out to explore cosmic transients - energetic flashes of light that are millions to billions of times the brightness of the sun caused by exotic cosmic events like explosive deaths of massive stars, white dwarf detonations, exotic neutron star or black hole mergers. Led by Caltech, fourteen partner institutions from around the world have created a collaborative network of observatories to effectively beat sunrise and keep our "eyes" fixed on these short-lived cosmic events by switching observations from one location to the next as the earth rotates. These extended initial observations in the first 24 hours after a cosmic transient is detected will help us localize the primary source of gravitational wave, identify the long sought cosmic location of heavy element production, track and analyze small near-earth asteroids and much more. GROWTH is jointly funded by the National Science Foundation under the PIRE program and national funding provided by partner institutions in Japan, Taiwan and India. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.” | |||||||
8. Non-scientific publications, news & press releases, interviews, blogs, etc |
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1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are | ||||||||
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Japan: _The author(s) also acknowledge the support of Japan Society for the Promotion of Science._ Taiwan: _The author(s) also acknowledge the support of the Ministry of Science & Technology, Taiwan under Grant 104-2923-M-008-004-MY5._ | ||||||||
Changed: | ||||||||
< < | India: The author(s) also acknowledge the support of the Science and Engineering Research Board, Department of Science and Technology, India. | |||||||
> > | India: The author(s) also acknowledge the support of Indo-US Science and Technology Forum and the Science and Engineering Research Board, Department of Science and Technology, India. | |||||||
(2) Acknowledgement in non-scientific publications |
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1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are | ||||||||
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(1.1) Short acknowledgement statement (must be used in all scientific articles or papers appearing in scientific, technical or professional journals) | ||||||||
Changed: | ||||||||
< < | "This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949." | |||||||
> > | "This work was supported by the GROWTH project funded by the National Science Foundation under PIRE Grant No 1545949." | |||||||
(1.2) Long acknowledgement statement (optional) (can be used in all scientific articles or papers appearing in scientific, technical or professional journals instead of the short statement) | ||||||||
Changed: | ||||||||
< < | "This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949. GROWTH is a collaborative project among California Institute of Technology (USA), Pomona College (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany)" | |||||||
> > | "This work was supported by the GROWTH (Global Relay of Observatories Watching Transients Happen) project funded by the National Science Foundation under PIRE Grant No 1545949. GROWTH is a collaborative project among California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), Liverpool John Moores University (UK)." | |||||||
(1.3) Important Note: When the published work is entirely or partly conducted by GROWTH team members from Japan, India and Taiwan or it uses data obtained by one or more of the GROWTH facilities in these countries, the following acknowledgement statements should be added to the short and long statement listed above: |
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1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are |
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1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are | ||||||||
Line: 52 to 52 | ||||||||
(1.2) Long acknowledgement statement (optional) (can be used in all scientific articles or papers appearing in scientific, technical or professional journals instead of the short statement) | ||||||||
Changed: | ||||||||
< < | "This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949. GROWTH is a collaborative project between California Institute of Technology (USA), Pomona College (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany)" | |||||||
> > | "This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949. GROWTH is a collaborative project among California Institute of Technology (USA), Pomona College (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany)" | |||||||
(1.3) Important Note: When the published work is entirely or partly conducted by GROWTH team members from Japan, India and Taiwan or it uses data obtained by one or more of the GROWTH facilities in these countries, the following acknowledgement statements should be added to the short and long statement listed above: | ||||||||
Line: 73 to 73 | ||||||||
(3) Boilerplate text (to be used in non-scientific publications like press releases, interviews, featured stories, etc) | ||||||||
Changed: | ||||||||
< < | “GROWTH is a collaborative project in astronomy set out to explore cosmic transients - energetic flashes of light that are millions to billions of times the brightness of the sun caused by exotic cosmic events like explosive deaths of massive stars, white dwarf detonations, exotic neutron star or black hole mergers. Led by Caltech, twelve partner institutions from around the world have created a collaborative network of observatories to effectively beat sunrise and keep our "eyes" fixed on these short-lived cosmic events by switching observations from one location to the next as the earth rotates. These extended initial observations in the first 24 hours after a cosmic transient is detected will help us localize the primary source of gravitational wave, identify the long sought cosmic location of heavy element production, track and analyze small near-earth asteroids and much more. GROWTH is jointly funded by the National Science Foundation and national funding provided by partner institutions in Japan, Taiwan and India under the PIRE program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.” | |||||||
> > | “GROWTH is a collaborative project in astronomy set out to explore cosmic transients - energetic flashes of light that are millions to billions of times the brightness of the sun caused by exotic cosmic events like explosive deaths of massive stars, white dwarf detonations, exotic neutron star or black hole mergers. Led by Caltech, twelve partner institutions from around the world have created a collaborative network of observatories to effectively beat sunrise and keep our "eyes" fixed on these short-lived cosmic events by switching observations from one location to the next as the earth rotates. These extended initial observations in the first 24 hours after a cosmic transient is detected will help us localize the primary source of gravitational wave, identify the long sought cosmic location of heavy element production, track and analyze small near-earth asteroids and much more. GROWTH is jointly funded by the National Science Foundation under the PIRE program and national funding provided by partner institutions in Japan, Taiwan and India. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.” | |||||||
8. Non-scientific publications, news & press releases, interviews, blogs, etc |
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1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are | ||||||||
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(1.3) Important Note: When the published work is entirely or partly conducted by GROWTH team members from Japan, India and Taiwan or it uses data obtained by one or more of the GROWTH facilities in these countries, the following acknowledgement statements should be added to the short and long statement listed above: | ||||||||
