Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Rawle, Timothy D."'
Autor:
Bechtold, Katie, Böker, Torsten, Franz, David E., Plate, Maurice te, Rawle, Timothy D., Wu, Rai, Zeidler, Peter
The Near Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope affords the astronomical community an unprecedented space-based Multi-Object Spectroscopy (MOS) capability through the use of a programmable array of micro-electro-mechanical
Externí odkaz:
http://arxiv.org/abs/2408.15940
Autor:
Birkmann, Stephan M., Giardino, Giovanna, Sirianni, Marco, Ferruit, Pierre, Rauscher, Bernhard, de Oliveira, Catarina Alves, Böker, Torsten, Kumari, Nimisha, Lützgendorf, Nora, Manjavacas, Elena, Proffitt, Charles, Rawle, Timothy D., Plate, Maurice te, Zeidler, Peter
The Near-Infrared Spectrograph (NIRSpec) is one the four focal plane instruments on the James Webb Space Telescope (JWST) which was launched on December 25, 2021. We present the in-flight status and performance of NIRSpec's detector system as derived
Externí odkaz:
http://arxiv.org/abs/2208.12686
Autor:
Rawle, Timothy D., Giardino, Giovanna, Franz, David E., Rapp, Robert, Plate, Maurice te, Zincke, Christian A., Abul-Huda, Yasin M., de Oliveira, Catarina Alves, Bechtold, Katie, Beck, Tracy, Birkmann, Stephan M., Böker, Torsten, Ehrenwinkler, Ralf, Ferruit, Pierre, Garland, Dennis, Jakobsen, Peter, Karakla, Diane, Karl, Hermann, Keyes, Charles D., Koehler, Robert, Kumari, Nimisha, Lützgendorf, Nora, Manjavacas, Elena, Marston, Anthony, Moseley, S. Harvey, Mosner, Peter, Muzerolle, James, Ogle, Patrick, Proffitt, Charles, Sabbi, Elena, Sirianni, Marco, Wahlgren, Glenn, Wislowski, Emily, Wright, Raymond H., Wu, Chi Rai, Zeidler, Peter
The NIRSpec instrument on the James Webb Space Telescope (JWST) brings the first multi-object spectrograph (MOS) into space, enabled by a programmable Micro Shutter Array (MSA) of ~250,000 individual apertures. During the 6-month Commissioning period
Externí odkaz:
http://arxiv.org/abs/2208.04673
Autor:
Sun, Fengwu, Egami, Eiichi, Pérez-González, Pablo G., Smail, Ian, Caputi, Karina I., Bauer, Franz E., Rawle, Timothy D., Fujimoto, Seiji, Kohno, Kotaro, Dudzevičiūtė, Ugnė, Atek, Hakim, Bianconi, Matteo, Chapman, Scott C., Combes, Francoise, Jauzac, Mathilde, Jolly, Jean-Baptiste, Koekemoer, Anton M., Magdis, Georgios E., Rodighiero, Giulia, Rujopakarn, Wiphu, Schaerer, Daniel, Steinhardt, Charles L., Van der Werf, Paul, Walth, Gregory L., Weaver, John R.
We present a Spitzer/IRAC survey of H-faint ($H_{160} \gtrsim 26.4$, $<5\sigma$) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of $\sim$648 arcmin$^2$ (effectively $\sim$221 arcmin$^2$ in the source plane), we have sec
Externí odkaz:
http://arxiv.org/abs/2109.01751
Autor:
Sun, Fengwu, Egami, Eiichi, Rawle, Timothy D., Walth, Gregory L., Smail, Ian, Dessauges-Zavadsky, Miroslava, Perez-Gonzalez, Pablo G., Richard, Johan, Combes, Francoise, Ebeling, H., Pello, Roser, van der Werf, Paul P., Altieri, B., Boone, Frederic, Cava, Antonio, Chapman, Scott C., Clement, Benjamin, Finoguenov, Alexis, Nakajima, Kimihiko, Rujopakarn, Wiphu, Schaerer, Daniel, Valtchanov, Ivan
We present an ALMA 1.3 mm (Band 6) continuum survey of lensed submillimeter galaxies (SMGs) at $z=1.0\sim3.2$ with an angular resolution of $\sim0.2$". These galaxies were uncovered by the Herschel Lensing Survey (HLS), and feature exceptionally brig
Externí odkaz:
http://arxiv.org/abs/2101.03677
Autor:
Walth, Gregory L., Egami, Eiichi, Clément, Benjamin, Rawle, Timothy D., Rex, Marie, Richard, Johan, Pérez-González, Pablo, Boone, Frédéric, Dessauges-Zavadsky, Miroslava, Portouw, Jeff, Weiner, Benjamin, McGreer, Ian, Schneider, Evan
Using the Spitzer Space Telescope and Herschel Space Observatory, we have conducted a survey of infrared galaxies in the field of the galaxy cluster Abell S1063 (AS1063) at $z=0.347$, which is one of the most massive clusters known and a target of th
Externí odkaz:
http://arxiv.org/abs/1904.07256
Autor:
Williams, Christina C., Curtis-Lake, Emma, Hainline, Kevin N., Chevallard, Jacopo, Robertson, Brant E., Charlot, Stephane, Endsley, Ryan, Stark, Daniel P., Willmer, Christopher N. A., Alberts, Stacey, Amorin, Ricardo, Arribas, Santiago, Baum, Stefi, Bunker, Andrew, Carniani, Stefano, Crandall, Sara, Egami, Eiichi, Eisenstein, Daniel J., Ferruit, Pierre, Husemann, Bernd, Maseda, Michael V., Maiolino, Roberto, Rawle, Timothy D., Rieke, Marcia, Smit, Renske, Tacchella, Sandro, Willott, Chris J.
We present an original phenomenological model to describe the evolution of galaxy number counts, morphologies, and spectral energy distributions across a wide range of redshifts (0.26]. Our model follows obser
Externí odkaz:
http://arxiv.org/abs/1802.05272
Autor:
Chevallard, Jacopo, Curtis-Lake, Emma, Charlot, Stephane, Ferruit, Pierre, Giardino, Giovanna, Franx, Marijn, Maseda, Michael V., Amorin, Ricardo, Arribas, Santiago, Bunker, Andy, Carniani, Stefano, Husemann, Bernd, Jakobsen, Peter, Maiolino, Roberto, Pforr, Janine, Rawle, Timothy D., Rix, Hans-Walter, Smit, Renske, Willott, Chris J.
The James Webb Space Telescope (JWST) will enable the detection of optical emission lines in galaxies spanning a broad range of luminosities out to redshifts z>10. Measurements of key galaxy properties, such as star formation rate and metallicity, th
Externí odkaz:
http://arxiv.org/abs/1711.07481
Autor:
Dwek, Eli, Staguhn, Johannes, Arendt, Richard G., Kovács, Attila, Decarli, Roberto, Egami, Eiichi, Michałowski, Michał J., Rawle, Timothy D., Toft, Sune, Walter, Fabian
Two millimeter observations of the MACS J1149.6+2223 cluster have detected a source that was consistent with the location of the lensed MACS1149-JD galaxy at z=9.6. A positive identification would have rendered this galaxy as the youngest dust formin
Externí odkaz:
http://arxiv.org/abs/1509.09204
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.