Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Lothringer, Josh"'
Autor:
Alam, Munazza K., Rickman, Emily, Hoch, Kielan, Mollière, Paul, Lothringer, Josh, Carter, Aarynn L., Rebollido, Isabel, Sutlieff, Ben J., Kammerer, Jens
We propose a comprehensive survey of giant planets ranging from close-in highly irradiated hot Jupiters to young, wide-orbit directly imaged planets. The combination of two established techniques for probing planetary atmospheric compositions (time-s
Externí odkaz:
http://arxiv.org/abs/2409.00190
Autor:
Crossfield, Ian, Flores, Becky, Lothringer, Josh, Mills, Elisabeth, Valverde, Jessica, Freedman, Richard, Coria, David
GeoSnap is a new HgCdTe detector currently showing QE ~50% across 3-13?m. The device takes advantage of a ROIC currently operated at 85Hz full-frame readout across a 2048x1024 array, with larger sizes easily possible. This talk presents characterizat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::043d062c8a08bfa32849640671141ea1
Autor:
Lothringer, Joshua D., Benneke, Björn, Crossfield, Ian J. M., Henry, Gregory W., Morley, Caroline, Dragomir, Diana, Barman, Travis, Knutson, Heather, Kempton, Eliza, Fortney, Jonathan, McCullough, Peter, Howard, Andrew W.
GJ 436b is a prime target for understanding warm Neptune exoplanet atmospheres and a target for multiple James Webb Space Telescope (JWST) Guaranteed Time Observation programs. Here, we report the first space-based optical transmission spectrum of th
Externí odkaz:
http://hdl.handle.net/10150/626526
http://arizona.openrepository.com/arizona/handle/10150/626526
http://arizona.openrepository.com/arizona/handle/10150/626526
Autor:
Bell, Taylor J., Nikolov, Nikolay, Cowan, Nicolas B., Barstow, Joanna K., Barman, Travis S., Crossfield, Ian J. M., Gibson, Neale P., Evans, Thomas M., Sing, David K., Knutson, Heather A., Kataria, Tiffany, Lothringer, Joshua D., Benneke, Björn, Schwartz, Joel C.
We present an optical eclipse observation of the hot Jupiter WASP-12b using the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. These spectra allow us to place an upper limit of A(g) < 0.064 (97.5% confidence level) on the p
Externí odkaz:
http://hdl.handle.net/10150/625800
http://arizona.openrepository.com/arizona/handle/10150/625800
http://arizona.openrepository.com/arizona/handle/10150/625800
Autor:
Crossfield, Ian J. M., Ciardi, David R., Petigura, Erik A., Sinukoff, Evan, Schlieder, Joshua E., Howard, Andrew W., Beichman, Charles A., Isaacson, Howard, Dressing, Courtney D., Christiansen, Jessie L., Fulton, Benjamin J., Lepine, Sebastien, Weiss, Lauren, Hirsch, Lea, Livingston, John, Baranec, Christoph, Law, Nicholas M., Riddle, Reed, Ziegler, Carl, Howell, Steve B., Horch, Elliott, Everett, Mark, Teske, Johanna, Martinez, Arturo O., Obermeier, Christian, Benneke, Bjorn, Scott, Nic, Deacon, Niall, Aller, Kimberly M., Hansen, Brad M. S., Mancini, Luigi, Ciceri, Simona, Brahm, Rafael, Jordan, Andres, Knutson, Heather A., Henning, Thomas, Bonnefoy, Michael, Liu, Michael C., Crepp, Justin R., Lothringer, Joshua, Hinz, Phil, Bailey, Vanessa, Skemer, Andrew, Defrere, Denis
We present 197 planet candidates discovered using data from the first year of the NASA K2 mission (Campaigns 0-4), along with the results of an intensive program of photometric analyses, stellar spectroscopy, high-resolution imaging, and statistical
Externí odkaz:
http://hdl.handle.net/10150/624074
http://arizona.openrepository.com/arizona/handle/10150/624074
http://arizona.openrepository.com/arizona/handle/10150/624074