| Original language | English (US) |
|---|---|
| Pages (from-to) | 879-881 |
| Number of pages | 3 |
| Journal | Nature Astronomy |
| Volume | 7 |
| Issue number | 8 |
| DOIs |
|
| State | Published - Aug 2023 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
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In: Nature Astronomy, Vol. 7, No. 8, 08.2023, p. 879-881.
Research output: Contribution to journal › Comment/debate › peer-review
TY - JOUR
T1 - Introducing QUOTAS as a new research platform for the data-driven discovery of supermassive black holes
AU - Natarajan, Priyamvada
AU - Tang, Kwok Sun
AU - Khochfar, Sadegh
AU - Nord, Brian
AU - Sigurdsson, Steinn
AU - Tricot, Joe
AU - Cappelluti, Nico
AU - George, Daniel
AU - Hidary, Jack
N1 - Funding Information: P.N. gratefully acknowledges the invitation to Google’s Science Festival SciFoo in 2018, where she first hatched this idea, and thanks S. Sarma and B. Subirana at MIT for early discussions. She acknowledges Alphabet-X for technical support and computational resources for this project. P.N. and K.S.T. thank R. Ebert at the Infrared Processing and Analysis Center (IPAC) at the California Institute of Technology for his help with accessing the NED database. K.S.T. thanks F. Wang at Google for his help with the Google Cloud Platform. S.K. acknowledges use of the ARCHER UK National Super-computing Service (http://www.archer.ac.uk) for running the LEGACY simulation. B.N. acknowledges support from the Fermi National Accelerator Laboratory, managed and operated by Fermi Research Alliance, LLC under contract no. DE-AC02-07CH11359 with the US Department of Energy. This manuscript has been authored by Fermi Research Alliance, LLC under contract no. DE-AC02-07CH11359 with the US Department of Energy, Office of Science, Office of High Energy Physics. S.S. acknowledges the Aspen Center for Physics where parts of this work were done, which is supported by National Science Foundation grant PHY-1607611. Funding Information: P.N. gratefully acknowledges the invitation to Google’s Science Festival SciFoo in 2018, where she first hatched this idea, and thanks S. Sarma and B. Subirana at MIT for early discussions. She acknowledges Alphabet-X for technical support and computational resources for this project. P.N. and K.S.T. thank R. Ebert at the Infrared Processing and Analysis Center (IPAC) at the California Institute of Technology for his help with accessing the NED database. K.S.T. thanks F. Wang at Google for his help with the Google Cloud Platform. S.K. acknowledges use of the ARCHER UK National Super-computing Service ( http://www.archer.ac.uk ) for running the LEGACY simulation. B.N. acknowledges support from the Fermi National Accelerator Laboratory, managed and operated by Fermi Research Alliance, LLC under contract no. DE-AC02-07CH11359 with the US Department of Energy. This manuscript has been authored by Fermi Research Alliance, LLC under contract no. DE-AC02-07CH11359 with the US Department of Energy, Office of Science, Office of High Energy Physics. S.S. acknowledges the Aspen Center for Physics where parts of this work were done, which is supported by National Science Foundation grant PHY-1607611.
PY - 2023/8
Y1 - 2023/8
UR - http://www.scopus.com/inward/record.url?scp=85165660428&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85165660428&partnerID=8YFLogxK
U2 - 10.1038/s41550-021-01478-x
DO - 10.1038/s41550-021-01478-x
M3 - Comment/debate
AN - SCOPUS:85165660428
SN - 2397-3366
VL - 7
SP - 879
EP - 881
JO - Nature Astronomy
JF - Nature Astronomy
IS - 8
ER -