J/MNRAS/498/5972   Variables and dippers in young associations (Nardiello, 2020)

A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS). III. Exploring the properties of young associations through their variables, dippers, and candidate exoplanets. Nardiello D. <Mon. Not. R. Astron. Soc., 498, 5972-5989 (2020)> =2020MNRAS.498.5972N 2020MNRAS.498.5972N (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, globular ; Stars, variable; Photometry ; Optical ; Photometry, infrared Keywords: techniques: image processing - techniques: photometric - planets and satellites: general - stars: variables: general - open clusters and associations: general Abstract: Young associations in star-forming regions are stellar systems that allow us to understand the mechanisms that characterize the stars in their early life and what happens around them. In particular, the analysis of the discs and of the exoplanets around young stars allows us to know the key processes that prevail in their evolution and understand the properties of the exoplanets orbiting older stars. The Transiting Exoplanet Survey Satellite mission is giving us the opportunity to extract and analyse the light curves of association members with high accuracy, but the crowding that affects these regions makes difficult the light curve extraction. In the PATHOS project, cutting-edge tools are used to extract high-precision light curves and identify variable stars and transiting exoplanets in open clusters and associations. In this work, I analysed the light curves of stars in five young (<10Myr) associations, searching for variables and candidate exoplanets. Using the rotational periods of the association members, I constrained the ages of the five stellar systems (∼2-10Myr). I searched for dippers, and I investigated the properties of the dust that forms the circumstellar discs. Finally, I searched for transiting signals, finding six strong candidate exoplanets. No candidates with radius Rp<0.9RJ have been detected, in agreement with the expectations. The frequency of giant planets resulted to be ∼2-3 per cent, higher than that expected for field stars (<1 per cent); the low statistic makes this conclusion not strong, and new investigations on young objects are mandatory to confirm this result. Description: Properties of variable stars and disk around "dippers" in 5 young stellar associations (ChI, ChII, CrA, Lup and Vel). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file var.dat 413 1286 List of identified variables dippers.dat 413 71 List of identified dippers -------------------------------------------------------------------------------- See also: I/345 : Gaia DR2 (Gaia Collaboration, 2018) IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019) J/MNRAS/490/3806 : Exoplanets & variable stars in 47 Tuc (Nardiello+, 2019) J/MNRAS/495/4924 : Exoplanets in Southern open clusters (Nardiello+, 2020) https://archive.stsci.edu/hlsp/pathos : PATHOS Home Page Byte-by-byte Description of file: var.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.6 deg RAdeg Right ascension (ICRS) at Ep=2015.5 13- 22 F10.6 deg DEdeg Declination (ICRS) at Ep=2015.5 30- 38 I9 --- TIC TESS Input Catalog ID 43- 61 I19 --- GaiaDR2 Gaia DR2 Source ID 72- 82 F11.8 d Per ?=-99.9 Period 88- 93 F6.3 mag Gmag Gaia DR2 G magnitude 99-103 F5.3 mag e_Gmag Error on Gaia DR2 G magnitude 109-114 F6.3 mag BPmag ?=0.0 Gaia DR2 GBP magnitude 120-124 F5.3 mag e_BPmag ?=0.0 Error on Gaia DR2 GBP magnitude 130-135 F6.3 mag RPmag ?=0.0 Gaia DR2 GRP magnitude 141-145 F5.3 mag e_RPmag ?=0.0 Error on Gaia DR2 GRP magnitude 151-156 F6.3 mag Tmag TESS T magnitude 162-166 F5.3 mag e_Tmag Error on TESS T magnitude 172-177 F6.3 mag Bmag ?=0.0 B Johnson magnitude 183-187 F5.3 mag e_Bmag ?