Zobrazeno 1 - 10
of 13 688
pro vyhledávání: '"Newman, A B"'
Autor:
Hung, Denise, Lemaux, Brian C., Cucciati, Olga, Forrest, Ben, Shah, Ekta A., Gal, Roy R., Giddings, Finn, Sikorski, Derek, Golden-Marx, Emmet, Lubin, Lori M., Hathi, Nimish, Zamorani, Giovanni, Bardelli, Sandro, Cassara, Letizia P., De Lucia, Gabriella, Fontanot, Fabio, Garilli, Bianca, Guaita, Lucia, Hirschmann, Michaela Monika, Lee, Kyoung-Soo, Newman, Andrew B., Ramakrishnan, Vandana, Vergani, Daniela, Xie, Lizhi, Zucca, Elena
The Charting Cluster Construction with VUDS and ORELSE (C3VO) survey is an ongoing imaging and spectroscopic campaign aiming to map out the growth of structure up to $z\sim5$ and was born from the combination of the VIMOS Ultra Deep Survey (VUDS) and
Externí odkaz:
http://arxiv.org/abs/2410.00237
Autor:
Dhawan, S., Pierel, J. D. R., Gu, M., Newman, A. B., Larison, C., Siebert, M., Petrushevska, T., Poidevin, F., Jha, S. W., Chen, W., Ellis, Richard S., Frye, B., Hjorth, J., Koekemoer, Anton M., Pérez-Fournon, I., Rest, A., Treu, T., Windhorst, R. A., Zenati, Y.
Strong gravitational lensing magnifies the light from a background source, allowing us to study these sources in detail. Here, we study the spectra of a $z = 1.95$ lensed Type Ia supernova SN~Encore for its brightest Image A, taken 39 days apart. We
Externí odkaz:
http://arxiv.org/abs/2407.16492
Autor:
Smee, Stephen A., Hope, Stephen C., Hammond, Randolph P., Aslan, Leon, Barkhouser, Robert H., Smee, Katherine G., Bianco, Andrea, Birk, Christoph, Cosens, Maren, Gray, Aidan C., Frangiamore, Michele, Harding, Albert C., Hare, Tyson, Kelson, Daniel D., Killion, Gerrad, Konidaris II, Nicholas P., Lanz, Alicia, McCloskey, Jacob, Newman, Andrew B., Ramirez, Solange, Rudie, Gwen C., Vanella, Andrea, Williams, Jason E.
Publikováno v:
Proc. SPIE, Technologies for Vacuum and Cryogenic Instruments I, Paper No. 13100-107 (June 2024)
This paper presents the design and technical progress of a precision X-Y stage for detector dithering and flexure compensation. The stage is being developed for use in the Magellan InfraRed Multi-Object Spectrograph, MIRMOS. MIRMOS is a very large Na
Externí odkaz:
http://arxiv.org/abs/2407.14493
Autor:
Cosens, Maren, Konidaris II, Nicholas P., Rudie, Gwen C., Newman, Andrew B., Killion, Gerrad, Aslan, Leon, Barkhouser, Robert, Bianco, Andrea, Birk, Christoph, Brady, Julia, Frangiamore, Michele, Hare, Tyson, Hope, Stephen C., Kelson, Daniel D., Lanz, Alicia, Ramirez, Solange, Smee, Stephen A., Vanella, Andrea, Williams, Jason E.
Publikováno v:
Proc. SPIE, Ground-based and Airborne Instrumentation for Astronomy X, Paper No. 13096-321 (June 2024)
The Magellan InfraRed Multi-Object Spectrograph (MIRMOS) is a planned next generation multi-object and integral field spectrograph for the 6.5m Magellan telescopes at Las Campanas Observatory in Chile. MIRMOS will perform R$\sim$3700 spectroscopy ove
Externí odkaz:
http://arxiv.org/abs/2407.13747
Autor:
Beverage, Aliza G., Slob, Martje, Kriek, Mariska, Conroy, Charlie, Barro, Guillermo, Bezanson, Rachel, Brammer, Gabriel, Cheng, Chloe M., de Graaff, Anna, Schreiber, Natascha M. Förster, Franx, Marijn, Lorenz, Brian, Piña, Pavel E. Mancera, Marchesini, Danilo, Muzzin, Adam, Newman, Andrew B., Price, Sedona H., Shapley, Alice E., Stefanon, Mauro, Suess, Katherine A., van Dokkum, Pieter, Weinberg, David, Weisz, Daniel R.
