
§ 01People · Faculty
Andy Howell
Adjunct Professor; Senior Staff Scientist, Las Cumbres Observatory
Andy Howell is a senior staff scientist at Las Cumbres Observatory, where he runs a research group, and an adjunct professor at UCSB, where he teaches and advises students and postdocs. He studies supernovae, kilonovae and tidal disruption events.
He is PI of the Global Supernova Project, a collaboration of more than 200 scientists, and co-PI of the Global Kilonova Project, which searches for the counterparts of gravitational wave events. In 2017 his group at Las Cumbres was one of six teams to find the first kilonova, from a neutron star merger in NGC 4993. He has helped discover new types of supernovae and has used supernovae for cosmology, including in the Supernova Legacy Survey.
He received his PhD from the University of Texas and was a postdoc at Lawrence Berkeley National Laboratory and the University of Toronto.
§ 02Fig. 1
Where in the universe
Range 3.2 Mly to 10 Gly
§ 03Publications
Recent papers
The newest papers with Andy Howell as an author, from NASA ADS. Group members are in gold.
- 01Oct 2026ApJLJWST Observations of SN 2024abup: First Detection of CO in a Broad-lined Type Ic Supernova and Constraints on r-process NucleosynthesisM. Shrestha, L. A. Kwok, D. J. Sand, S. Barmentloo, C. Christy, A. Jerkstrand, K. A. Bostroem, J. E. Andrews et al. (45 authors); UCSB: D. A. Howell, C. McCully, K. WynnStars & transientsarXiv:2606.28561
- 02Oct 2026ApJJWST Nebular Spectroscopy of SN 2023qov: Circumstellar Dust Emission in a Normal Type Ia SupernovaC. W. Macrie, C. Larison, H. Sears, L. A. Kwok, S. W. Jha, M. Dai, J. Johansson, S. Blondin et al. (46 authors); UCSB: D. A. HowellStars & transientsarXiv:2604.09777
- 03Sep 2026arXivNearby Supernova Science in the Era of High Cadence, Deep Time Domain SurveysD. J. Sand, B. Subrayan, C. L. Ransome, G. Hosseinzadeh, K. A. Bostroem, J. E. Andrews, J. Pearson, Y. Dong et al. (44 authors); UCSB: D. A. Howell, C. McCullyStars & transientsarXiv:2609.38304
- 04Sep 2026arXivThe 91T/99aa-like Type Ia Supernova 2019vrq, Part I: Photometry, Spectroscopy, and Spectropolarimetry of a Nearly Standard CandleY. Yang, P. Hoeflich, J. C. Wheeler, D. Baade, L. Wang, A. Cikota, D. A. Howell, C. McCully et al. (19 authors)Stars & transientsarXiv:2609.31510
- 05Sep 2026arXivTomography analysis of the intermediate-luminosity Type Iax SN 2024pxlB. Barna, M. Singh, L. A. Kwok, S. W. Jha, R. Dastidar, C. Larison, A. V. Filippenko, J. P. Anderson et al. (93 authors); UCSB: D. A. Howell, C. McCullyStars & transientsarXiv:2609.28712
- 06Sep 2026arXivEarly NIR echo and the time variable mass loss history of Type IIn SN 2024kgiN. Dukiya, K. Misra, A. Pastorello, A. Reguitti, A. Gangopadhyay, A. P. Ravi, B. Hsu, N. Franz et al. (33 authors); UCSB: D. A. Howell, C. McCully, K. WynnStars & transientsarXiv:2609.25233
- 07Sep 2026arXivA Proliferated Space Architecture for Time-Domain AstrophysicsD. Kocevski, E. Burns, T. Barclay, N. E. White, M. Galeazzi, B. O'Connor, A. Lien, C. Fryer et al. (61 authors); UCSB: D. A. HowellStars & transientsarXiv:2609.12153
- 08Sep 2026arXivSN 2025fhm: A central-engine powered Ic-BL supernova associated with X-ray transient EP250304aC.-Y. Song, N. Jiang, X. Wang, Y.-H. I. Yin, L. Wang, W. Li, S. Yan, D.-S. Moon et al. (35 authors); UCSB: K. Wynn, D. A. Howell, C. McCullyStars & transientsarXiv:2609.08356
- 09Sep 2026ApJSN 2019cqc: A Hydrogen-rich Superluminous Supernova Showing Electron-scattering SignaturesD. Hebbar, R. Roy, M. Nicholl, J. Sollerman, J. P. Anderson, M. Gromadzki, D. A. Howell, T. Kangas et al. (18 authors); UCSB: C. McCullyStars & transientsarXiv:2608.30309
- 10Sep 2026ApJAT 2022csn: A Photometrically Peculiar Optical/UV Tidal Disruption Event in a Type II AGNY. Dgany, I. Arcavi, G. Zeltyn, S. Gomez, D. Hiramatsu, B. Trakhtenbrot, M. Newsome, D. Baron et al. (21 authors); UCSB: D. A. HowellStars & transientsarXiv:2608.02725
§ 04Sky
Gravitational wave events
Events from Andy Howell's papers. Most have no point position on the sky, only a region that holds the source with 90% probability.
Binary neutron star merger
GW170817
- 90% region
- 16 deg²
- Distance
- dL = 40 Mpc
Map: GWTC-1 skymap (GWOSC)
Binary neutron star merger
GW190425
- 90% region
- 8,700 deg²
- Distance
- dL = 150 Mpc
- Las Cumbres Observatory Gravitational-wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy 2026
- The Gravity Collective: A Comprehensive Analysis of the Electromagnetic Search for the Binary Neutron Star Merger GW190425 2025
- The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: A Case Study on GW190425 2021
Map: GWTC-2.1 (GWOSC)
Neutron star–black hole merger
GW190426_152155
- 90% region
- 1,385 deg²
- Distance
- dL = 370 Mpc
Map: GWTC-2 skymap (GWOSC)
Binary black hole merger
GW190728_064510
- 90% region
- 400 deg²
- Distance
- z = 0.18
Map: GWTC-2.1 (GWOSC)
Neutron star–black hole merger
GW190814
- 90% region
- 22 deg²
- Distance
- dL = 230 Mpc
- Las Cumbres Observatory Gravitational-wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy 2026
- SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO/Virgo Event GW190814 2022
- The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814 2021
Map: GWTC-2.1 skymap (GWOSC)
Binary black hole merger
GW191216_213338
- 90% region
- 910 deg²
- Distance
- dL = 340 Mpc
Map: GWTC-3 (GWOSC)