Published May 14, 2023
| Version 1e
Dataset
Open
PEARLS: Near Infrared Photometry in the JWST North Ecliptic Pole Time Domain Field
Authors/Creators
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Willmer, Christopher N. A.1
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Ly, Chun2
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Kikuta, Satoshi3
- Kattner, S. A.4
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Jansen, Rolf A5
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Cohen, Seth6
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Windhorst, Rogier5
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Smail, Ian7
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Tompkins, Scott8
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Beacom, John F.9
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Cheng, Cheng10
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Comselice, Christopher J.11
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Frye, Brenda L.1
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Koekemoer, Anton M.12
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Hathi, Nimish12
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Hyun, Minhee13
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Im, Myungshin14
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Willner, Steven P.15
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Zhao, X.15
- Brisken, Walter A.16
- Civano, Francesca17
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Cotton, William18
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Hasinger, Guenther19
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Maksym, W. Peter15
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Rieke, Marcia, J1
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Grogin, Norman, A12
- 1. Steward Observatory, University of Arizona
- 2. Princeton Plasma Physics Laboratory: Princeton, NJ, US
- 3. National Astronomical Observatory of Japan
- 4. MMT Observatory, University of Arizona
- 5. Arizona State University: Tempe, AZ, US
- 6. rizona State University: Tempe, AZ, US
- 7. Centre for Extragalactic Astronomy, Department of Physics, Durham University
- 8. School of Earth \& Space Exploration, Arizona State University
- 9. Center for Cosmology and AstroParticle Physics,Department of Astronomy, Ohio State University
- 10. Chinese Academy of Sciences, South America Center for Astronomy, National Astronomical Observatories
- 11. Jodrell Bank Centre for Astrophysics, University of Manchester
- 12. Space Telescope Science Institute
- 13. Korea Astronomy and Space Science Institute
- 14. SNU, Astronomy Research Center, Astronomy program, Dept. of Physics \& Astronomy, Seoul National University
- 15. Center for Astrophysics, Harvard University
- 16. Long Baseline Observatory
- 17. NASA Goddard Space Flight Center
- 18. National Radio Astronomy Observatory
- 19. ESA, European Space Astronomy Centre
Description
We make public visible and near-infrared images and derived catalogues obtained as part of the ground-based observations targetting the North Ecliptic Pole Time Domain Field. This is one of the prime targets of the PEARLS collaboration (Windhorst+ 2023, AJ 165, 13 (https://doi.org/10.3847/1538-3881/aca163), and was designed to identify transient objects (outer Solar System objects, variable stars, Active Galactic Nuclei, Supernovae). These data complement the already extensive coverage this field has had from space and ground-based observatories ranging from hard X-rays to radio.
Files
NEP_MMIRS_HSC_data_release.pdf
Files
(16.0 GB)
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