Zobrazeno 1 - 10
of 112
pro vyhledávání: '"Howard Isaacson"'
Autor:
Malena Rice, Songhu Wang, Konstantin Gerbig, Xian-Yu Wang, Fei Dai, Dakotah Tyler, Howard Isaacson, Andrew W. Howard
The evolutionary history of an extrasolar system is, in part, fossilized through its planets’ orbital orientations relative to the host star’s spin axis. However, spin–orbit constraints for warm Jupiters—particularly in binary star systems, w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c20a1f6b54b7781b794233a58aea714
https://resolver.caltech.edu/CaltechAUTHORS:20230314-845495900.62
https://resolver.caltech.edu/CaltechAUTHORS:20230314-845495900.62
Autor:
Samuel K. Grunblatt, Nicholas Saunders, Ashley Chontos, Soichiro Hattori, Dimitri Veras, Daniel Huber, Ruth Angus, Malena Rice, Katelyn Breivik, Sarah Blunt, Steven Giacalone, Jack Lubin, Howard Isaacson, Andrew W. Howard, David R. Ciardi, Boris S. Safonov, Ivan A. Strakhov, David W. Latham, Allyson Bieryla, George R. Ricker, Jon M. Jenkins, Peter Tenenbaum, Avi Shporer, Edward H. Morgan, Veselin Kostov, Hugh P. Osborn, Diana Dragomir, Sara Seager, Roland K. Vanderspek, Joshua N. Winn
The fate of planets around rapidly evolving stars is not well understood. Previous studies have suggested that relative to the main sequence population, planets transiting evolved stars ($P$ $
21 pages, 11 figures, favorably reviewed by AAS Jour
21 pages, 11 figures, favorably reviewed by AAS Jour
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4766a89dc3af8bfa2a84b925d47cbbe4
https://resolver.caltech.edu/CaltechAUTHORS:20230330-579847500.10
https://resolver.caltech.edu/CaltechAUTHORS:20230330-579847500.10
Autor:
Stephen R. Kane, Michelle L. Hill, Paul A. Dalba, Tara Fetherolf, Gregory W. Henry, Sergio B. Fajardo-Acosta, Crystal L. Gnilka, Andrew W. Howard, Steve B. Howell, Howard Isaacson
Publikováno v:
The Astronomical Journal. 165:252
From the thousands of known exoplanets, those that transit bright host stars provide the greatest accessibility toward detailed system characterization. The first known such planets were generally discovered using the radial velocity technique, then
Autor:
Emma V. Turtelboom, Lauren M. Weiss, Courtney D. Dressing, Grzegorz Nowak, Enric Pallé, Corey Beard, Sarah Blunt, Casey Brinkman, Ashley Chontos, Zachary R. Claytor, Fei Dai, Paul A. Dalba, Steven Giacalone, Erica Gonzales, Caleb K. Harada, Michelle L. Hill, Rae Holcomb, Judith Korth, Jack Lubin, Thomas Masseron, Mason MacDougall, Andrew W. Mayo, Teo Močnik, Joseph M. Akana Murphy, Alex S. Polanski, Malena Rice, Ryan A. Rubenzahl, Nicholas Scarsdale, Keivan G. Stassun, Dakotah B. Tyler, Judah Van Zandt, Ian J. M. Crossfield, Hans J. Deeg, Benjamin Fulton, Davide Gandolfi, Andrew W. Howard, Dan Huber, Howard Isaacson, Stephen R. Kane, Kristine W. F. Lam, Rafael Luque, Eduardo L. Martín, Giuseppe Morello, Jaume Orell-Miquel, Erik A. Petigura, Paul Robertson, Arpita Roy, Vincent Van Eylen, David Baker, Alexander A. Belinski, Allyson Bieryla, David R. Ciardi, Karen A. Collins, Neil Cutting, Devin J. Della-Rose, Taylor B. Ellingsen, E. Furlan, Tianjun Gan, Crystal L. Gnilka, Pere Guerra, Steve B. Howell, Mary Jimenez, David W. Latham, Maude Larivière, Kathryn V. Lester, Jorge Lillo-Box, Lindy Luker, Christopher R. Mann, Peter P. Plavchan, Boris Safonov, Brett Skinner, Ivan A. Strakhov, Justin M. Wittrock, Douglas A. Caldwell, Zahra Essack, Jon M. Jenkins, Elisa V. Quintana, George R. Ricker, Roland Vanderspek, S. Seager, Joshua N. Winn
