The following article is Free article

ERRATUM: Revised Stellar Properties of Kepler Targets for the Q1–17 (DR25) Transit Detection Run (ApJS, 229, 30)

, , , , , , , , , , , , , , , , and

Published 2018 February 14 • © 2018. The American Astronomical Society. All rights reserved.
, , Citation Savita Mathur et al 2018 ApJS 234 43 DOI 10.3847/1538-4365/aaa291

Download Article PDF
DownloadArticle ePub

You need an eReader or compatible software to experience the benefits of the ePub3 file format.

This is a correction for 2017 ApJS 229 30

Article metrics

821 Total downloads

Share this article

Author affiliations

1 Space Science Institute, 4750 Walnut Street Suite #205, Boulder, CO 80301, USA

2 Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia

3 SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA

4 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

5 NASA Ames Research Center, Moffett Field, CA 94035 USA

6 IPAC, Mail Code 100-22, Caltech, 1200 E. California Boulevard, Pasadena, CA 91125 USA

7 Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16803, USA

8 Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, USA

9 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA

10 Niels Bohr Institute, University of Copenhagen, Copenhagen DK-2100, Denmark

11 Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, DK-1350 Copenhagen, Denmark

12 The University of Texas, Austin TX 78712, USA

13 Astronomy Department, University of California Berkeley, CA, US

14 National Optical Astronomy Observatory, 950 N. Cherry Avenue, Tucson, AZ 85719 USA

Author notes

15 Hubble Fellow.

ORCID iDs

Dates

  1. Received 2017 November 10
  2. Revised 2017 December 17
  3. Accepted 2017 December 17
  4. Published

Check for updates using Crossmark

Journal RSS
Create or edit your corridor alerts

What are corridors?opens in new tab

0067-0049/234/2/43

Export citation and abstract BibTeX RIS

Previous article in issue

1. New Stellar Properties for 779 KOI

We report here new stellar properties for 779 Kepler Objects of Interest where an erroneous metallicity value was used in the DR25 Kepler stellar properties catalog (Mathur et al. 2017). This affects all the parameters of these host stars where the metallicity provenance was from the spectroscopic observations and analysis of the Kepler Community Follow-up Program (CFOP, provenance SPE90). The impact is generally small, with radii and masses changing by less than 10% and 20% in general (up to 60% in the masses for a few cases), respectively. Corrected radii are typically smaller than the radii reported in the original paper. Figure 11 of the original paper has been updated and is presented here as Figure 1. The new input and output values are provided in Tables 1 and 2 and have been updated on the NASA exoplanet archive.16

Figure 1.

Figure 1. Comparison of radii and masses of planet host stars between the DR24 (Huber 2014) and the DR25 (Mathur et al. 2017) as a function of effective temperature. The different colors represent the different input values used: DR24 catalog values (black), LAMOST (green), Flicker (blue), CFOP (cyan), and other inputs (pink). The corrected values presented in this erratum only affect CFOP values, and generally result in a decrease in radii by less than 10% and a decrease in mass by less than 20% in general.

Download figure:

Standard image High-resolution image

Table 1.  Input Values of the DR25 Stellar Properties Catalog for the 779 KOI

KIC ${T}_{\mathrm{eff}}$ $\mathrm{log}g$ [Fe/H] ${P}_{\mathrm{Teff}}$ ${P}_{\mathrm{logg}}$ ${P}_{\mathrm{Fe}/{\rm{H}}}$
1429589 6338 ± 80 4.440 ± 0.150 −0.010 ± 0.150 SPE90 SPE90 SPE90
1431122 5295 ± 80 4.320 ± 0.150 0.230 ± 0.150 SPE90 SPE90 SPE90
1432789 5783 ± 80 4.280 ± 0.150 0.150 ± 0.150 SPE90 SPE90 SPE90
1870398 6195 ± 80 4.080 ± 0.150 0.060 ± 0.150 SPE90 SPE90 SPE90
2013883 6221 ± 80 4.070 ± 0.150 0.000 ± 0.150 SPE90 SPE90 SPE90
2019477 5438 ± 80 3.420 ± 0.150 0.100 ± 0.150 SPE90 SPE90 SPE90
2437209 4822 ± 152 3.130 ± 0.150 0.000 ± 0.150 PHO1 SPE90 SPE90
2576962 5864 ± 80 4.280 ± 0.150 0.180 ± 0.150 SPE90 SPE90 SPE90
2693736 5085 ± 80 4.350 ± 0.150 −0.040 ± 0.150 SPE90 SPE90 SPE90
2713049 5523 ± 80 4.350 ± 0.150 −0.040 ± 0.150 SPE90 SPE90 SPE90
2716979 5788 ± 80 3.797 ± 0.200 −0.020 ± 0.150 SPE90 FLK73 SPE90
⋯          

Note. See Table 5 of Mathur et al. (2017) for the reference key for the provenances listed in the last three columns.

Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.

