The DOI matches its Crossref record; 11 of the 11 references it cites were found in a registry or an index.
THE OCCURRENCE OF POTENTIALLY HABITABLE PLANETS ORBITING M DWARFS ESTIMATED FROM THE FULL KEPLER DATASET AND AN EMPIRICAL MEASUREMENT OF THE DETECTION SENSITIVITY
Open accessAbstract
We present an improved estimate of the occurrence rate of small planets orbiting small stars by searching the full four-year Kepler data set for transiting planets using our own planet detection pipeline and conducting transit injection and recovery simulations to empirically measure the search completeness of our pipeline. We identified 156 planet candidates, including one object that was not previously identified as a Kepler Object of Interest. We inspected all publicly available follow-up images, observing notes, and centroid analyses, and corrected for the likelihood of false positives. We evaluated the sensitivity of our detection pipeline on a star-by-star basis by injecting 2000 transit signals into the light curve of each target star. For periods shorter than 50 days, we find Earth-size planets (1−1.5 R ⊕ ) and super-Earths (1.5−2 R ⊕ ) per M dwarf. In total, we estimate a cumulative planet occurrence rate of 2.5 ± 0.2 planets per M dwarf with radii 1−4 R ⊕ and periods shorter than 200 days. Within a conservatively defined habitable zone (HZ) based on the moist greenhouse inner limit and maximum greenhouse outer limit, we estimate an occurrence rate of Earth-size planets and super-Earths per M dwarf HZ. Adopting the broader insolation boundaries of the recent Venus and early Mars limits yields a higher estimate of Earth-size planets and super-Earths per M dwarf HZ. This suggests that the nearest potentially habitable non-transiting and transiting Earth-size planets are 2.6 ± 0.4 pc and pc away, respectively. If we include super-Earths, these distances diminish to 2.1 ± 0.2 pc and pc.
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Cites
Equation of State Calculations by Fast Computing Machines
Metropolis, N., Rosenbluth, A. W., Rosenbluth, M. N., Teller, A. H., & Teller, E. (1953) · The Journal of Chemical Physics · doi:10.1063/1.1699114 · Cited by 37,192
Gelman, A., Carlin, J. B., Stern, H. S., & Rubin, D. B. (2003) · doi:10.1201/9780429258480 · Cited by 27,276
Kepler planet-detection mission: Introduction and first results
Borucki, W. J., Koch, D., Basri, G., Batalha, N., Brown, T., Caldwell, D., Caldwell, J., Christensen-Dalsgaard, J., Cochran, W. D., DeVore, E., et al. (2010) · Science · doi:10.1126/science.1185402 · Cited by 4,035
Self-citationHabitable Zones around Main Sequence Stars
Kasting, J. F., Whitmire, D. P., & Reynolds, R. T. (1993) · Icarus · doi:10.1006/icar.1993.1010 · Cited by 2,501 · cited 2×
“Using conservative habitable zone limits from Kasting et al. (1993), we estimated an occurrence rate of 0.15 potentially habitable Earthsize (0.5 − 1.4R⊕) planets per small star.”
BackgroundInfluentialHABITABLE ZONES AROUND MAIN-SEQUENCE STARS: NEW ESTIMATES
Kopparapu, R. K., Ramirez, R., Kasting, J. F., Eymet, V., Robinson, T. D., Mahadevan, S., Terrien, R. C., Domagal-Goldman, S., Meadows, V., & Deshpande, R. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/765/2/131 · Cited by 1,615 · cited 7×
“In the most conservative case, we adopt the maximum greenhouse (Max GH) and moist greenhouse (Moist GH) insolation limits from Kopparapu et al. (2013b).”
BackgroundMethodInfluentialBorucki, W. J., Koch, D. G., Basri, G., Batalha, N., Brown, T. M., Bryson, S. T., Caldwell, D., Christensen-Dalsgaard, J., Cochran, W. D., DeVore, E., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/736/1/19 · Cited by 1,042
Self-citationA box-fitting algorithm in the search for periodic transits
Kovács, G., Zucker, S., & Mazeh, T. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20020802 · Cited by 995 · cited 1×
“We then determined the signal detection efficiency (SDE) for each possible signal in the composite periodogram using Equation 6 in Kovács et al. (2002).”
MethodUNDERSTANDING THE MASS-RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION
Lopez, E. D., & Fortney, J. J. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/792/1/1 · Cited by 722
THE MASS-RADIUS RELATION FOR 65 EXOPLANETS SMALLER THAN 4 EARTH RADII
Weiss, L. M., & Marcy, G. W. (2014) · The Astrophysical Journal · doi:10.1088/2041-8205/783/1/l6 · Cited by 665
HYDROGEN GREENHOUSE PLANETS BEYOND THE HABITABLE ZONE
Pierrehumbert, R., & Gaidos, E. (2011) · The Astrophysical Journal · doi:10.1088/2041-8205/734/1/l13 · Cited by 295 · cited 2×
“We do not provide an estimate based on the hydrogen atmosphere HZ of Pierrehumbert & Gaidos (2011) because our search completeness is very low at the maximum allowed separation of 2.4 AU.”
BackgroundInfluentialHABITABLE CLIMATES: THE INFLUENCE OF OBLIQUITY
Spiegel, D. S., Menou, K., & Scharf, C. A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/691/1/596 · Cited by 164
Cited by
Dawson, R. I., & Johnson, J. A. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051853 · Cited by 622
BREEDING SUPER-EARTHS AND BIRTHING SUPER-PUFFS IN TRANSITIONAL DISKS
Lee, E. J., & Chiang, E. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/817/2/90 · Cited by 317
Optimized transit detection algorithm to search for periodic transits of small planets
Hippke, M., & Heller, R. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201834672 · Cited by 250
ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS
Cuntz, M., & Guinan, E. F. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/827/1/79 · Cited by 77
“%) of red dwarfs is expected to host terrestrial-size planets within their CLI-HZs (e.g., Bonfils et al. 2013; Dressing & Charbonneau 2013, 2015).”
BackgroundGuinan, E. F., Engle, S. G., & Durbin, A. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/821/2/81 · Cited by 77
Metadata
- Authors
- Dressing, C. D., & Charbonneau, D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2015-06-30
- Volume
- 807
- Issue
- 1
- Pages
- 45
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2963604282
- Cited by
- 1,012
- References
- 11
- FWCI
- 61.93
- Type
- journal article
- Language
- en
- Open access
- bronze
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