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Turtelboom, E, Weiss, L M, Dressing, C D, Nowak, G, Palle, E, Beard, C, Blunt, S, Brinkman, C, Chontos, A, Claytor, Z R, Dai, F, Dalba, P A, Giacalone, S, Gonzales, E, Harada, C K, Hill, M L, Holcomb, R, Korth, J, Lubin, J, Masseron, T, MacDougall, M, Mayo, A W, Mocnik, T, Murphy, J M A, Polanski, A S, Rice, M, Rubenzahl, R A, Scarsdale, N, Stassun, K G, Tyler, D B, Van Zandt, J, Crossfield, I J M, Deeg, H J, Fulton, B, Gandolfi, D, Howard, A W, Huber, D, Isaacson, H, Kane, S R, Lam, K W F, Luque, R, Martin, E L, Morello, G, Orell-Miquel, J, Petigura, E A, Robertson, P, Roy, A, Van Eylen, V, Baker, D, Belinski, A A, Bieryla, A, Ciardi, D R, Collins, K A, Cutting, N, Della-Rose, D J, Ellingsen, T B, Furlan, E, Gan, T, Gnilka, C L, Guerra, P, Howell, S B, Jimenez, M, Latham, D W, Lariviere, M, Lester, K, Lillo-Box, J, Luker, L, Mann, C R, Plavchan, P P, Safonov, B, Skinner, B, Strakhov, I A, Wittrock, J M, Caldwell, D A, Essack, Z, Jenkins, J M, Quintana, E, Ricker, G R, Vanderspek, R, Seager, S & Winn, J N 2022, ' The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI-1246 ', Astronomical Journal, vol. 163, no. 6, 293 . https://doi.org/10.3847/1538-3881/ac69e5
instname
Turtelboom, E, Weiss, L M, Dressing, C D, Nowak, G, Palle, E, Beard, C, Blunt, S, Brinkman, C, Chontos, A, Claytor, Z R, Dai, F, Dalba, P A, Giacalone, S, Gonzales, E, Harada, C K, Hill, M L, Holcomb, R, Korth, J, Lubin, J, Masseron, T, MacDougall, M, Mayo, A W, Mocnik, T, Murphy, J M A, Polanski, A S, Rice, M, Rubenzahl, R A, Scarsdale, N, Stassun, K G, Tyler, D B, Van Zandt, J, Crossfield, I J M, Deeg, H J, Fulton, B, Gandolfi, D, Howard, A W, Huber, D, Isaacson, H, Kane, S R, Lam, K W F, Luque, R, Martin, E L, Morello, G, Orell-Miquel, J, Petigura, E A, Robertson, P, Roy, A, Van Eylen, V, Baker, D, Belinski, A A, Bieryla, A, Ciardi, D R, Collins, K A, Cutting, N, Della-Rose, D J, Ellingsen, T B, Furlan, E, Gan, T, Gnilka, C L, Guerra, P, Howell, S B, Jimenez, M, Latham, D W, Lariviere, M, Lester, K, Lillo-Box, J, Luker, L, Mann, C R, Plavchan, P P, Safonov, B, Skinner, B, Strakhov, I A, Wittrock, J M, Caldwell, D A, Essack, Z, Jenkins, J M, Quintana, E, Ricker, G R, Vanderspek, R, Seager, S & Winn, J N 2022, ' The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI-1246 ', Astronomical Journal, vol. 163, no. 6, 293 . https://doi.org/10.3847/1538-3881/ac69e5
Full list of authors: Turtelboom, Emma V.; Weiss, Lauren M.; Dressing, Courtney D.; Nowak, Grzegorz; Pallé, Enric; Beard, Corey; Blunt, Sarah; Brinkman, Casey; Chontos, Ashley; Claytor, Zachary R.; Dai, Fei; Dalba, Paul A.; Giacalone, Steven; Gonzal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46cd7e5841a2687b64e662da98d1bdf2
https://resolver.caltech.edu/CaltechAUTHORS:20220517-214311999
