ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations
Autoři
KOKORI, A., A. TSIARAS, B. EDWARDS, A. JONES, G. PANTELIDOU, G. TINETTI, L. BEWERSDORFF, A. ILIADOU, Y. JONGEN, G. LEKKAS, A. NASTASI, E. POULTOURTZIDIS, C. SIDIROPOULOS, F. WALTER, A. WUENSCHE, R. ABRAHAM, V. K. AGNIHOTRI, R. ALBANESI, E. ARCE-MANSEGO, D. ARNOT, M. AUDEJEAN, C. AUMASSON, M. BACHSCHMIDT, G. BAJ, P. R. BARROY, A. A. BELINSKI, D. BENNETT, P. BENNI, K. BERNACKI, L. BETTI, A. BIAGINI, P. BOSCH, P. BRANDEBOURG, L. BRAT, M. BRETTON, S M BRINCAT, S. BROUILLARD, A. BRUZAS, A. BRUZZONE, R. A. BUCKLAND, M. CALO, F. CAMPOS, A. CARRENO, J. A. CARRION RODRIGO, R. CASALI, G. CASALNUOVO, M. CATANEO, C. -M. CHANG, L. CHANGEAT, V. CHOWDHURY, R. CIANTINI, M. CILLUFFO, J. -F. COLIAC, G. CONZO, M. CORREA, G. COULON, N. CROUZET, M. V. CROW, I. A. CURTIS, D. DANIEL, B. DAUCHET, S. DAWES, M. DELDEM, D. DELIGEORGOPOULOS, G. DRANSFIELD, R. DYMOCK, T. EENMAEE, N. ESSEIVA, P. EVANS, C. FALCO, R. G. FARFAN, E. FERNANDEZ-LAJUS, S. FERRATFIAT, S. L. FERREIRA, A. FERRETTI, J. FIOLKA, M. FOWLER, S. R. FUTCHER, D. GABELLINI, T. GAINEY, J. GAITAN, P. GAJDOS, A. GARCIA-SANCHEZ, J. GARLITZ, C. GILLIER, C. GISON, J. GONZALES, D. GORSHANOV, F. GRAU HORTA, G. GRIVAS, P. GUERRA, T. GUILLOT, C. A. HASWELL, T. HAYMES, V. -P. HENTUNEN, K. HILLS, K. HOSE, T. HUMBERT, F. HURTER, T. HYNEK, M. IRZYK, J. JACOBSEN, A. L. JANNETTA, K. JOHNSON, P. JOZWIK-WABIK, A. E. KAEOUACH, W. KANG, H. KIISKINEN, T. KIM, Ue. KIVILA, B. KOCH, U. KOLB, Hana KUČÁKOVÁ (203 Česká republika, domácí), S. -P. LAI, D. LALOUM, S. LASOTA, L. A. LEWIS, G. -I. LIAKOS, F. LIBOTTE, F. LOMOZ, C. LOPRESTI, R. MAJEWSKI, A. MALCHER, M. MALLONN, M. MANNUCCI, A. MARCHINI, J. -M. MARI, A. MARINO, G. MARINO, J. -C. MARIO, J. -B. MARQUETTE, F. A. MARTINEZ-BRAVO, M. MASEK, P. MATASSA, P. MICHEL, J. MICHELET, M. MILLER, E. MINY, D. MOLINA, T. MOLLIER, B. MONTELEONE, N. MONTIGIANI, M. MORALES-AIMAR, F. MORTARI, M. MORVAN, L. V. MUGNAI, G. MURAWSKI, L. NAPONIELLO, J. -L. NAUDIN, R. NAVES, D. NEEL, R. NEITO, S. NEVEU, A. NOSCHESE, Y. OEGMEN, O. OHSHIMA, Z. ORBANIC, E. P. PACE, C. PANTACCHINI, N. I. PASCHALIS, C. PEREIRA, I. PERETTO, V. PERROUD, M. PHILLIPS, P. PINTR, J. -B. PIOPPA, J. PLAZAS, A. J. POELARENDS, A. POPOWICZ, J. PURCELL, N. QUINN, M. RAETZ, D. REES, F. REGEMBAL, M. ROCCHETTO, P. -F. ROCCI, M. ROCKENBAUER, R. ROTH, L. ROUSSELOT, X. RUBIA, N. RUOCCO, E. RUSSO, M. SALISBURY, F. SALVAGGIO, A. SANTOS, J. SAVAGE, F. SCAGGIANTE, D. SEDITA, S. SHADICK, A. F. SILVA, N. SIOULAS, V. SKOLNIK, M. SMITH, M. SMOLKA, A. SOLMAZ, N. STANBURY, D. STOURAITIS, T. -G. TAN, M. THEUSNER, G. THURSTON, F. P. TIFNER, A. TOMACELLI, A. TOMATIS, J. TRNKA, M. TYLSAR, P. VALEAU, J. -P. VIGNES, A. VILLA, A. Vives SUREDA, K. VORA, M. VRASTAK, D. WALLIANG, B. WENZEL, D. E. WRIGHT, R. ZAMBELLI, M. ZHANG a M. ZIBAR