=0.0 Error on B Johnson magnitude 193-198 F6.3 mag Vmag ?=0.0 V Johnson magnitude 204-208 F5.3 mag e_Vmag ?=0.0 Error on V Johnson magnitude 214-219 F6.3 mag Jmag ?=0.0 2MASS J magnitude 225-229 F5.3 mag e_Jmag ?=0.0 Error on 2MASS J magnitude 235-240 F6.3 mag Hmag ?=0.0 2MASS H magnitude 246-250 F5.3 mag e_Hmag ?=0.0 Error on 2MASS H magnitude 256-261 F6.3 mag Kmag ?=0.0 2MASS K magnitude 267-271 F5.3 mag e_Kmag ?=0.0 Error on 2MASS K magnitude 277-282 F6.3 mag W1mag ?=0.0 WISE W1 magnitude 288-292 F5.3 mag e_W1mag ?=0.0 Error on WISE W1 magnitude 298-303 F6.3 mag W2mag ?=0.0 WISE W2 magnitude 309-313 F5.3 mag e_W2mag ?=0.0 Error on WISE W2 magnitude 319-324 F6.3 mag W3mag ?=0.0 WISE W3 magnitude 330-334 F5.3 mag e_W3mag ?=0.0 Error on WISE W3 magnitude 341-345 F5.3 mag W4mag ?=0.0 WISE W4 magnitude 351-355 F5.3 mag e_W4mag Error on WISE W4 magnitude 359-364 F6.4 --- E(B-V) Reddening 369-374 F6.4 mas Plx Parallax from Gaia DR2 376-383 F8.4 mas/yr pmRA Proper motion along RA from Gaia DR2, pmRA*cosDE 385-392 F8.4 mas/yr pmDE Proper motion along Dec from Gaia DR2 410-413 A4 --- Assoc Name of the association that host the star (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: dippers.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.6 deg RAdeg Right ascension (ICRS) at Ep=2015.5 13- 22 F10.6 deg DEdeg Declination (ICRS) at Ep=2015.5 30- 38 I9 --- TIC TESS Input Catalog ID 43- 61 I19 --- GaiaDR2 Gaia DR2 Source ID 65- 72 F8.4 --- AT/Ag ?=-99.9 Absorption in T and g bands ratio 75- 82 F8.4 --- e_AT/Ag ?=-99.9 Error on AT/Ag value 88- 93 F6.3 mag Gmag Gaia DR2 G magnitude 99-103 F5.3 mag e_Gmag Error on Gaia DR2 G magnitude 109-114 F6.3 mag BPmag ?=0.0 Gaia DR2 GBP magnitude 120-124 F5.3 mag e_BPmag ?=0.0 Error on Gaia DR2 GBP magnitude 130-135 F6.3 mag RPmag ?=0.0 Gaia DR2 GRP magnitude 141-145 F5.3 mag e_RPmag ?=0.0 Error on Gaia DR2 GRP magnitude 151-156 F6.3 mag Tmag TESS T magnitude 162-166 F5.3 mag e_Tmag Error on TESS T magnitude 172-177 F6.3 mag Bmag ?=0.0 B Johnson magnitude 183-187 F5.3 mag e_Bmag ?=0.0 Error on B Johnson magnitude 193-198 F6.3 mag Vmag ?=0.0 V Johnson magnitude 204-208 F5.3 mag e_Vmag ?=0.0 Error on V Johnson magnitude 214-219 F6.3 mag Jmag ?=0.0 2MASS J magnitude 225-229 F5.3 mag e_Jmag ?=0.0 Error on 2MASS J magnitude 235-240 F6.3 mag Hmag ?=0.0 2MASS H magnitude 246-250 F5.3 mag e_Hmag ?=0.0 Error on 2MASS H magnitude 256-261 F6.3 mag Kmag ?=0.0 2MASS K magnitude 267-271 F5.3 mag e_Kmag ?=0.0 Error on 2MASS K magnitude 277-282 F6.3 mag W1mag ?=0.0 WISE W1 magnitude 288-292 F5.3 mag e_W1mag ?=0.0 Error on WISE W1 magnitude 298-303 F6.3 mag W2mag ?=0.0 WISE W2 magnitude 309-313 F5.3 mag e_W2mag ?=0.0 Error on WISE W2 magnitude 319-324 F6.3 mag W3mag ?=0.0 WISE W3 magnitude 330-334 F5.3 mag e_W3mag ?=0.0 Error on WISE W3 magnitude 340-345 F6.3 mag W4mag ?=0.0 WISE W4 magnitude 351-355 F5.3 mag e_W4mag Error on WISE W4 magnitude 359-364 F6.4 --- E(B-V) Reddening 369-374 F6.4 mas Plx Parallax from Gaia DR2 376-383 F8.4 mas/yr pmRA Proper motion along RA from Gaia DR2, pmRA*cosDE 385-392 F8.4 mas/yr pmDE Proper motion along Dec from Gaia DR2 410-413 A4 --- Assoc Name of the association that host the star (G1) -------------------------------------------------------------------------------- Global notes: Note (G1): association are ChI, ChII, CrA, Lup and Vel. -------------------------------------------------------------------------------- Acknowledgements: Domenico Nardiello, domenico.nardiello(at)lam.fr References: Nardiello et al., Paper I 2019MNRAS.490.3806N 2019MNRAS.490.3806N, Cat. J/MNRAS/490/3806 Nardiello et al., Paper II 2020MNRAS.495.4924N 2020MNRAS.495.4924N, Cat. J/MNRAS/495/4924
(End) Patricia Vannier [CDS] 23-Oct-2020
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line