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J/A+A/607/A127     2014-2017 photometry for ASASSN-13db (Sicilia-Aguilar+, 2017)

The 2014-2017 outburst of the young star ASASSN-13db. Sicilia-Aguilar A., Oprandi A., Froebrich D., Fang M., Prieto J.L., Stanek K., Scholz A., Kochanek C.S., Henning T., Gredel R., Holoien T.S.W., Rabus M., Shappee B.J., Billington S.J., Campbell-White J., Zegmott T.J. <Astron. Astrophys. 607, A127 (2017)> =2017A&A...607A.127S (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Stars, pre-main sequence ; Photometry Keywords: stars: pre-main sequence - stars: T Tauri, Herbig Ae/Be - stars: individual: ASASSN-13db - stars: low-mass - protoplanetary disks - accretion - techniques: spectroscopic Abstract: Accretion outbursts are key elements in star formation. ASASSN-13db is a M5-type star with a protoplanetary disk, the lowest-mass star known to experience accretion outbursts. Since its discovery in 2013, it has experienced two outbursts, the second of which started in November 2014 and lasted until February 2017. We explore the photometric and spectroscopic behavior of ASASSN-13db during the 2014-2017 outburst. We use high- and low-resolution spectroscopy and time-resolved photometry from the ASAS-SN survey, the LCOGT and the Beacon Observatory to study the lightcurve of ASASSN-13db and the dynamical and physical properties of the accretion flow. Results. The 2014-2017 outburst lasted for nearly 800 days. A 4.15d period in the light curve likely corresponds to rotational modulation of a star with hot spot(s). The spectra show multiple emission lines with variable inverse P-Cygni profiles and a highly variable blue-shifted absorption below the continuum. Line ratios from metallic emission lines (FeI/FeII, TiI/TiII) suggest temperatures of ∼5800-6000K in the accretion flow. Description: Table 1 contains the full photometry from the All Sky Automated Survey for Supernovae (ASAS-SN) for the variable star ASASSN-13db. Detections with their errors and 5-sigma upper limits are given. Upper limits are marked by the "<" sign and have the error column set to 99.99. Objects: ------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------ 05 10 11.08 -03 28 26.3 ASASSN-13db = ASASSN -13db ------------------------------------------------------ File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 27 1017 ASAS-SN photometry for ASASSN-13db
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 13 F13.5 d HJD Heliocentric Julian Day 15 A1 --- l_Vmag Upper limit sign on Vmag 17- 21 F5.2 mag Vmag V magnitude 23- 27 F5.2 mag e_Vmag ?=99.99 Error in V magnitude, set to 99.99 for upper limits
Acknowledgements: Aurora Sicilia-Aguilar, a.siciliaaguilar(at)dundee.ac.uk
(End) Aurora Sicilia-Aguilar [Dundee], Patricia Vannier [CDS] 17-Aug-2017
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

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