Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Matt Matuszewski"'
Autor:
Marc . Kassis, Steve Allen, Carlos Alvarez, Ravinder Banyal, Robert Bertz, Charles Beichman, Aaron Brown, Matthew Brown, Gerald Cabak, Kevin Bundy, Sylvain Cetre, Jason Chin, Mark Chun, Will Deich, Richard Dekany, Jacques-Robert Delorme, Mark Devenot, Greg Doppmann, Michael P. Fitzgerald, Jason R. Fucik, Grant Hill, Philip . Hinz, Bradford P. Holden, Andrew W. Howard, Maodong Gao, Steve Gibson, Percy Gomez, Colby Gottschalk, Peter R. Gillingham, Tucker Jones, Nemanja Jovanovic, Evan Kirby, Quinn Konopacky, Shanti Krishnan, Renate Kupke, James E. Larkin, Stephanie D. Leifer, Hilton A. Lewis, Scott Lilley, Jessica Lu, James E. Lyke, Nicholas MacDonald, Eduardo Marin, Matt Matuszewski, Dimitri Mawet, Rosalie McGurk, Maxwell A. Millar-Blanchaer, Reston . Nash, Craig Nance, James D. Neill, John M. O'Meara, Eliad Peretz, Claire . Poppett, John C. Mather, Matthew V. Radovan, Mitsuko K. Roberts, Sam Ragland, Kodi Rider, Constance . Rockosi, Dale Sandfor, Boqiang Shen, Charles C. Steidel, Sunil Simha, Andy Skemer, Richard Stelter, Avinash Surendran, James Thorne, Ben McCarney, Kyle Lanclos, Ashley Baker, Ryan Rubenzahl, Arpita Roy, Sam Halverson, Jerry Edelstein, Christopher Martin, Maureen Savage, Dale Sandford, Stephanie Sallum, Josh Walawender, Peter Wizinowich, Kyle B. Westfall, Kerry J. Vahala, Shelley A. Wright, Truman Wold, Sherry Yeh
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy IX.
Autor:
Kristi A Webb, Alexa Villaume, Seppo Laine, Aaron J Romanowsky, Michael Balogh, Pieter van Dokkum, Duncan A Forbes, Jean Brodie, Christopher Martin, Matt Matuszewski
We study the star formation history (SFH) of the ultra-diffuse galaxy (UDG) Dragonfly 44 (DF44) based on the simultaneous fit to near-ultraviolet to near-infrared photometry and high signal-to-noise optical spectroscopy. In fitting the observations w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e029bc8faf4f29ab53a3e1f99a41adc6
http://arxiv.org/abs/2208.11038
http://arxiv.org/abs/2208.11038
Autor:
Alexa Villaume, Aaron J. Romanowsky, Jean Brodie, Pieter van Dokkum, Charlie Conroy, Duncan A. Forbes, Shany Danieli, Christopher Martin, Matt Matuszewski
We use the Keck Cosmic Web Imager integral field unit spectrograph to (1) measure the global stellar population parameters for the ultra-diffuse galaxy (UDG) Dragonfly 44 (DF44) to much higher precision than previously possible for any UDG and (2) fo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c439dc9dfdaa902377a34735917ccf5f
https://resolver.caltech.edu/CaltechAUTHORS:20220114-265463000
https://resolver.caltech.edu/CaltechAUTHORS:20220114-265463000
Autor:
Joshua D. Simon, Andrew B. Newman, Patrick Morrissey, Nicole C. Relatores, Alberto D. Bolatto, Leo Blitz, Matt Matuszewski, Christopher Martin, Richard S. Ellis, Phuongmai Truong, James D. Neill
Dark matter-only simulations predict that dark matter halos have steep, cuspy inner density profiles, while observations of dwarf galaxies find a range of inner slopes that are often much shallower. There is debate whether this discrepancy can be exp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::271e98579b41e1e25c5663fa41c844bf
http://arxiv.org/abs/1911.05836
http://arxiv.org/abs/1911.05836
Autor:
Alexa Villaume, John Tamanas, Pieter van Dokkum, Shany Danieli, Jean P. Brodie, Asher Wasserman, Aaron J. Romanowsky, Roberto Abraham, Christopher Martin, Stefano Profumo, Duncan A. Forbes, Matt Matuszewski
Publikováno v:
Astrophysical Journal, vol 885, iss 2
Wasserman, Asher; Dokkum, Pieter van; Romanowsky, Aaron J; Brodie, Jean; Danieli, Shany; Forbes, Duncan A; et al.(2019). Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/5982p41g
The Astrophysical Journal, vol 885, iss 2
Wasserman, Asher; Dokkum, Pieter van; Romanowsky, Aaron J; Brodie, Jean; Danieli, Shany; Forbes, Duncan A; et al.(2019). Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/5982p41g
The Astrophysical Journal, vol 885, iss 2
Given the absence of directly detected dark matter (DM) as weakly interacting massive particles, there is strong interest in the possibility that DM is an ultra-light scalar field, here denoted as fuzzy DM. Ultra-diffuse galaxies, with the sizes of g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1560badabd15b2ba5aefc1e431526c14