Vydání
Astrophysical Journal Supplement Series, GB - Spojené království Velké Británie a, 2023, 0067-0049
The ExoClock project has been created to increase the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides of Ariel candidates, in order to produce a consistent catalog of reliable and precise ephemerides. This work presents a homogenous catalog of updated ephemerides for 450 planets, generated by the integration of similar to 18,000 data points from multiple sources. These sources include observations from ground-based telescopes (the ExoClock network and the Exoplanet Transit Database), midtime values from the literature, and light curves from space telescopes (Kepler, K2, and TESS). With all the above, we manage to collect observations for half of the postdiscovery years (median), with data that have a median uncertainty less than 1 minute. In comparison with the literature, the ephemerides generated by the project are more precise and less biased. More than 40% of the initial literature ephemerides had to be updated to reach the goals of the project, as they were either of low precision or drifting. Moreover, the integrated approach of the project enables both the monitoring of the majority of the Ariel candidates (95%), and also the identification of missing data. These results highlight the need for continuous monitoring to increase the observing coverage of the candidate planets. Finally, the extended observing coverage of planets allows us to detect trends (transit-timing variations) for a sample of 19 planets. All the products, data, and codes used in this work are open and accessible to the wider scientific community.
KOKORI, A., A. TSIARAS, B. EDWARDS, A. JONES, G. PANTELIDOU, G. TINETTI, L. BEWERSDORFF, A. ILIADOU, Y. JONGEN, G. LEKKAS, A. NASTASI, E. POULTOURTZIDIS, C. SIDIROPOULOS, F. WALTER, A. WUENSCHE, R. ABRAHAM, V. K. AGNIHOTRI, R. ALBANESI, E. ARCE-MANSEGO, D. ARNOT, M. AUDEJEAN, C. AUMASSON, M. BACHSCHMIDT, G. BAJ, P. R. BARROY, A. A. BELINSKI, D. BENNETT, P. BENNI, K. BERNACKI, L. BETTI, A. BIAGINI, P. BOSCH, P. BRANDEBOURG, L. BRAT, M. BRETTON, S M