https://resolver.caltech.edu/CaltechAUTHORS:20220517-214311999
Autor:
Anna Zuckerman, Zoe Ko, Howard Isaacson, Steve Croft, Danny Price, Matt Lebofsky, Andrew Siemion
Publikováno v:
The Astronomical Journal. 165:114
The Search for Extraterrestrial Intelligence (SETI) has traditionally been conducted at radio wavelengths, but optical searches are well-motivated and increasingly feasible due to the growing availability of high-resolution spectroscopy. We present a
Autor:
Jennifer G. Winters, Ryan Cloutier, Amber A. Medina, Jonathan M. Irwin, David Charbonneau, Nicola Astudillo-Defru, Xavier Bonfils, Andrew W. Howard, Howard Isaacson, Jacob L. Bean, Andreas Seifahrt, Johanna K. Teske, Jason D. Eastman, Joseph D. Twicken, Karen A. Collins, Eric L. N. Jensen, Samuel N. Quinn, Matthew J. Payne, Martti H. Kristiansen, Alton Spencer, Andrew Vanderburg, Mathias Zechmeister, Lauren M. Weiss, Sharon Xuesong Wang, Gavin Wang, Stéphane Udry, Ivan A. Terentev, Julian Stürmer, Gudmundur Stefánsson, Avi Shporer, Stephen Shectman, Ramotholo Sefako, Hans Martin Schwengeler, Richard P. Schwarz, Nicholas Scarsdale, Ryan A. Rubenzahl, Arpita Roy, Lee J. Rosenthal, Paul Robertson, Erik A. Petigura, Francesco Pepe, Mark Omohundro, Joseph M. Akana Murphy, Felipe Murgas, Teo Močnik, Benjamin T. Montet, Ronald Mennickent, Andrew W. Mayo, Bob Massey, Jack Lubin, Christophe Lovis, Pablo Lewin, David Kasper, Stephen R. Kane, Jon M. Jenkins, Daniel Huber, Keith Horne, Michelle L. Hill, Paula Gorrini, Steven Giacalone, Benjamin Fulton, Thierry Forveille, Pedro Figueira, Tara Fetherolf, Courtney Dressing, Rodrigo F. Díaz, Xavier Delfosse, Paul A. Dalba, Fei Dai, C. C. Cortés, Ian J. M. Crossfield, Jeffrey D. Crane, Dennis M. Conti, Kevin I. Collins, Ashley Chontos, R. Paul Butler, Peyton Brown, Madison Brady, Aida Behmard, Corey Beard, Natalie M. Batalha, Jose-Manuel Almenara
Publikováno v:
Winters, J G, Cloutier, R, Medina, A A, Irwin, J M, Charbonneau, D, Astudillo-Defru, N, Bonfils, X, Howard, A W, Isaacson, H, Bean, J L, Seifahrt, A, Teske, J K, Eastman, J D, Twicken, J D, Collins, K A, Jensen, E L N, Quinn, S N, Payne, M J, Kristiansen, M H, Spencer, A, Vanderburg, A, Zechmeister, M, Weiss, L M, Wang, S X, Wang, G, Udry, S, Terentev, I A, Stürmer, J, Stefánsson, G, Shporer, A, Shectman, S, Sefako, R, Schwengeler, H M, Schwarz, R P, Scarsdale, N, Rubenzahl, R A, Roy, A, Rosenthal, L J, Robertson, P, Petigura, E A, Pepe, F, Omohundro, M, Murphy, J M A, Murgas, F, Močnik, T, Montet, B T, Mennickent, R, Mayo, A W, Massey, B, Lubin, J, Lovis, C, Lewin, P, Kasper, D, Kane, S R, Jenkins, J M, Huber, D, Horne, K, Hill, M L, Gorrini, P, Giacalone, S, Fulton, B, Forveille, T, Figueira, P, Fetherolf, T, Dressing, C, Díaz, R F, Delfosse, X, Dalba, P A, Dai, F, Cortés, C C, Crossfield, I J M, Crane, J D, Conti, D M, Collins, K I, Chontos, A, Butler, R P, Brown, P, Brady, M, Behmard, A, Beard, C, Batalha, N M & Almenara, J M 2022, ' A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds ', Astronomical Journal, vol. 163, no. 4, 168 . https://doi.org/10.3847/1538-3881/ac50a9
