Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS)
A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is supported by a large representation of the community of Galactic astronomers. The combination of sensitivity, angular resolution and large field of view make Roman uniquely able to study the crowded and highly extincted lines...
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creator | Paladini, Roberta Zucker, Catherine Benjamin, Robert Nataf, David Minniti, Dante Zasowski, Gail Peek, Joshua Carey, Sean Allen, Lori Alonso-Garcia, Javier Alves, Joao Anders, Friederich Athanassoula, Evangelie Beers, Timothy C Bird, Jonathan Bland-Hwathorn, Joss Brown, Anthony Buder, Sven Casagrande, Luca Casey, Andrew Cassisi, Santi Catelan, Marcio Chary, Ranga-Ram Chene, Andre-Nicolas Ciardi, David Comeron, Fernando Cohen, Roger Dame, Thomas Drimmel, Ronald Trincado, Jose Fernandez Finkbeiner, Douglas Geisler, Douglas Gennaro, Mario Goodman, Alyssa Green, Gregory Hajdu, Gergely Henderson, Calen Hora, Joseph Ivanov, Valentin D Kirkpatrick, Davy Kobayashi, Chiaki Kuhn, Michael Kunder, Andres Lu, Jessica Lucas, Philip W Majaess, Daniel Megeath, S. Thomas Meisner, Aaron Molinari, Sergio Mroz, Przemek Ness, Meliss Neumayer, Nadine Nogueras-Lara, Francisco Noriega-Crespo, Alberto Poleski, Radek Rix, Hans-Walter Rebull, Luisa Reggiani, Henrique Rejkuba, Marina Saito, Roberto K Schoenrich, Ralph Saydjari, Andrew Schisano, Eugenio Schlafly, Edward Schlaufman, Keving Smith, Leigh Speagle, Joshua Wisz, Dan Wyse, Rosemary Zakamska, Nadia |
description | A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is
supported by a large representation of the community of Galactic astronomers.
The combination of sensitivity, angular resolution and large field of view make
Roman uniquely able to study the crowded and highly extincted lines of sight in
the Galactic plane. A ~1000 deg2 survey of the bulge and inner Galactic disk
would yield an impressive dataset of ~120 billion sources and map the structure
of our Galaxy. The effort would foster subsequent expansions in numerous
dimensions (spatial, depth, wavelengths, epochs). Importantly, the survey would
benefit from early defintion by the community, namely because the Galactic disk
is a complex environment, and different science goals will require trade offs. |
doi_str_mv | 10.48550/arxiv.2307.07642 |
format | Article |
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supported by a large representation of the community of Galactic astronomers.
The combination of sensitivity, angular resolution and large field of view make
Roman uniquely able to study the crowded and highly extincted lines of sight in
the Galactic plane. A ~1000 deg2 survey of the bulge and inner Galactic disk
would yield an impressive dataset of ~120 billion sources and map the structure
of our Galaxy. The effort would foster subsequent expansions in numerous
dimensions (spatial, depth, wavelengths, epochs). Importantly, the survey would
benefit from early defintion by the community, namely because the Galactic disk