BRINCAT, S. BROUILLARD, A. BRUZAS, A. BRUZZONE, R. A. BUCKLAND, M. CALO, F. CAMPOS, A. CARRENO, J. A. CARRION RODRIGO, R. CASALI, G. CASALNUOVO, M. CATANEO, C. -M. CHANG, L. CHANGEAT, V. CHOWDHURY, R. CIANTINI, M. CILLUFFO, J. -F. COLIAC, G. CONZO, M. CORREA, G. COULON, N. CROUZET, M. V. CROW, I. A. CURTIS, D. DANIEL, B. DAUCHET, S. DAWES, M. DELDEM, D. DELIGEORGOPOULOS, G. DRANSFIELD, R. DYMOCK, T. EENMAEE, N. ESSEIVA, P. EVANS, C. FALCO, R. G. FARFAN, E. FERNANDEZ-LAJUS, S. FERRATFIAT, S. L. FERREIRA, A. FERRETTI, J. FIOLKA, M. FOWLER, S. R. FUTCHER, D. GABELLINI, T. GAINEY, J. GAITAN, P. GAJDOS, A. GARCIA-SANCHEZ, J. GARLITZ, C. GILLIER, C. GISON, J. GONZALES, D. GORSHANOV, F. GRAU HORTA, G. GRIVAS, P. GUERRA, T. GUILLOT, C. A. HASWELL, T. HAYMES, V. -P. HENTUNEN, K. HILLS, K. HOSE, T. HUMBERT, F. HURTER, T. HYNEK, M. IRZYK, J. JACOBSEN, A. L. JANNETTA, K. JOHNSON, P. JOZWIK-WABIK, A. E. KAEOUACH, W. KANG, H. KIISKINEN, T. KIM, Ue. KIVILA, B. KOCH, U. KOLB, Hana KUČÁKOVÁ, S. -P. LAI, D. LALOUM, S. LASOTA, L. A. LEWIS, G. -I. LIAKOS, F. LIBOTTE, F. LOMOZ, C. LOPRESTI, R. MAJEWSKI, A. MALCHER, M. MALLONN, M. MANNUCCI, A. MARCHINI, J. -M. MARI, A. MARINO, G. MARINO, J. -C. MARIO, J. -B. MARQUETTE, F. A. MARTINEZ-BRAVO, M. MASEK, P. MATASSA, P. MICHEL, J. MICHELET, M. MILLER, E. MINY, D. MOLINA, T. MOLLIER, B. MONTELEONE, N. MONTIGIANI, M. MORALES-AIMAR, F. MORTARI, M. MORVAN, L. V. MUGNAI, G. MURAWSKI, L. NAPONIELLO, J. -L. NAUDIN, R. NAVES, D. NEEL, R. NEITO, S. NEVEU, A. NOSCHESE, Y. OEGMEN, O. OHSHIMA, Z. ORBANIC, E. P. PACE, C. PANTACCHINI, N. I. PASCHALIS, C. PEREIRA, I. PERETTO, V. PERROUD, M. PHILLIPS, P. PINTR, J. -B. PIOPPA, J. PLAZAS, A. J. POELARENDS, A. POPOWICZ, J. PURCELL, N. QUINN, M. RAETZ, D. REES, F. REGEMBAL, M. ROCCHETTO, P. -F. ROCCI, M. ROCKENBAUER, R. ROTH, L. ROUSSELOT, X. RUBIA, N. RUOCCO, E. RUSSO, M. SALISBURY, F. SALVAGGIO, A. SANTOS, J. SAVAGE, F. SCAGGIANTE, D. SEDITA, S. SHADICK, A. F. SILVA, N. SIOULAS, V. SKOLNIK, M. SMITH, M. SMOLKA, A. SOLMAZ, N. STANBURY, D. STOURAITIS, T. -G. TAN, M. THEUSNER, G. THURSTON, F. P. TIFNER, A. TOMACELLI, A. TOMATIS, J. TRNKA, M. TYLSAR, P. VALEAU, J. -P. VIGNES, A. VILLA, A. Vives SUREDA, K. VORA, M. VRASTAK, D. WALLIANG, B. WENZEL, D. E. WRIGHT, R. ZAMBELLI, M. ZHANG a M. ZIBAR. ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations. Astrophysical Journal Supplement Series. GB - Spojené království Velké Británie a, 2023, roč. 265, č. 1, s. "4-1"-"4-20", 20 s. ISSN 0067-0049. Dostupné z: https://dx.doi.org/10.3847/1538-4365/ac9da4.