Winters, J G, Cloutier, R, Medina, A A, Irwin, J M, Charbonneau, D, Astudillo-Defru, N, Bonfils, X, Howard, A W, Isaacson, H, Bean, J L, Seifahrt, A, Teske, J K, Eastman, J D, Twicken, J D, Collins, K A, Jensen, E L N, Quinn, S N, Payne, M J, Kristiansen, M H, Spencer, A, Vanderburg, A, Zechmeister, M, Weiss, L M, Wang, S X, Wang, G, Udry, S, Terentev, I A, Stuermer, J, Stefansson, G, Shporer, A, Shectman, S, Sefako, R, Schwengeler, H M, Schwarz, R P, Scarsdale, N, Rubenzahl, R A, Roy, A, Rosenthal, L J, Robertson, P, Petigura, E A, Pepe, F, Omohundro, M, Murphy, J M A, Murgas, F, Mocnik, T, Montet, B T, Mennickent, R, Mayo, A W, Massey, B, Lubin, J, Lovis, C, Lewin, P, Kasper, D, Kane, S R, Jenkins, J M, Huber, D, Horne, K, Hill, M L, Gorrini, P, Giacalone, S, Fulton, B, Forveille, T, Figueira, P, Fetherolf, T, Dressing, C, Diaz, R F, Delfosse, X, Dalba, P A, Dai, F, Cortes, C C, Crossfield, I J M, Crane, J D, Conti, D M, Collins, K, Chontos, A, Butler, R P, Brown, P, Brady, M, Behmard, A, Beard, C, Batalha, N M & Almenara, J-M 2022, ' A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds ', Astronomical Journal, vol. 163, no. 4, 168 . https://doi.org/10.3847/1538-3881/ac50a9
Winters, J G, Cloutier, R, Medina, A A, Irwin, J M, Charbonneau, D, Astudillo-Defru, N, Bonfils, X, Howard, A W, Isaacson, H, Bean, J L, Seifahrt, A, Teske, J K, Eastman, J D, Twicken, J D, Collins, K A, Jensen, E L N, Quinn, S N, Payne, M J, Kristiansen, M H, Spencer, A, Vanderburg, A, Zechmeister, M, Weiss, L M, Wang, S X, Wang, G, Udry, S, Terentev, I A, Stuermer, J, Stefansson, G, Shporer, A, Shectman, S, Sefako, R, Schwengeler, H M, Schwarz, R P, Scarsdale, N, Rubenzahl, R A, Roy, A, Rosenthal, L J, Robertson, P, Petigura, E A, Pepe, F, Omohundro, M, Murphy, J M A, Murgas, F, Mocnik, T, Montet, B T, Mennickent, R, Mayo, A W, Massey, B, Lubin, J, Lovis, C, Lewin, P, Kasper, D, Kane, S R, Jenkins, J M, Huber, D, Horne, K, Hill, M L, Gorrini, P, Giacalone, S, Fulton, B, Forveille, T, Figueira, P, Fetherolf, T, Dressing, C, Diaz, R F, Delfosse, X, Dalba, P A, Dai, F, Cortes, C C, Crossfield, I J M, Crane, J D, Conti, D M, Collins, K, Chontos, A, Butler, R P, Brown, P, Brady, M, Behmard, A, Beard, C, Batalha, N M & Almenara, J-M 2022, ' A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds ', Astronomical Journal, vol. 163, no. 4, 168 . https://doi.org/10.3847/1538-3881/ac50a9
LTT 1445 is a hierarchical triple M-dwarf star system located at a distance of 6.86 parsecs. The primary star LTT 1445A (0.257 M_Sun) is known to host the transiting planet LTT 1445Ab with an orbital period of 5.4 days, making it the second closest k
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a670cd3935b41769154fe8c069a0d229
https://resolver.caltech.edu/CaltechAUTHORS:20211018-185047173
https://resolver.caltech.edu/CaltechAUTHORS:20211018-185047173
Autor:
Erik A. Petigura, James G. Rogers, Howard Isaacson, James E. Owen, Adam L. Kraus, Joshua N. Winn, Mason G. MacDougall, Andrew W. Howard, Benjamin Fulton, Molly R. Kosiarek, Lauren M. Weiss, Aida Behmard, Sarah Blunt