is a complex environment, and different science goals will require trade offs.</description><identifier>DOI: 10.48550/arxiv.2307.07642</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Instrumentation and Methods for Astrophysics</subject><creationdate>2023-07</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2307.07642$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2307.07642$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Paladini, Roberta</creatorcontrib><creatorcontrib>Zucker, Catherine</creatorcontrib><creatorcontrib>Benjamin, Robert</creatorcontrib><creatorcontrib>Nataf, David</creatorcontrib><creatorcontrib>Minniti, Dante</creatorcontrib><creatorcontrib>Zasowski, Gail</creatorcontrib><creatorcontrib>Peek, Joshua</creatorcontrib><creatorcontrib>Carey, Sean</creatorcontrib><creatorcontrib>Allen, Lori</creatorcontrib><creatorcontrib>Alonso-Garcia, Javier</creatorcontrib><creatorcontrib>Alves, Joao</creatorcontrib><creatorcontrib>Anders, Friederich</creatorcontrib><creatorcontrib>Athanassoula, Evangelie</creatorcontrib><creatorcontrib>Beers, Timothy C</creatorcontrib><creatorcontrib>Bird, Jonathan</creatorcontrib><creatorcontrib>Bland-Hwathorn, Joss</creatorcontrib><creatorcontrib>Brown, Anthony</creatorcontrib><creatorcontrib>Buder, Sven</creatorcontrib><creatorcontrib>Casagrande, Luca</creatorcontrib><creatorcontrib>Casey, Andrew</creatorcontrib><creatorcontrib>Cassisi, Santi</creatorcontrib><creatorcontrib>Catelan, Marcio</creatorcontrib><creatorcontrib>Chary, Ranga-Ram</creatorcontrib><creatorcontrib>Chene, Andre-Nicolas</creatorcontrib><creatorcontrib>Ciardi, David</creatorcontrib><creatorcontrib>Comeron, Fernando</creatorcontrib><creatorcontrib>Cohen, Roger</creatorcontrib><creatorcontrib>Dame, Thomas</creatorcontrib><creatorcontrib>Drimmel, Ronald</creatorcontrib><creatorcontrib>Trincado, Jose Fernandez</creatorcontrib><creatorcontrib>Finkbeiner, Douglas</creatorcontrib><creatorcontrib>Geisler, Douglas</creatorcontrib><creatorcontrib>Gennaro, Mario</creatorcontrib><creatorcontrib>Goodman, Alyssa</creatorcontrib><creatorcontrib>Green, Gregory</creatorcontrib><creatorcontrib>Hajdu, Gergely</creatorcontrib><creatorcontrib>Henderson, Calen</creatorcontrib><creatorcontrib>Hora, Joseph</creatorcontrib><creatorcontrib>Ivanov, Valentin D</creatorcontrib><creatorcontrib>Kirkpatrick, Davy</creatorcontrib><creatorcontrib>Kobayashi, Chiaki</creatorcontrib><creatorcontrib>Kuhn, Michael</creatorcontrib><creatorcontrib>Kunder, Andres</creatorcontrib><creatorcontrib>Lu, Jessica</creatorcontrib><creatorcontrib>Lucas, Philip W</creatorcontrib><creatorcontrib>Majaess, Daniel</creatorcontrib><creatorcontrib>Megeath, S. Thomas</creatorcontrib><creatorcontrib>Meisner, Aaron</creatorcontrib><creatorcontrib>Molinari, Sergio</creatorcontrib><creatorcontrib>Mroz, Przemek</creatorcontrib><creatorcontrib>Ness, Meliss</creatorcontrib><creatorcontrib>Neumayer, Nadine</creatorcontrib><creatorcontrib>Nogueras-Lara, Francisco</creatorcontrib><creatorcontrib>Noriega-Crespo, Alberto</creatorcontrib><creatorcontrib>Poleski, Radek</creatorcontrib><creatorcontrib>Rix, Hans-Walter</creatorcontrib><creatorcontrib>Rebull, Luisa</creatorcontrib><creatorcontrib>Reggiani, Henrique</creatorcontrib><creatorcontrib>Rejkuba, Marina</creatorcontrib><creatorcontrib>Saito, Roberto K</creatorcontrib><creatorcontrib>Schoenrich, Ralph</creatorcontrib><creatorcontrib>Saydjari, Andrew</creatorcontrib><creatorcontrib>Schisano, Eugenio</creatorcontrib><creatorcontrib>Schlafly, Edward</creatorcontrib><creatorcontrib>Schlaufman, Keving</creatorcontrib><creatorcontrib>Smith, Leigh</creatorcontrib><creatorcontrib>Speagle, Joshua</creatorcontrib><creatorcontrib>Wisz, Dan</creatorcontrib><creatorcontrib>Wyse, Rosemary</creatorcontrib><creatorcontrib>Zakamska, Nadia</creatorcontrib><title>Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS)</title><description>A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is
supported by a large representation of the community of Galactic astronomers.