@article{77461, author = {Kokori, A. and Tsiaras, A. and Edwards, B. and Jones, A. and Pantelidou, G. and Tinetti, G. and Bewersdorff, L. and Iliadou, A. and Jongen, Y. and Lekkas, G. and Nastasi, A. and Poultourtzidis, E. and Sidiropoulos, C. and Walter, F. and Wuensche, A. and Abraham, R. and Agnihotri, V. K. and Albanesi, R. and ArceandMansego, E. and Arnot, D. and Audejean, M. and Aumasson, C. and Bachschmidt, M. and Baj, G. and Barroy, P. R. and Belinski, A. A. and Bennett, D. and Benni, P. and Bernacki, K. and Betti, L. and Biagini, A. and Bosch, P. and Brandebourg, P. and Brat, L. and Bretton, M. and Brincat, S M and Brouillard, S. and Bruzas, A. and Bruzzone, A. and Buckland, R. A. and Calo, M. and Campos, F. and Carreno, A. and Carrion Rodrigo, J. A. and Casali, R. and Casalnuovo, G. and Cataneo, M. and Chang, C. andM. and Changeat, L. and Chowdhury, V. and Ciantini, R. and Cilluffo, M. and Coliac, J. andF. and Conzo, G. and Correa, M. and Coulon, G. and Crouzet, N. and Crow, M. V. and Curtis, I. A. and Daniel, D. and Dauchet, B. and Dawes, S. and Deldem, M. and Deligeorgopoulos, D. and Dransfield, G. and Dymock, R. and Eenmaee, T. and Esseiva, N. and Evans, P. and Falco, C. and Farfan, R. G. and FernandezandLajus, E. and Ferratfiat, S. and Ferreira, S. L. and Ferretti, A. and Fiolka, J. and Fowler, M. and Futcher, S. R. and Gabellini, D. and Gainey, T. and Gaitan, J. and Gajdos, P. and GarciaandSanchez, A. and Garlitz, J. and Gillier, C. and Gison, C. and Gonzales, J. and Gorshanov, D. and Grau Horta, F. and Grivas, G. and Guerra, P. and Guillot, T. and Haswell, C. A. and Haymes, T. and Hentunen, V. andP. and Hills, K. and Hose, K. and Humbert, T. and Hurter, F. and Hynek, T. and Irzyk, M. and Jacobsen, J. and Jannetta, A. L. and Johnson, K. and JozwikandWabik, P. and Kaeouach, A. E. and Kang, W. and Kiiskinen, H. and Kim, T. and Kivila, Ue. and Koch, B. and Kolb, U. and Kučáková, Hana and Lai, S. andP. and Laloum, D. and Lasota, S. and Lewis, L. A. and Liakos, G. andI. and Libotte, F. and Lomoz, F. and Lopresti, C. and Majewski, R. and Malcher, A. and Mallonn, M. and Mannucci, M. and Marchini, A. and Mari, J. andM. and Marino, A. and Marino, G. and Mario, J. andC. and Marquette, J. andB. and MartinezandBravo, F. A. and Masek, M. and Matassa, P. and Michel, P. and Michelet, J. and Miller, M. and Miny, E. and Molina, D. and Mollier, T. and Monteleone, B. and Montigiani, N. and MoralesandAimar, M. and Mortari, F. and Morvan, M. and Mugnai, L. V. and Murawski, G. and Naponiello, L. and Naudin, J. andL. and Naves, R. and Neel, D. and Neito, R. and Neveu, S. and Noschese, A. and Oegmen, Y. and Ohshima, O. and Orbanic, Z. and Pace, E. P. and Pantacchini, C. and Paschalis, N. I. and Pereira, C. and Peretto, I. and Perroud, V. and Phillips, M. and Pintr, P. and Pioppa, J. andB. and Plazas, J. and Poelarends, A. J. and Popowicz, A. and Purcell, J. and Quinn, N. and Raetz, M. and Rees, D. and Regembal, F. and Rocchetto, M. and Rocci, P. andF. and Rockenbauer, M. and Roth, R. and Rousselot, L. and Rubia, X. and Ruocco, N. and Russo, E. and Salisbury, M. and Salvaggio, F. and Santos, A. and Savage, J. and Scaggiante, F. and Sedita, D. and Shadick, S. and Silva, A. F. and Sioulas, N. and Skolnik, V. and Smith, M. and Smolka, M. and Solmaz, A. and Stanbury, N. and Stouraitis, D. and Tan, T. andG. and Theusner, M. and Thurston, G. and Tifner, F. P. and Tomacelli, A. and Tomatis, A. and Trnka, J. and Tylsar, M. and Valeau, P. and Vignes, J. andP. and Villa, A. and Sureda, A. Vives and Vora, K. and Vrastak, M. and Walliang, D. and Wenzel, B. and Wright, D. E. and Zambelli, R. and Zhang, M. and Zibar, M.}, article_location = {GB - Spojené království Velké Británie a}, article_number = {1}, doi = {http://dx.doi.org/10.3847/1538-4365/ac9da4}, keywords = {transiting hot Jupiter;optical-transmission spectrum; high-precision phometry; Saturn-mass planet;light-curve project;low-density planet;refined physical-properties;spin-orbit alignment; short-period planet; earth-sized planet}, language = {eng}, issn = {0067-0049}, journal = {Astrophysical Journal Supplement Series}, title = {ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations}, url = {https://iopscience.iop.org/article/10.3847/1538-4365/ac9da4}, volume = {265}, year = {2023} }
TY - JOUR ID - 77461 AU - Kokori, A. - Tsiaras, A. - Edwards, B. - Jones, A. - Pantelidou, G. - Tinetti, G. - Bewersdorff, L. - Iliadou, A. - Jongen, Y. - Lekkas, G. - Nastasi, A. - Poultourtzidis, E. - Sidiropoulos, C. - Walter, F. - Wuensche, A. - Abraham, R. - Agnihotri, V. K. - Albanesi, R. - Arce-Mansego, E. - Arnot, D. - Audejean, M. - Aumasson, C. - Bachschmidt, M. - Baj, G. - Barroy, P. R. - Belinski, A. A. - Bennett, D. - Benni, P. - Bernacki, K. - Betti, L. - Biagini, A. - Bosch, P. - Brandebourg, P. - Brat, L. - Bretton, M. - Brincat, S M - Brouillard, S. - Bruzas, A. - Bruzzone, A. - Buckland, R. A. - Calo, M. - Campos, F. - Carreno, A. - Carrion Rodrigo, J. A. - Casali, R. - Casalnuovo, G. - Cataneo, M. - Chang, C. -M. - Changeat, L. - Chowdhury, V. - Ciantini, R. - Cilluffo, M. - Coliac, J. -F. - Conzo, G. - Correa, M. - Coulon, G. - Crouzet, N. - Crow, M. V. - Curtis, I. A. - Daniel, D. - Dauchet, B. - Dawes, S. - Deldem, M. - Deligeorgopoulos, D. - Dransfield, G. - Dymock, R. - Eenmaee, T. - Esseiva, N. - Evans, P. - Falco, C. - Farfan, R. G. - Fernandez-Lajus, E. - Ferratfiat, S. - Ferreira, S. L. - Ferretti, A. - Fiolka, J. - Fowler, M. - Futcher, S. R. - Gabellini, D. - Gainey, T. - Gaitan, J. - Gajdos, P. - Garcia-Sanchez, A. - Garlitz, J. - Gillier, C. - Gison, C. - Gonzales, J. - Gorshanov, D. - Grau Horta, F. - Grivas, G. - Guerra, P. - Guillot, T. - Haswell, C. A. - Haymes, T. - Hentunen, V. -P. - Hills, K. - Hose, K. - Humbert, T. - Hurter, F. - Hynek, T. - Irzyk, M. - Jacobsen, J. - Jannetta, A. L. - Johnson, K. - Jozwik-Wabik, P. - Kaeouach, A. E. - Kang, W. - Kiiskinen, H. - Kim, T. - Kivila, Ue. - Koch, B. - Kolb, U. - Kučáková, Hana - Lai, S. -P. - Laloum, D. - Lasota, S. - Lewis, L. A. - Liakos, G. -I. - Libotte, F. - Lomoz, F. - Lopresti, C. - Majewski, R. - Malcher, A. - Mallonn, M. - Mannucci, M. - Marchini, A. - Mari, J. -M. - Marino, A. - Marino, G. - Mario, J. -C. - Marquette, J. -B. - Martinez-Bravo, F. A. - Masek, M. - Matassa, P. - Michel, P. - Michelet, J. - Miller, M. - Miny, E. - Molina, D. - Mollier, T. - Monteleone, B. - Montigiani, N. - Morales-Aimar, M. - Mortari, F. - Morvan, M. - Mugnai, L. V. - Murawski, G. - Naponiello, L. - Naudin, J. -L. - Naves, R. - Neel, D. - Neito, R. - Neveu, S. - Noschese, A. - Oegmen, Y. - Ohshima, O. - Orbanic, Z. - Pace, E. P. - Pantacchini, C. - Paschalis, N. I. - Pereira, C. - Peretto, I. - Perroud, V. - Phillips, M. - Pintr, P. - Pioppa, J. -B. - Plazas, J. - Poelarends, A. J. - Popowicz, A. - Purcell, J. - Quinn, N. - Raetz, M. - Rees, D. - Regembal, F. - Rocchetto, M. - Rocci, P. -F. - Rockenbauer, M. - Roth, R. - Rousselot, L. - Rubia, X. - Ruocco, N. - Russo, E. - Salisbury, M. - Salvaggio, F. - Santos, A. - Savage, J. - Scaggiante, F. - Sedita, D. - Shadick, S. - Silva, A. F. - Sioulas, N. - Skolnik, V. - Smith, M. - Smolka, M. - Solmaz, A. - Stanbury, N. - Stouraitis, D. - Tan, T. -G. - Theusner, M. - Thurston, G. - Tifner, F. P. - Tomacelli, A. - Tomatis, A. - Trnka, J. - Tylsar, M. - Valeau, P. - Vignes, J. -P. - Villa, A. - Sureda, A. Vives - Vora, K. - Vrastak, M. - Walliang, D. - Wenzel, B. - Wright, D. E. - Zambelli, R. - Zhang, M. - Zibar, M. PY - 2023 TI - ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations JF - Astrophysical Journal Supplement Series VL - 265 IS - 1 SP - "4-1"-"4-20" EP - "4-1"-"4-20" SN - 00670049 KW - transiting hot Jupiter;optical-transmission spectrum KW - high-precision phometry KW - Saturn-mass planet;light-curve project;low-density planet;refined physical-properties;spin-orbit alignment KW - short-period planet KW - earth-sized planet UR - https://iopscience.iop.org/article/10.3847/1538-4365/ac9da4 N2 - The ExoClock project has been created to increase the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides of Ariel candidates, in order to produce a consistent catalog of reliable and precise ephemerides. This work presents a homogenous catalog of updated ephemerides for 450 planets, generated by the integration of similar to 18,000 data points from multiple sources. These sources include observations from ground-based telescopes (the ExoClock network and the Exoplanet Transit Database), midtime values from the literature, and light curves from space telescopes (Kepler, K2, and TESS). With all the above, we manage to collect observations for half of the postdiscovery years (median), with data that have a median uncertainty less than 1 minute. In comparison with the literature, the ephemerides generated by the project are more precise and less biased. More than 40% of the initial literature ephemerides had to be updated to reach the goals of the project, as they were either of low precision or drifting. Moreover, the integrated approach of the project enables both the monitoring of the majority of the Ariel candidates (95%), and also the identification of missing data. These results highlight the need for continuous monitoring to increase the observing coverage of the candidate planets. Finally, the extended observing coverage of planets allows us to detect trends (transit-timing variations) for a sample of 19 planets. All the products, data, and codes used in this work are open and accessible to the wider scientific community. ER -
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