In 2017, the California-Kepler Survey (CKS) published its first data release (DR1) of high-resolution optical spectra of 1305 planet hosts. Refined CKS planet radii revealed that small planets are bifurcated into two distinct populations: super-Earth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26d026e4f1a3e4f2ff3b632b320b901a
https://resolver.caltech.edu/CaltechAUTHORS:20220228-183210630
https://resolver.caltech.edu/CaltechAUTHORS:20220228-183210630
Autor:
Lynne A. Hillenbrand, Howard Isaacson, Antonio C. Rodriguez, Michael Connelley, Bo Reipurth, Michael A. Kuhn, Tracy Beck, Diego Rodriguez Perez
Magakian et al. called attention to the current bright state of LkHα 225 South, a well-known highly embedded, intermediate-mass young stellar object that over the past two decades has brightened visually from >20 m to m . We present recent optical p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ada8c7accb33668a0b95423cbeda8680
https://resolver.caltech.edu/CaltechAUTHORS:20211214-190100059
https://resolver.caltech.edu/CaltechAUTHORS:20211214-190100059
Autor:
Xian-Yu Wang, Malena Rice, Songhu Wang, Bonan Pu, Gudmundur Stefánsson, Suvrath Mahadevan, Brandon Radzom, Steven Giacalone, Zhen-Yu Wu, Thomas M. Esposito, Paul A. Dalba, Arin Avsar, Bradford Holden, Brian Skiff, Tom Polakis, Kevin Voeller, Sarah E. Logsdon, Jessica Klusmeyer, Heidi Schweiker, Dong-Hong Wu, Corey Beard, Fei Dai, Jack Lubin, Lauren M. Weiss, Chad F. Bender, Cullen H. Blake, Courtney D. Dressing, Samuel Halverson, Fred Hearty, Andrew W. Howard, Daniel Huber, Howard Isaacson, James A. G. Jackman, Joe Llama, Michael W. McElwain, Jayadev Rajagopal, Arpita Roy, Paul Robertson, Christian Schwab, Evgenya L. Shkolnik, Jason T. Wright, Gregory Laughlin
We present spectroscopic measurements of the Rossiter-McLaughlin effect for WASP-148b, the only known hot Jupiter with a nearby warm-Jupiter companion, from the WIYN/NEID and Keck/HIRES instruments. This is one of the first scientific results reporte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1258d436f67930045331047bdcaa8a19
https://resolver.caltech.edu/CaltechAUTHORS:20211130-215726378
https://resolver.caltech.edu/CaltechAUTHORS:20211130-215726378
Autor:
Jack Lubin, Judah Van Zandt, Rae Holcomb, Lauren M. Weiss, Erik A Petigura, Paul Robertson, Joseph M. Akana Murphy, Nicholas Scarsdale, Konstantin Batygin, Alex S. Polanski, Natalie M. Batalha, Ian J. M. Crossfield, Courtney Dressing, Benjamin Fulton, Andrew W. Howard, Daniel Huber, Howard Isaacson, Stephen R. Kane, Arpita Roy, Corey Beard, Sarah Blunt, Ashley Chontos, Fei Dai, Paul A. Dalba, Kaz Gary, Steven Giacalone, Michelle L. Hill, Andrew Mayo, Teo Močnik, Molly R. Kosiarek, Malena Rice, Ryan A. Rubenzahl, David W. Latham, S. Seager, Joshua N. Winn
Exoplanet systems with multiple transiting planets are natural laboratories for testing planetary astrophysics. One such system is HD 191939 (TOI-1339), a bright (V=9) and Sun-like (G9V) star, which TESS found to host three transiting planets (b, c,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc6e0bee9b81790c21f626d4cc4a542e
https://resolver.caltech.edu/CaltechAUTHORS:20211018-185245786
https://resolver.caltech.edu/CaltechAUTHORS:20211018-185245786