Download table as:  DataTypeset image

Table 2.  Output Values of the DR25 Stellar Properties Catalog for the 779 KOI

KIC ${T}_{\mathrm{eff}}$ (K) $\mathrm{log}g$ [Fe/H] R (R⊙) M (M⊙) ρ d (kpc) AV ${P}_{{\rm{M}},{\rm{R}},\rho }$
1429589 ${6344}_{-82}^{+69}$ 4.396 ± 0.105 ${0.000}_{-0.150}^{+0.150}$ ${1.14}_{-0.07}^{+0.16}$ ${1.18}_{-0.09}^{+0.07}$ ${1.12}_{-0.34}^{+0.16}$ ${0.60}_{-0.04}^{+0.09}$ ${0.36}_{-0.02}^{+0.04}$ DSEP
1431122 ${5300}_{-71}^{+87}$ 4.362 ± 0.096 ${0.240}_{-0.100}^{+0.150}$ ${1.02}_{-0.14}^{+0.14}$ ${0.88}_{-0.03}^{+0.06}$ ${1.16}_{-0.37}^{+0.68}$ ${0.74}_{-0.10}^{+0.11}$ ${0.43}_{-0.05}^{+0.03}$ DSEP
1432789 ${5782}_{-78}^{+78}$ 4.280 ± 0.112 ${0.160}_{-0.150}^{+0.150}$ ${1.22}_{-0.18}^{+0.20}$ ${1.04}_{-0.06}^{+0.08}$ ${0.80}_{-0.27}^{+0.51}$ ${1.34}_{-0.19}^{+0.22}$ ${0.56}_{-0.03}^{+0.02}$ DSEP
1870398 ${6195}_{-80}^{+74}$ 4.089 ± 0.112 ${0.060}_{-0.100}^{+0.150}$ ${1.70}_{-0.38}^{+0.31}$ ${1.29}_{-0.16}^{+0.12}$ ${0.37}_{-0.13}^{+0.33}$ ${1.66}_{-0.37}^{+0.30}$ ${0.59}_{-0.03}^{+0.01}$ DSEP
2013883 ${6225}_{-80}^{+74}$ 4.058 ± 0.098 ${0.000}_{-0.150}^{+0.150}$ ${1.76}_{-0.41}^{+0.27}$ ${1.30}_{-0.19}^{+0.11}$ ${0.33}_{-0.10}^{+0.33}$ ${0.38}_{-0.09}^{+0.06}$ ${0.23}_{-0.06}^{+0.04}$ DSEP
2019477 ${5428}_{-81}^{+81}$ 3.440 ± 0.088 ${0.100}_{-0.150}^{+0.150}$ ${4.28}_{-1.44}^{+0.62}$ ${1.84}_{-0.44}^{+0.15}$ ${0.03}_{-0.01}^{+0.06}$ ${1.78}_{-0.63}^{+0.29}$ ${0.62}_{-0.06}^{+0.01}$ DSEP
2437209 ${4821}_{-77}^{+96}$ 3.125 ± 0.135 ${0.000}_{-0.150}^{+0.150}$ ${4.72}_{-0.93}^{+1.14}$ ${1.08}_{-0.10}^{+0.28}$ ${0.01}_{-0.01}^{+0.01}$ ${5.03}_{-0.87}^{+1.17}$ ${0.52}_{-0.05}^{+0.05}$ DSEP
2576962 ${5872}_{-88}^{+70}$ 4.274 ± 0.108 ${0.180}_{-0.150}^{+0.150}$ ${1.27}_{-0.19}^{+0.21}$ ${1.10}_{-0.09}^{+0.07}$ ${0.76}_{-0.25}^{+0.48}$ ${0.94}_{-0.14}^{+0.14}$ ${0.49}_{-0.04}^{+0.03}$ DSEP
2693736 ${5094}_{-76}^{+83}$ 4.499 ± 0.028 −${0.020}_{-0.100}^{+0.150}$ ${0.82}_{-0.06}^{+0.04}$ ${0.77}_{-0.03}^{+0.06}$ ${1.98}_{-0.21}^{+0.58}$ ${0.70}_{-0.06}^{+0.04}$ ${0.34}_{-0.02}^{+0.01}$ DSEP
2713049 ${5525}_{-74}^{+83}$ 4.345 ± 0.100 −${0.040}_{-0.100}^{+0.150}$ ${1.03}_{-0.16}^{+0.14}$ ${0.86}_{-0.04}^{+0.07}$ ${1.10}_{-0.32}^{+0.75}$ ${0.99}_{-0.16}^{+0.14}$ ${0.49}_{-0.04}^{+0.02}$ DSEP
2716979 ${5787}_{-78}^{+78}$ 3.797 ± 0.112 −${0.020}_{-0.150}^{+0.150}$ ${2.38}_{-0.94}^{+0.43}$ ${1.30}_{-0.29}^{+0.12}$ ${0.14}_{-0.05}^{+0.35}$ ${1.12}_{-0.44}^{+0.20}$ ${0.54}_{-0.13}^{+0.03}$ DSEP

Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.

Download table as:  DataTypeset image

Footnotes

Please wait… references are loading.
10.3847/1538-4365/aaa291