THE gemini/nici planet-finding campaign: The frequency of planets around young moving group stars

Beth A. Biller, Michael C. Liu, Zahed Wahhaj, Eric L. Nielsen, Thomas L. Hayward, Jared R. Males, Andrew Skemer, Laird M Close, Mark Chun, Christ Ftaclas, Fraser Clarke, Niranjan Thatte, Evgenya L. Shkolnik, I. Neill Reid, Markus Hartung, Alan Boss, Douglas Lin, Silvia H P Alencar, Elisabete De Gouveia Dal Pino, Jane Gregorio-HetemDouglas Toomey

Research output: Contribution to journalArticle

114 Citations (Scopus)

Abstract

We report results of a direct imaging survey for giant planets around 80 members of the β Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI Planet-Finding Campaign. For this sample, we obtained median contrasts of ΔH = 13.9 mag at 1″ in combined CH4 narrowband ADI+SDI mode and median contrasts of ΔH = 15.1 mag at 2″ in H-band ADI mode. We found numerous (>70) candidate companions in our survey images. Some of these candidates were rejected as common-proper motion companions using archival data; we reobserved with Near-Infrared Coronagraphic Imager (NICI) all other candidates that lay within 400 AU of the star and were not in dense stellar fields. The vast majority of candidate companions were confirmed as background objects from archival observations and/or dedicated NICI Campaign followup. Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36 ± 6 M Jup, 16.4 ± 1.0 AU), CD-35 2722B (31 ± 8 M Jup, 67 ± 4 AU), HD 12894B (0.46 ± 0.08 M , 15.7 ± 1.0 AU), and BD+07 1919C (0.20 ± 0.03 M , 12.5 ± 1.4 AU). From a Bayesian analysis of the achieved H band ADI and ASDI contrasts, using power-law models of planet distributions and hot-start evolutionary models, we restrict the frequency of 1-20 M Jup companions at semi-major axes from 10-150 AU to <18% at a 95.4% confidence level using DUSTY models and to <6% at a 95.4% using COND models. Our results strongly constrain the frequency of planets within semi-major axes of 50 AU as well. We restrict the frequency of 1-20 M Jup companions at semi-major axes from 10-50 AU to <21% at a 95.4% confidence level using DUSTY models and to <7% at a 95.4% using COND models. This survey is the deepest search to date for giant planets around young moving group stars.

Original languageEnglish (US)
Article number160
JournalAstrophysical Journal
Volume777
Issue number2
DOIs
StatePublished - Nov 10 2013

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planets
planet
stars
near infrared
confidence
Bayesian analysis
star distribution
proper motion
stellar mass
narrowband
young
power law

Keywords

  • binaries: close
  • brown dwarfs
  • planetary systems
  • planets and satellites: detection
  • stars: late-type

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Biller, B. A., Liu, M. C., Wahhaj, Z., Nielsen, E. L., Hayward, T. L., Males, J. R., ... Toomey, D. (2013). THE gemini/nici planet-finding campaign: The frequency of planets around young moving group stars. Astrophysical Journal, 777(2), [160]. https://doi.org/10.1088/0004-637X/777/2/160

THE gemini/nici planet-finding campaign : The frequency of planets around young moving group stars. / Biller, Beth A.; Liu, Michael C.; Wahhaj, Zahed; Nielsen, Eric L.; Hayward, Thomas L.; Males, Jared R.; Skemer, Andrew; Close, Laird M; Chun, Mark; Ftaclas, Christ; Clarke, Fraser; Thatte, Niranjan; Shkolnik, Evgenya L.; Reid, I. Neill; Hartung, Markus; Boss, Alan; Lin, Douglas; Alencar, Silvia H P; De Gouveia Dal Pino, Elisabete; Gregorio-Hetem, Jane; Toomey, Douglas.

In: Astrophysical Journal, Vol. 777, No. 2, 160, 10.11.2013.