https://escholarship.org/uc/item/5982p41g
https://escholarship.org/uc/item/5982p41g
Autor:
Aaron J. Romanowsky, Asher Wasserman, Jean P. Brodie, Matt Matuszewski, Charlie Conroy, Christopher Martin, Roberto Abraham, Shany Danieli, Alexa Villaume, Duncan A. Forbes, Pieter van Dokkum
We present spatially-resolved stellar kinematics of the well-studied ultra diffuse galaxy (UDG) Dragonfly 44, as determined from 25.3 hrs of observations with the Keck Cosmic Web Imager. The luminosity-weighted dispersion within the half-light radius
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2a733cbae9e1df85b232f1be557ae96
Autor:
Ofer Yaron, S. Bradley Cenko, Ragnhild Lunnan, D. Sullivan, Mansi M. Kasliwal, Yi Cao, Kaushik De, Eran O. Ofek, Yvette C. Perrott, Joel Johansson, Matt Matuszewski, Albert K. H. Kong, Umaa Rebbapragada, Shrinivas R. Kulkarni, Adam Rubin, T. M. Cantwell, Kunal Mooley, Peter Nugent, Avishay Gal-Yam, Frank J. Masci, James D. Neill
Publikováno v:
De, K; Kasliwal, MM; Cantwell, T; Cao, Y; Cenko, SB; Gal-Yam, A; et al.(2018). IPTF 16hgs: A Double-peaked Ca-rich Gap Transient in a Metal-poor, Star-forming Dwarf Galaxy. Astrophysical Journal, 866(1). doi: 10.3847/1538-4357/aadf8e. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/7402j53d
De, K, Kasliwal, M M, Cantwell, T, Cao, Y, Cenko, S B, Gal-yam, A, Johansson, J, Kong, A, Kulkarni, S R, Lunnan, R, Masci, F, Matuszewski, M, Mooley, K P, Neill, J D, Nugent, P E, Ofek, E O, Perrott, Y, Rebbapragada, U D, Rubin, A, Sullivan, D O & Yaron, O 2018, ' iPTF 16hgs: A Double-peaked Ca-rich Gap Transient in a Metal-poor, Star-forming Dwarf Galaxy ', The Astrophysical Journal, vol. 866, no. 1, pp. 72 . https://doi.org/10.3847/1538-4357/aadf8e
Astrophysical Journal, vol 866, iss 1
The Astrophysical Journal, vol 866, iss 1
De, K, Kasliwal, M M, Cantwell, T, Cao, Y, Cenko, S B, Gal-yam, A, Johansson, J, Kong, A, Kulkarni, S R, Lunnan, R, Masci, F, Matuszewski, M, Mooley, K P, Neill, J D, Nugent, P E, Ofek, E O, Perrott, Y, Rebbapragada, U D, Rubin, A, Sullivan, D O & Yaron, O 2018, ' iPTF 16hgs: A Double-peaked Ca-rich Gap Transient in a Metal-poor, Star-forming Dwarf Galaxy ', The Astrophysical Journal, vol. 866, no. 1, pp. 72 . https://doi.org/10.3847/1538-4357/aadf8e
Astrophysical Journal, vol 866, iss 1
The Astrophysical Journal, vol 866, iss 1
Calcium rich gap transients represent an intriguing new class of faint and fast evolving supernovae that exhibit strong [Ca II] emission in their nebular phase spectra. In this paper, we present the discovery and follow-up observations of iPTF 16hgs
Autor:
James D. Neill, Sebastiano Cantalupo, Anna M. Moore, Ran Wang, Matt Matuszewski, Erika T. Hamden, Christopher Martin, Qiong Li, Patrick Morrissey, J. Xavier Prochaska, Zheng Cai, Fabrizio Arrigoni Battaia, Donal O'Sullivan
Publikováno v:
The Astrophysical Journal Letters, 861 (1)
Enormous Lyα nebulae (ELANe) represent the extrema of Lyα nebulosities. They have detected extents of >200 kpc in Lyα and Lyα luminosities >10^(44) erg s^(−1). The ELAN population is an ideal laboratory to study the interactions between galaxie
Autor:
S. Rahman, Daphne Chang, Charles C. Steidel, Matt Matuszewski, D. Christopher Martin, Anna M. Moore, Patrick Morrissey
The Palomar Cosmic Web Imager (PCWI), an integral field spectrograph designed to detect and map low surface brightness emission, has obtained imaging spectroscopic maps of Ly-alpha from the circum-QSO medium (CQM) of QSO HS1549+19 at redshift of 2.84
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a15e1294d96538710a1950ffe5ecb11
https://resolver.caltech.edu/CaltechAUTHORS:20140303-152428640
https://resolver.caltech.edu/CaltechAUTHORS:20140303-152428640
Autor:
D. Christopher Martin, Jean Evrard, David Schiminovich, Robert Grange, Frederi Mirc, Robert Chave, R. McLean, Sarah Tuttle, Matt Matuszewski, Jean Michel Deharveng, Shahinur Rahman, Bruno Milliard
Publikováno v:
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray.
FIREBALL (the Faint Intergalactic Redshifted Emission Balloon) is a balloon-borne 1m telescope coupled to an ultraviolet fiber-fed spectrograph. FIREBALL is designed to study the faint and diffuse emission of the intergalactic medium, until now detec