We present the stellar metallicities and multi-element abundances (C, Mg, Si, Ca, Ti, Cr, and Fe) of 15 massive (log $M/M_\odot=10.2-11.2$) quiescent galaxies at z=1-3, derived from ultradeep JWST-SUSPENSE spectra. Compared to quiescent galaxies at z
Externí odkaz:
http://arxiv.org/abs/2407.02556
Autor:
Jafariyazani, Marziye, Newman, Andrew B., Mobasher, Bahram, Belli, Sirio, Ellis, Richard S., Faisst, Andreas L.
Recent stellar chemical abundance measurements of a handful of $z\sim2$ quiescent galaxies have suggested these galaxies exhibit a remarkably strong $\alpha$-enhancement compared to their local and intermediate redshift counterparts. This apparent ch
Externí odkaz:
http://arxiv.org/abs/2406.03549
Autor:
Slob, Martje, Kriek, Mariska, Beverage, Aliza G., Suess, Katherine A., Barro, Guillermo, Bezanson, Rachel, Brammer, Gabriel, Cheng, Chloe M., Conroy, Charlie, de Graaff, Anna, Schreiber, Natascha M. Förster, Franx, Marijn, Lorenz, Brian, Piña, Pavel E. Mancera, Marchesini, Danilo, Muzzin, Adam, Newman, Andrew B., Price, Sedona H., Shapley, Alice E., Stefanon, Mauro, van Dokkum, Pieter, Weisz, Daniel R.
We present an overview and first results from the Spectroscopic Ultradeep Survey Probing Extragalactic Near-infrared Stellar Emission (SUSPENSE), executed with NIRSpec on JWST. The primary goal of the SUSPENSE program is to characterize the stellar,
Externí odkaz:
http://arxiv.org/abs/2404.12432
Autor:
Pierel, J. D. R., Newman, A. B., Dhawan, S., Gu, M., Joshi, B. A., Li, T., Schuldt, S., Strolger, L. G., Suyu, S. H., Caminha, G. B., Cohen, S. H., Diego, J. M., Dsilva, J. C. J., Ertl, S., Frye, B. L., Granata, G., Grillo, C., Koekemoer, A. M., Li, J., Robotham, A., Summers, J., Treu, T., Windhorst, R. A., Zitrin, A., Agarwal, S., Agrawal, A., Arendse, N., Belli, S., Burns, C., Cañameras, R., Chakrabarti, S., Chen, W., Collett, T. E., Coulter, D. A., Ellis, R. S., Engesser, M., Foo, N., Fox, O. D., Gall, C., Garuda, N., Gezari, S., Gomez, S., Glazebrook, K., Hjorth, J., Huang, X., Jha, S. W., Kamieneski, P. S., Kelly, P., Larison, C., Moustakas, L. A., Pascale, M., Pérez-Fournon, I., Petrushevska, T., Poidevin, F., Rest, A., Shahbandeh, M., Shajib, A. J., Siebert, M., Storfer, C., Talbot, M., Wang, Q., Wevers, T., Zenati, Y.
A bright ($m_{\rm F150W,AB}$=24 mag), $z=1.95$ supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply-imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detecte
Externí odkaz:
http://arxiv.org/abs/2404.02139
Autor:
Newman, Andrew B., Qezlou, Mahdi, Chartab, Nima, Rudie, Gwen C., Blanc, Guillermo A., Bird, Simeon, Benson, Andrew J., Kelson, Daniel D., Lemaux, Brian C.
The connection between galaxies and dark matter halos is often quantified using the stellar mass-halo mass (SMHM) relation. Optical and near-infrared imaging surveys have led to a broadly consistent picture of the evolving SMHM relation based on meas
Externí odkaz:
http://arxiv.org/abs/2311.00184
Autor:
Matthews, A. M, Kelson, D. D., Newman, A. B., Camilo, F., Condon, J. J., Cotton, W. D., Dickinson, M., Jarrett, T. H., Lacy, M.
We present the initial sample of redshifts for 3,839 galaxies in the MeerKAT DEEP2 field -- the deepest $\sim$1.4\,GHz radio field yet observed. Using a spectrophotometric technique combining coarse optical spectra with broadband photometry, we obtai
Externí odkaz:
http://arxiv.org/abs/2310.17701