Research output: Contribution to journalArticle

Biller, BA, Liu, MC, Wahhaj, Z, Nielsen, EL, Hayward, TL, Males, JR, Skemer, A, Close, LM, Chun, M, Ftaclas, C, Clarke, F, Thatte, N, Shkolnik, EL, Reid, IN, Hartung, M, Boss, A, Lin, D, Alencar, SHP, De Gouveia Dal Pino, E, Gregorio-Hetem, J & Toomey, D 2013, 'THE gemini/nici planet-finding campaign: The frequency of planets around young moving group stars', Astrophysical Journal, vol. 777, no. 2, 160. https://doi.org/10.1088/0004-637X/777/2/160
Biller, Beth A. ; Liu, Michael C. ; Wahhaj, Zahed ; Nielsen, Eric L. ; Hayward, Thomas L. ; Males, Jared R. ; Skemer, Andrew ; Close, Laird M ; Chun, Mark ; Ftaclas, Christ ; Clarke, Fraser ; Thatte, Niranjan ; Shkolnik, Evgenya L. ; Reid, I. Neill ; Hartung, Markus ; Boss, Alan ; Lin, Douglas ; Alencar, Silvia H P ; De Gouveia Dal Pino, Elisabete ; Gregorio-Hetem, Jane ; Toomey, Douglas. / THE gemini/nici planet-finding campaign : The frequency of planets around young moving group stars. In: Astrophysical Journal. 2013 ; Vol. 777, No. 2.
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AU - Nielsen, Eric L.

AU - Hayward, Thomas L.

AU - Males, Jared R.

AU - Skemer, Andrew

AU - Close, Laird M

AU - Chun, Mark

AU - Ftaclas, Christ

AU - Clarke, Fraser

AU - Thatte, Niranjan

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AU - Boss, Alan

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AU - Toomey, Douglas

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N2 - We report results of a direct imaging survey for giant planets around 80 members of the β Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI Planet-Finding Campaign. For this sample, we obtained median contrasts of ΔH = 13.9 mag at 1″ in combined CH4 narrowband ADI+SDI mode and median contrasts of ΔH = 15.1 mag at 2″ in H-band ADI mode. We found numerous (>70) candidate companions in our survey images. Some of these candidates were rejected as common-proper motion companions using archival data; we reobserved with Near-Infrared Coronagraphic Imager (NICI) all other candidates that lay within 400 AU of the star and were not in dense stellar fields. The vast majority of candidate companions were confirmed as background objects from archival observations and/or dedicated NICI Campaign followup. Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36 ± 6 M Jup, 16.4 ± 1.0 AU), CD-35 2722B (31 ± 8 M Jup, 67 ± 4 AU), HD 12894B (0.46 ± 0.08 M , 15.7 ± 1.0 AU), and BD+07 1919C (0.20 ± 0.03 M , 12.5 ± 1.4 AU). From a Bayesian analysis of the achieved H band ADI and ASDI contrasts, using power-law models of planet distributions and hot-start evolutionary models, we restrict the frequency of 1-20 M Jup companions at semi-major axes from 10-150 AU to <18% at a 95.4% confidence level using DUSTY models and to <6% at a 95.4% using COND models. Our results strongly constrain the frequency of planets within semi-major axes of 50 AU as well. We restrict the frequency of 1-20 M Jup companions at semi-major axes from 10-50 AU to <21% at a 95.4% confidence level using DUSTY models and to <7% at a 95.4% using COND models. This survey is the deepest search to date for giant planets around young moving group stars.

AB - We report results of a direct imaging survey for giant planets around 80 members of the β Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI Planet-Finding Campaign. For this sample, we obtained median contrasts of ΔH = 13.9 mag at 1″ in combined CH4 narrowband ADI+SDI mode and median contrasts of ΔH = 15.1 mag at 2″ in H-band ADI mode. We found numerous (>70) candidate companions in our survey images. Some of these candidates were rejected as common-proper motion companions using archival data; we reobserved with Near-Infrared Coronagraphic Imager (NICI) all other candidates that lay within 400 AU of the star and were not in dense stellar fields. The vast majority of candidate companions were confirmed as background objects from archival observations and/or dedicated NICI Campaign followup. Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36 ± 6 M Jup, 16.4 ± 1.0 AU), CD-35 2722B (31 ± 8 M Jup, 67 ± 4 AU), HD 12894B (0.46 ± 0.08 M , 15.7 ± 1.0 AU), and BD+07 1919C (0.20 ± 0.03 M , 12.5 ± 1.4 AU). From a Bayesian analysis of the achieved H band ADI and ASDI contrasts, using power-law models of planet distributions and hot-start evolutionary models, we restrict the frequency of 1-20 M Jup companions at semi-major axes from 10-150 AU to <18% at a 95.4% confidence level using DUSTY models and to <6% at a 95.4% using COND models. Our results strongly constrain the frequency of planets within semi-major axes of 50 AU as well. We restrict the frequency of 1-20 M Jup companions at semi-major axes from 10-50 AU to <21% at a 95.4% confidence level using DUSTY models and to <7% at a 95.4% using COND models. This survey is the deepest search to date for giant planets around young moving group stars.

KW - binaries: close

KW - brown dwarfs

KW - planetary systems

KW - planets and satellites: detection

KW - stars: late-type

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