Changed: | ||||||||
< < | Japan: The author(s) also acknowledge the support of Japan Society for the Promotion of Science. Taiwan: The author(s) also acknowledge the support of the Ministry of Science & Technology, Taiwan under Grant 104-2923-M-008-004-MY5. | |||||||
> > | Japan: _The author(s) also acknowledge the support of Japan Society for the Promotion of Science._ Taiwan: _The author(s) also acknowledge the support of the Ministry of Science & Technology, Taiwan under Grant 104-2923-M-008-004-MY5._ | |||||||
India: The author(s) also acknowledge the support of the Science and Engineering Research Board, Department of Science and Technology, India. |
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Added: | ||||||||
> > |
1. PurposeGROWTH is a collaboration of researchers who use our global network of observatories to conduct rapid follow-up observations of fast transients. The goals of this policy are
2. OversightThe GROWTH Management Team is responsible for managing all aspects of the publication policy. The Management Team shall arbitrate and settle any publication dispute. Authors may appeal to the Management Team for exceptions to the publication policy in special cases.3. Coverage of PolicyThis policy applies to all members in GROWTH as defined by the membership policy and all “GROWTH publications”. The latter are defined as:
4. AuthorshipAuthorship on GROWTH scientific publications should be driven by direct contribution to the scientific work. Contributions could be in the form of:
5. Conferences and PresentationsAny GROWTH member who is going to attend and present at a conference should inform the Program Coordinator via email providing information about the event (title, dates, location) as well as a title and an abstract to be presented. Authors are free to circulate abstracts to the GROWTH partnership for feedback via the existing mailing lists All presentations shall be uploaded to the GROWTH document repository.6. Circulation & SubmissionRough draft manuscripts shall be uploaded to the relevant sections of the existing iPTF twiki as well as circulated to GROWTH members via mailing lists a minimum of one week prior to desired submission date. In case of time-critical or competition-sensitive information/data in the draft, MT can grant exceptions to the circulation rule listed above. Drafts of peer-reviewed publications are discussed during the weekly science meetings of GROWTH. Any GROWTH member may suggest changes to the content and author list. Non-authors may not distribute draft manuscripts further without permission of authors. The corresponding author shall notify the Program Coordinator when the paper is accepted. The Program Coordinator maintains an ADS private library of publications with bibliographic information.7. AcknowledgementsThe following acknowledgement statements must be added to all GROWTH online or printed publications. All member of the GROWTH team should ensure that the appropriate acknowledgement features in their published work. (1) Acknowledgement in scientific publications (1.1) Short acknowledgement statement (must be used in all scientific articles or papers appearing in scientific, technical or professional journals) "This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949." (1.2) Long acknowledgement statement (optional) (can be used in all scientific articles or papers appearing in scientific, technical or professional journals instead of the short statement) "This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949. GROWTH is a collaborative project between California Institute of Technology (USA), Pomona College (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany)" (1.3) Important Note: When the published work is entirely or partly conducted by GROWTH team members from Japan, India and Taiwan or it uses data obtained by one or more of the GROWTH facilities in these countries, the following acknowledgement statements should be added to the short and long statement listed above: Japan: The author(s) also acknowledge the support of Japan Society for the Promotion of Science. Taiwan: The author(s) also acknowledge the support of the Ministry of Science & Technology, Taiwan under Grant 104-2923-M-008-004-MY5. India: The author(s) also acknowledge the support of the Science and Engineering Research Board, Department of Science and Technology, India. (2) Acknowledgement in non-scientific publications Note that except for articles or papers published in scientific, technical or professional journals, the following disclaimer must be included in all publication (including World Wide Web pages): "Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation." NSF support also must be orally acknowledged during all news media interviews, including popular media such as radio, television and news magazines. (3) Boilerplate text (to be used in non-scientific publications like press releases, interviews, featured stories, etc) “GROWTH is a collaborative project in astronomy set out to explore cosmic transients - energetic flashes of light that are millions to billions of times the brightness of the sun caused by exotic cosmic events like explosive deaths of massive stars, white dwarf detonations, exotic neutron star or black hole mergers. Led by Caltech, twelve partner institutions from around the world have created a collaborative network of observatories to effectively beat sunrise and keep our "eyes" fixed on these short-lived cosmic events by switching observations from one location to the next as the earth rotates. These extended initial observations in the first 24 hours after a cosmic transient is detected will help us localize the primary source of gravitational wave, identify the long sought cosmic location of heavy element production, track and analyze small near-earth asteroids and much more. GROWTH is jointly funded by the National Science Foundation and national funding provided by partner institutions in Japan, Taiwan and India under the PIRE program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.”8. Non-scientific publications, news & press releases, interviews, blogs, etcGROWTH is committed to communicating its scientific results to a wide range of audiences and the public at large. A well established mechanism of doing so includes press releases and news stories posted publicly on our website and shared on social media. Most publication are worthy of a news story. Therefore, if GROWTH members are interested in having their publication covered as a news story and potentially being picked up by larger media outlets, they need to inform and share their draft with the Program Coordinator at least one week BEFORE the publication is submitted to the public ArXiv.org. Press releases report or significant results and discoveries and are usually issued by a partner institution or our funding agency NSF. If members’ publication reports on significant advances in any GROWTH-related science field, they shall inform and share a draft with the Program Coordinator at least 2 weeks prior to submission. The Program Coordinator will work with the lead author(s) to draft a press release and pitch it to the appropriate larger organization. If a GROWTH member is contacted by any media representative for expert opinions and quote, interviews, or participation in podcast or other multimedia platforms, the member shall contact the Program Coordinator who must be aware of any appearance of GROWTH in local, national or international media. If a GROWTH members has or begins a personal blog, they shall inform the Program Coordinator as well. -- IvaKostadinova - 19 Oct 2016 |