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NANCY: Next-generation All-sky Near-infrared Community surveY

Journal Article · · No journal information
OSTI ID:2202841
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  1. Harvard-Smithsonian Ctr. Astrophys.
  2. Natl. Solar Observ., Tucson
  3. Flatiron Inst., New York
  4. Baltimore, Space Telescope Sci.
  5. KIPAC, Menlo Park; Stanford U.; SLAC
  6. Carnegie Inst. Observ.
  7. LBL, Berkeley
  8. Fermilab; Chicago U., Astron. Astrophys. Ctr.; Chicago U., EFI; Chicago U., KICP
  9. Canadian Inst. Theor. Astrophys.; Carnegie Inst. Observ.
  10. Edinburgh U., Inst. Astron.; Cambridge U.
  11. Arizona U., Astron. Dept. - Steward Observ.
  12. Heidelberg, Max Planck Inst. Astron.
  13. KASI, DaeJeon
  14. Kansas State U.
  15. U. Michigan, Dept. Astron.
  16. Washington U., Seattle
  17. Rochester U.
  18. SUNY, Stony Brook
  19. New York U., CCPP
  20. Caltech; Caltech, JPL
  21. Leiden Observ.
  22. Garching, Max Planck Inst., MPE
  23. NRAO, Tucson
  24. Durham U.; Durham U., ICC
  25. Barcelona, IEEC
  26. Academia Sinica, Taiwan
  27. Stanford U.; KIPAC, Menlo Park
  28. Michigan U., Dearborn
  29. NCTS, Hsinchu
  30. Caltech, JPL
  31. Columbia U.
  32. Princeton U., Astrophys. Sci. Dept.
  33. Potsdam, Astrophys. Inst.
  34. Pittsburgh U.
  35. Buenos Aires, CONICET; Cordoba U.
  36. NRAO, Socorro
  37. Surrey U.
  38. Princeton U., Astrophys. Sci. Dept.; Carnegie Inst. Observ.
  39. Edinburgh U., Inst. Astron.
  40. Johns Hopkins U. (main)
  41. Andes U., Bogota
  42. Rutgers U., Piscataway
  43. Yale U.
  44. Texas U., Astron. Dept.
  45. Caltech
  46. Ohio State U.
  47. San Francisco State U.
  48. Shanghai, Astron. Observ.
  49. Strasbourg Observ.
  50. Gemini Observ., La Serena; Natl. Solar Observ., Tucson
  51. Virginia U., Astron. Dept.
  52. UC, Merced
  53. Wigner RCP, Budapest
  54. Perimeter Inst. Theor. Phys.; Waterloo U., Math. Dept.
  55. LPSC, Grenoble
  56. Sejong U.
  57. NRAO, Charlottesville
  58. Taiwan, Natl. Taiwan U.
  59. Calgary U.
  60. Canadian Inst. Theor. Astrophys.
  61. Barcelona, IFAE; Barcelona, Autonoma U.
  62. Harvard-Smithsonian Ctr. Astrophys.; Columbia U.
  63. Strasbourg Observ.; Sejong U.
  64. Tsinghua U., Beijing; PCL, Shenzhen
  65. Costa Rica U.
  66. Siena Coll., Loudonville
  67. Dartmouth Coll.
  68. Harvard-Smithsonian Ctr. Astrophys.; Cambridge U.
  69. Wyoming U.
  70. Carnegie Inst. Observ.; UCLA
  71. La Serena U.
  72. Columbia U.; Flatiron Inst., New York
  73. Montana State U.
  74. Stockholm U., OKC
  75. Carnegie Mellon U.
  76. Argelander Inst. Astron.
  77. APC, Paris
  78. UCLA
  79. UC, Santa Cruz, Astron. Astrophys.
  80. UPenn, Philadelphia
  81. Newcastle U., United Kingdom, Sch. Math. Stat.
  82. MIT, MKI
  83. UC, Berkeley
  84. Clemson U.; LSST, Tucson
  85. Tsinghua U., Beijing
  86. Florida U.
  87. Keck Observ.
  88. U. Toronto (main); Pittsburgh U.; Canadian Inst. Theor. Astrophys.
  89. LPNHE, Paris
  90. UC, San Diego
  91. Chicago U., Astron. Astrophys. Ctr.; Chicago U., EFI; Chicago U., KICP
  92. UC, Davis
  93. Baltimore, Space Telescope Sci.; Johns Hopkins U. (main)
  94. Harvard U., Phys. Dept.; Harvard-Smithsonian Ctr. Astrophys.
  95. Beijing Observ.
  96. Baltimore, Space Telescope Sci.; Harvard-Smithsonian Ctr. Astrophys.
+ Show Author Affiliations
The Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This opportunity arises in the midst of numerous ground- and space-based surveys that will provide extensive spectroscopy and imaging together covering the entire sky (such as Rubin/LSST, Euclid, UNIONS, SPHEREx, DESI, SDSS-V, GALAH, 4MOST, WEAVE, MOONS, PFS, UVEX, NEO Surveyor, etc.). Roman can uniquely provide uniform high-spatial-resolution (~0.1 arcsec) imaging over the entire sky, vastly expanding the science reach and precision of all of these near-term and future surveys. This imaging will not only enhance other surveys, but also facilitate completely new science. By imaging the full sky over two epochs, Roman can measure the proper motions for stars across the entire Milky Way, probing 100 times fainter than Gaia out to the very edge of the Galaxy. Here, we propose NANCY: a completely public, all-sky survey that will create a high-value legacy dataset benefiting innumerable ongoing and forthcoming studies of the universe. NANCY is a pure expression of Roman's potential: it images the entire sky, at high spatial resolution, in a broad infrared bandpass that collects as many photons as possible. The majority of all ongoing astronomical surveys would benefit from incorporating observations of NANCY into their analyses, whether these surveys focus on nearby stars, the Milky Way, near-field cosmology, or the broader universe.
Research Organization:
Calgary U.; MIT, MKI; UC, Merced; Dartmouth Coll.; Chicago U., Astron. Astrophys. Ctr.; Strasbourg Observ.; Yale U.; La Serena U.; Newcastle U., United Kingdom, Sch. Math. Stat.; Waterloo U., Math. Dept.; Durham U., ICC; Natl. Solar Observ., Tucson; Siena Coll., Loudonville; Surrey U.; Baltimore, Space Telescope Sci.; NRAO, Charlottesville; NRAO, Tucson; LPNHE, Paris; Tsinghua U., Beijing; Barcelona, IEEC; Chicago U., EFI; New York U., CCPP; APC, Paris; Harvard-Smithsonian Ctr. Astrophys.; Stanford U.; Caltech; Florida U.; Heidelberg, Max Planck Inst. Astron.; Texas U., Astron. Dept.; Michigan U., Dearborn; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Shanghai, Astron. Observ.; Caltech, JPL; Taiwan, Natl. Taiwan U.; Cambridge U.; UC, Berkeley; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); UC, San Diego; Sejong U.; Beijing Observ.; Barcelona, Autonoma U.; Keck Observ.; Carnegie Mellon U.; Rutgers U., Piscataway; Andes U., Bogota; Virginia U., Astron. Dept.; Perimeter Inst. Theor. Phys.; Leiden Observ.; Edinburgh U., Inst. Astron.; LPSC, Grenoble; Durham U.; SUNY, Stony Brook; PCL, Shenzhen; KASI, DaeJeon; Columbia U.; Buenos Aires, CONICET; UPenn, Philadelphia; Carnegie Inst. Observ.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Wigner RCP, Budapest; UCLA; Pittsburgh U.; Stockholm U., OKC; Ohio State U.; U. Toronto (main); Potsdam, Astrophys. Inst.; UC, Santa Cruz, Astron. Astrophys.; U. Michigan, Dept. Astron.; Garching, Max Planck Inst., MPE; Costa Rica U.; UC, Davis; Argelander Inst. Astron.; Wyoming U.; Kansas State U.; Barcelona, IFAE; Cordoba U.; Montana State U.; Clemson U.; NCTS, Hsinchu; Chicago U., KICP; San Francisco State U.; Princeton U., Astrophys. Sci. Dept.; NRAO, Socorro; Flatiron Inst., New York; Rochester U.; LSST, Tucson; Gemini Observ., La Serena; Canadian Inst. Theor. Astrophys.; Johns Hopkins U. (main); Harvard U., Phys. Dept.; Arizona U., Astron. Dept. - Steward Observ.; Washington U., Seattle; Academia Sinica, Taiwan
Sponsoring Organization:
US Department of Energy
DOE Contract Number:
AC02-07CH11359; 89243024CSC000002
OSTI ID:
2202841
Report Number(s):
FERMILAB-PUB-23-591-PPD; oai:inspirehep.net:2700577; arXiv:2306.11784
Journal Information:
No journal information, Journal Name: No journal information
Country of Publication:
United States
Language:
English

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