Radial Velocity Survey for Planets around Young stars RV-SPY · 2020-01-23 · RV-SPY vs I SPY...

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Radial Velocity Survey for Planets around Young stars RV-SPY

Olga Zakhozhay

R. Launhardt, S. Brems, Th. Henning, A. Müller, T. Trifonov, M. Kürster, S. Reffert, A. Pavlov, G. Kennedy, J. Patel

Great Barriers in Planet Formation, Palm Cove— 23.07.2019

Search for Planets around Young Stars with

Search for Planets around Young Stars with

Instrument:

FEROS, 2.2m telescope (La Silla)

Observing time granted: 435h (p101-103, 2018-2019)

Science team: 11 researchers from 3 institutes

Targets sample:111 stars

Science goal: Characterizing the Giant Planets population at the separation of

<5 au around the stars with

debris disks

NaCo, UT1 (Paranal)

120n over 4.0yr (2015-2019)

22 researchers from 6 institutes

~230 stars

>5-10 au

protoplantery and debris disks

Radial Velosity Imaging (RV-SPY) (ISPY)

RV-SPY vs I SPY

Observing strategy:

Initial survey: - first 2 years

- observations of all targets in high-cadence (aim: 14 consecutive nights, 1 spectra each night and 1 night 3 spectra per target);

Follow-up observations: - after 2nd observing semester

- observations of the highest priority targets selected during initial survey results (cadence determined individually for each case).

Search for Planets around Young Stars with

RV-SPY targets parameters distribution

Observations: 370h, 1815 spectra.

95 targets observed in high cadence:

25 have clear activity indication: BIS(RV) anti-correlation; 12 positive BIS(RV) correlation;

20 are followed-up already due to the strongest evidence for a significant signal (short or long period) not induced by the stellar activity.

RV-SPY: results of 1.5 observing years

Bisector span (BIS)

Brahm et al. 2017

W. Torres, YPSW, Nov.2010

RV-SPY preliminary resultsClear activity cases (26% of the observed sample)

G1 V K0 V

G2 V G5 V

RV-SPY preliminary resultsInteresting candidate

K7 V

Best fit parameters: Mst = 0.7 Msun Mpl sin(i) = 0.7 Mjup a = 0.05 au P = 4.53 days e = 0.24

FEROS archive data RV-SPY data

RV-SPY preliminary resultsInteresting candidate

K7 V

RV-SPY preliminary resultsInteresting candidate→ activity case

K7 V

RV-SPY preliminary resultsInteresting candidate

K2 V

RV-SPY preliminary resultsPositive BIS (RV)

F5 V, 1.12 Gyr

Строка 1 Строка 2 Строка 3 Строка 40

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4

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12

Столбец 1

Столбец 2

Столбец 3

Conclusion:

- More observations are needed.