The combination of sensitivity, angular resolution and large field of view make
Roman uniquely able to study the crowded and highly extincted lines of sight in
the Galactic plane. A ~1000 deg2 survey of the bulge and inner Galactic disk
would yield an impressive dataset of ~120 billion sources and map the structure
of our Galaxy. The effort would foster subsequent expansions in numerous
dimensions (spatial, depth, wavelengths, epochs). Importantly, the survey would
benefit from early defintion by the community, namely because the Galactic disk
is a complex environment, and different science goals will require trade offs.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNo1j7FOwzAURb0woMIHMOERhgT3xYljtqqUEKlSq7Z79GI_C0tpEjlpRf4eaGG6y7lHOow9zEUs8zQVLxi-_DmGRKhYqEzCLbO77ogtX2FopuiNnG_96LuWL4YxdP3nNHgz8P0pnGnim77vwnj6IaZXXmCDZvSGXwVl6wIGsnzbYEv_j6diV273z3fsxmEz0P3fztjhfXVYfkTrTVEuF-sIMwVRrbVNAKwhQgnGqjxR0s5z0mAAjKlBo8vJKacpl5a0IidT7epaiNRlkMzY41V7yaz64I8Ypuo3t7rkJt-Mv1GQ</recordid><startdate>20230714</startdate><enddate>20230714</enddate><creator>Paladini, Roberta</creator><creator>Zucker, Catherine</creator><creator>Benjamin, Robert</creator><creator>Nataf, David</creator><creator>Minniti, Dante</creator><creator>Zasowski, Gail</creator><creator>Peek, Joshua</creator><creator>Carey, Sean</creator><creator>Allen, Lori</creator><creator>Alonso-Garcia, Javier</creator><creator>Alves, Joao</creator><creator>Anders, Friederich</creator><creator>Athanassoula, Evangelie</creator><creator>Beers, Timothy C</creator><creator>Bird, Jonathan</creator><creator>Bland-Hwathorn, Joss</creator><creator>Brown, Anthony</creator><creator>Buder, Sven</creator><creator>Casagrande, Luca</creator><creator>Casey, Andrew</creator><creator>Cassisi, Santi</creator><creator>Catelan, Marcio</creator><creator>Chary, Ranga-Ram</creator><creator>Chene, Andre-Nicolas</creator><creator>Ciardi, David</creator><creator>Comeron, Fernando</creator><creator>Cohen, Roger</creator><creator>Dame, Thomas</creator><creator>Drimmel, Ronald</creator><creator>Trincado, Jose Fernandez</creator><creator>Finkbeiner, Douglas</creator><creator>Geisler, Douglas</creator><creator>Gennaro, Mario</creator><creator>Goodman, Alyssa</creator><creator>Green, Gregory</creator><creator>Hajdu, Gergely</creator><creator>Henderson, Calen</creator><creator>Hora, Joseph</creator><creator>Ivanov, Valentin D</creator><creator>Kirkpatrick, Davy</creator><creator>Kobayashi, Chiaki</creator><creator>Kuhn, Michael</creator><creator>Kunder, Andres</creator><creator>Lu, Jessica</creator><creator>Lucas, Philip W</creator><creator>Majaess, Daniel</creator><creator>Megeath, S. 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Thomas</au><au>Meisner, Aaron</au><au>Molinari, Sergio</au><au>Mroz, Przemek</au><au>Ness, Meliss</au><au>Neumayer, Nadine</au><au>Nogueras-Lara, Francisco</au><au>Noriega-Crespo, Alberto</au><au>Poleski, Radek</au><au>Rix, Hans-Walter</au><au>Rebull, Luisa</au><au>Reggiani, Henrique</au><au>Rejkuba, Marina</au><au>Saito, Roberto K</au><au>Schoenrich, Ralph</au><au>Saydjari, Andrew</au><au>Schisano, Eugenio</au><au>Schlafly, Edward</au><au>Schlaufman, Keving</au><au>Smith, Leigh</au><au>Speagle, Joshua</au><au>Wisz, Dan</au><au>Wyse, Rosemary</au><au>Zakamska, Nadia</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS)</atitle><date>2023-07-14</date><risdate>2023</risdate><abstract>A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is
supported by a large representation of the community of Galactic astronomers.
The combination of sensitivity, angular resolution and large field of view make
Roman uniquely able to study the crowded and highly extincted lines of sight in
the Galactic plane. A ~1000 deg2 survey of the bulge and inner Galactic disk
would yield an impressive dataset of ~120 billion sources and map the structure
of our Galaxy. The effort would foster subsequent expansions in numerous
dimensions (spatial, depth, wavelengths, epochs). Importantly, the survey would
benefit from early defintion by the community, namely because the Galactic disk
is a complex environment, and different science goals will require trade offs.</abstract><doi>10.48550/arxiv.2307.07642</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | DOI: 10.48550/arxiv.2307.07642 |
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language | eng |
recordid | cdi_arxiv_primary_2307_07642 |
source | arXiv.org |
subjects | Physics - Astrophysics of Galaxies Physics - Instrumentation and Methods for Astrophysics |
title | Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS) |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T00%3A44%3A43IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Roman%20Early-Definition%20Astrophysics%20Survey%20Opportunity:%20Galactic%20Roman%20Infrared%20Plane%20Survey%20(GRIPS)&rft.au=Paladini,%20Roberta&rft.date=2023-07-14&rft_id=info:doi/10.48550/arxiv.2307.07642&rft_dat=%3Carxiv_GOX%3E2307_07642%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |