Zobrazeno 1 - 10
of 76
pro vyhledávání: '"Yahalomi, Daniel"'
Autor:
Yahalomi, Daniel A., Kipping, David
There are now thousands of single-planet systems observed to exhibit transit timing variations (TTVs), yet we largely lack any interpretation of the implied masses responsible for these perturbations. Even when assuming these TTVs are driven by pertu
Externí odkaz:
http://arxiv.org/abs/2411.10493
Autor:
Yahalomi, Daniel A., Kipping, David, Solano-Oropeza, Diana, Li, Madison, Poddar, Avishi, Xunhe, Zhang, Abaakil, Yassine, Cassese, Benjamin, Teachey, Alex, Liu, Jiajing, Sundai, Farai, Valaskovic, Lila
Accurate, precise, and computationally efficient removal of unwanted activity that exists as a combination of periodic, quasi-periodic, and non-periodic systematic trends in time-series photometric data is a critical step in exoplanet transit analysi
Externí odkaz:
http://arxiv.org/abs/2411.09753
Transit timing variations (TTVs) are observed for exoplanets at a range of amplitudes and periods, yielding an ostensibly degenerate forest of possible explanations. We offer some clarity in this forest, showing that systems with a distant perturbing
Externí odkaz:
http://arxiv.org/abs/2411.09752
Autor:
Kipping, David, Teachey, Alex, Yahalomi, Daniel A., Cassese, Ben, Quarles, Billy, Bryson, Steve, Hansen, Brad, Szulágyi, Judit, Burke, Chris, Hardegree-Ullman, Kevin
Recently, Heller & Hippke argued that the exomoon candidates Kepler-1625 b-i and Kepler-1708 b-i were allegedly 'refuted'. In this Matters Arising, we address these claims. For Kepler-1625 b, we show that their Hubble light curve is identical to that
Externí odkaz:
http://arxiv.org/abs/2401.10333
Autor:
Yahalomi, Daniel A., Kipping, David, Nesvorný, David, Dalba, Paul A., Benni, Paul, Cacho-Negrete, Ceiligh, Collins, Karen, Earwicker, Joel T., Lewis, John Arban, McLeod, Kim K., Schwarz, Richard P., Wang, Gavin
Transit Timing Variations (TTVs) can be induced by a range of physical phenomena, including planet-planet interactions, planet-moon interactions, and stellar activity. Recent work has shown that roughly half of moons would induce fast TTVs with a sho
Externí odkaz:
http://arxiv.org/abs/2310.03802
Autor:
Grunblatt, Samuel K., Wilson, Robert F., Winter, Andrew, Gaudi, B. Scott, Huber, Daniel, Yahalomi, Daniel A., Bellini, Andrea, Claytor, Zachary R., Palomera, Jorge Martinez, Barclay, Thomas, Fu, Guangwei, Price-Whelan, Adrian
Despite multiple previous searches, no transiting planets have yet been identified within a globular cluster. This is believed to be due to a combination of factors: the low metallicities of most globular clusters suggests that there is significantly
Externí odkaz:
http://arxiv.org/abs/2306.10647
Earth-mass exoplanets on year-long orbits and cool gas giants (CGG) on decade-long orbits lie at the edge of current detection limits. The Terra Hunting Experiment (THE) will take nightly radial velocity (RV) observations on HARPS3 of at least 40 bri
Externí odkaz:
http://arxiv.org/abs/2302.05064
Autor:
Kipping, David, Yahalomi, Daniel A.
An exomoon will produce transit timing variations (TTVs) upon the parent planet and their undersampled nature causes half of such TTVs to manifest within a frequency range of 2 to 4 cycles, irrespective of exomoon demographics. Here, we search throug
Externí odkaz:
http://arxiv.org/abs/2211.06210
Autor:
Christian, Sam, Vanderburg, Andrew, Becker, Juliette, Yahalomi, Daniel A., Pearce, Logan, Zhou, George, Collins, Karen A., Kraus, Adam L., Stassun, Keivan G., de Beurs, Zoe, Ricker, George R., Vanderspek, Roland K., Latham, David W., Winn, Joshua N., Seager, S., Jenkins, Jon M., Abe, Lyu, Agabi, Karim, Amado, Pedro J., Baker, David, Barkaoui, Khalid, Benkhaldoun, Zouhair, Benni, Paul, Berberian, John, Berlind, Perry, Bieryla, Allyson, Esparza-Borges, Emma, Bowen, Michael, Brown, Peyton, Buchhave, Lars A., Burke, Christopher J., Buttu, Marco, Cadieux, Charles, Caldwell, Douglas A., Charbonneau, David, Chazov, Nikita, Chimaladinne, Sudhish, Collins, Kevin I., Combs, Deven, Conti, Dennis M., Crouzet, Nicolas, de Leon, Jerome P., Deljookorani, Shila, Diamond, Brendan, Doyon, René, Dragomir, Diana, Dransfield, Georgina, Essack, Zahra, Evans, Phil, Fukui, Akihiko, Gan, Tianjun, Esquerdo, Gilbert A., Gillon, Michaël, Girardin, Eric, Guerra, Pere, Guillot, Tristan, Habich, Eleanor Kate K., Henriksen, Andreea, Hoch, Nora, Isogai, Keisuke I, Jehin, Emmanuël, Jensen, Eric L. N., Johnson, Marshall C., Livingston, John H., Kielkopf, John F., Kim, Kingsley, Kawauchi, Kiyoe, Krushinsky, Vadim, Kunzle, Veronica, Laloum, Didier, Leger, Dominic, Lewin, Pablo, Mallia, Franco, Massey, Bob, Mori, Mayuko, McLeod, Kim K., Mékarnia, Djamel, Mireles, Ismael, Mishevskiy, Nikolay, Tamura, Motohide, Murgas, Felipe, Narita, Norio, Naves, Ramon, Nelson, Peter, Osborn, Hugh P., Palle, Enric, Parviainen, Hannu, Plavchan, Peter, Pozuelos, Francisco J., Rabus, Markus, Relles, Howard M., López, Cristina Rodríguez, Quinn, Samuel N., Schmider, Francois-Xavier, Schlieder, Joshua E., Schwarz, Richard P., Shporer, Avi, Sibbald, Laurie, Srdoc, Gregor, Stibbards, Caitlin, Stickler, Hannah, Suarez, Olga, Stockdale, Chris, Tan, Thiam-Guan, Terada, Yuka, Triaud, Amaury, Tronsgaard, Rene, Waalkes, William C., Wang, Gavin, Watanabe, Noriharu, Wenceslas, Marie-Sainte, Wingham, Geof, Wittrock, Justin, Ziegler, Carl
Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 AU) on the formation and evolution of exoplanets. We investigate these effects using new data from Gaia EDR3 and the TESS mission to
Externí odkaz:
http://arxiv.org/abs/2202.00042
Autor:
Giacalone, Steven, Dressing, Courtney D., Hedges, Christina, Kostov, Veselin B., Collins, Karen A., Jensen, Eric L. N., Yahalomi, Daniel A., Bieryla, Allyson, Ciardi, David R., Howell, Steve B., Lillo-Box, Jorge, Barkaoui, Khalid, Winters, Jennifer G., Matthews, Elisabeth, Livingston, John H., Quinn, Samuel N., Safonov, Boris S., Cadieux, Charles, Furlan, E., Crossfield, Ian J. M., Mandell, Avi M., Gilbert, Emily A., Kruse, Ethan, Quintana, Elisa V., Ricker, George R., Seager, S., Winn, Joshua N., Jenkins, Jon M., Adkins, Britt Duffy, Baker, David, Barclay, Thomas, Barrado, David, Batalha, Natalie M., Belinski, Alexander A., Benkhaldoun, Zouhair, Buchhave, Lars A., Cacciapuoti, Luca, Charbonneau, David, Chontos, Ashley, Christiansen, Jessie L., Cloutier, Ryan, Collins, Kevin I., Conti, Dennis M., Cutting, Neil, Dixon, Scott, Doyon, René, Mufti, Mohammed El, Esparza-Borges, Emma, Essack, Zahra, Fukui, Akihiko, Gan, Tianjun, Gary, Kaz, Ghachoui, Mourad, Gillon, Michaël, Girardin, Eric, Glidden, Ana, Gonzales, Erica J., Guerra, Pere, Horch, Elliott P., Helminiak, Krzysztof G., Howard, Andrew W., Huber, Daniel, Irwin, Jonathan M., Isopi, Giovanni, Jehin, Emmanuël, Kagetani, Taiki, Kane, Stephen R., Kawauchi, Kiyoe, Kielkopf, John F., Lewin, Pablo, Luker, Lindy, Lund, Michael B., Mallia, Franco, Mao, Shude, Massey, Bob, Matson, Rachel A., Mireles, Ismael, Mori, Mayuko, Murgas, Felipe, Narita, Norio, O`Dwyer, Tanner, Petigura, Erik A., Polanski, Alex S., Pozuelos, Francisco J., Palle, Enric, Parviainen, Hannu, Plavchan, Peter P., Relles, Howard M., Robertson, Paul, Rose, Mark E., Rowden, Pamela, Roy, Arpita, Savel, Arjun B., Schlieder, Joshua E., Schnaible, Chloe, Schwarz, Richard P., Sefako, Ramotholo, Selezneva, Aleksandra, Skinner, Brett, Stockdale, Chris, Strakhov, Ivan A., Tan, Thiam-Guan, Torres, Guillermo, Tronsgaard, René, Twicken, Joseph D., Vermilion, David, Waite, Ian A., Walter, Bradley, Wang, Gavin, Ziegler, Carl, Zou, Yujie
Publikováno v:
AJ 163 99 (2022)
The James Webb Space Telescope (JWST) will be able to probe the atmospheres and surface properties of hot, terrestrial planets via emission spectroscopy. We identify 18 potentially terrestrial planet candidates detected by the Transiting Exoplanet Su
Externí odkaz:
http://arxiv.org/abs/2201.12661