_version_ 1866911777682358272
author Henderson, Beth A.
Casewell, Sarah L.
Goad, Michael R.
Acton, Jack S.
Günther, Maximilian N.
Nielsen, Louise D.
Burleigh, Matthew R.
Belardi, Claudia
Tilbrook, Rosanna H.
Turner, Oliver
Howell, Steve B.
Clark, Catherine A.
Littlefield, Colin
Barkaoui, Khalid
Alves, Douglas R.
Anderson, David R.
Bayliss, Daniel
Bouchy, Francois
Bryant, Edward M.
Dransfield, George
Ducrot, Elsa
Eigmüller, Philipp
Gill, Samuel
Gillen, Edward
Gillon, Michaël
Hawthorn, Faith
Hooton, Matthew J.
Jackman, James A. G.
Jehin, Emmanuel
Jenkins, James S.
Kendall, Alicia
Lendl, Monika
McCormac, James
Moyano, Maximiliano
Pedersen, Peter Pihlmann
Pozuelos, Francisco J.
Ramsay, Gavin
Sefako, Ramotholo R.
Timmermans, Mathilde
Triaud, Amaury H. M. J.
Udry, Stephane
Vines, Jose I.
Watson, Christopher A.
West, Richard G.
Wheatley, Peter J.
Zúñiga-Fernández, Sebastián
author_facet Henderson, Beth A.
Casewell, Sarah L.
Goad, Michael R.
Acton, Jack S.
Günther, Maximilian N.
Nielsen, Louise D.
Burleigh, Matthew R.
Belardi, Claudia
Tilbrook, Rosanna H.
Turner, Oliver
Howell, Steve B.
Clark, Catherine A.
Littlefield, Colin
Barkaoui, Khalid
Alves, Douglas R.
Anderson, David R.
Bayliss, Daniel
Bouchy, Francois
Bryant, Edward M.
Dransfield, George
Ducrot, Elsa
Eigmüller, Philipp
Gill, Samuel
Gillen, Edward
Gillon, Michaël
Hawthorn, Faith
Hooton, Matthew J.
Jackman, James A. G.
Jehin, Emmanuel
Jenkins, James S.
Kendall, Alicia
Lendl, Monika
McCormac, James
Moyano, Maximiliano
Pedersen, Peter Pihlmann
Pozuelos, Francisco J.
Ramsay, Gavin
Sefako, Ramotholo R.
Timmermans, Mathilde
Triaud, Amaury H. M. J.
Udry, Stephane
Vines, Jose I.
Watson, Christopher A.
West, Richard G.
Wheatley, Peter J.
Zúñiga-Fernández, Sebastián
contents We report the discovery of a brown dwarf orbiting a M1 host star. We first identified the brown dwarf within the Next Generation Transit Survey data, with supporting observations found in TESS sectors 11 and 38. We confirmed the discovery with follow-up photometry from the South African Astronomical Observatory, SPECULOOS-S, and TRAPPIST-S, and radial velocity measurements from HARPS, which allowed us to characterise the system. We find an orbital period of ~1.25 d, a mass of 69.0+5.3-4.8 MJ, close to the Hydrogen burning limit, and a radius of 0.95 +- 0.05 RJ. We determine the age to be >0.5 Gyr, using model isochrones, which is found to be in agreement with SED fitting within errors. NGTS-28Ab is one of the shortest period systems found within the brown dwarf desert, as well as one of the highest mass brown dwarfs that transits an M dwarf. This makes NGTS-28Ab another important discovery within this scarcely populated region.
format Preprint
id arxiv_https___arxiv_org_abs_2402_09943
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle NGTS-28Ab: A short period transiting brown dwarf
Henderson, Beth A.
Casewell, Sarah L.
Goad, Michael R.
Acton, Jack S.
Günther, Maximilian N.
Nielsen, Louise D.
Burleigh, Matthew R.
Belardi, Claudia
Tilbrook, Rosanna H.
Turner, Oliver
Howell, Steve B.
Clark, Catherine A.
Littlefield, Colin
Barkaoui, Khalid
Alves, Douglas R.
Anderson, David R.
Bayliss, Daniel
Bouchy, Francois
Bryant, Edward M.
Dransfield, George
Ducrot, Elsa
Eigmüller, Philipp
Gill, Samuel
Gillen, Edward
Gillon, Michaël
Hawthorn, Faith
Hooton, Matthew J.
Jackman, James A. G.
Jehin, Emmanuel
Jenkins, James S.
Kendall, Alicia
Lendl, Monika
McCormac, James
Moyano, Maximiliano
Pedersen, Peter Pihlmann
Pozuelos, Francisco J.
Ramsay, Gavin
Sefako, Ramotholo R.
Timmermans, Mathilde
Triaud, Amaury H. M. J.
Udry, Stephane
Vines, Jose I.
Watson, Christopher A.
West, Richard G.
Wheatley, Peter J.
Zúñiga-Fernández, Sebastián
Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
We report the discovery of a brown dwarf orbiting a M1 host star. We first identified the brown dwarf within the Next Generation Transit Survey data, with supporting observations found in TESS sectors 11 and 38. We confirmed the discovery with follow-up photometry from the South African Astronomical Observatory, SPECULOOS-S, and TRAPPIST-S, and radial velocity measurements from HARPS, which allowed us to characterise the system. We find an orbital period of ~1.25 d, a mass of 69.0+5.3-4.8 MJ, close to the Hydrogen burning limit, and a radius of 0.95 +- 0.05 RJ. We determine the age to be >0.5 Gyr, using model isochrones, which is found to be in agreement with SED fitting within errors. NGTS-28Ab is one of the shortest period systems found within the brown dwarf desert, as well as one of the highest mass brown dwarfs that transits an M dwarf. This makes NGTS-28Ab another important discovery within this scarcely populated region.
title NGTS-28Ab: A short period transiting brown dwarf
topic Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2402.09943