Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Matthew L. Stevans"'
Autor:
Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher, Elisabete da Cunha, Viviana Acquaviva, Denis Burgarella, Gabriela Calistro Rivera, Adam C. Carnall, Yu-Yen Chang, Nima Chartab, Kevin C. Cooke, Ciaran Fairhurst, Jeyhan Kartaltepe, Joel Leja, Katarzyna Małek, Brett Salmon, Marianna Torelli, Alba Vidal-García, Médéric Boquien, Gabriel G. Brammer, Michael J. I. Brown, Peter L. Capak, Jacopo Chevallard, Chiara Circosta, Darren Croton, Iary Davidzon, Mark Dickinson, Kenneth J. Duncan, Sandra M. Faber, Harry C. Ferguson, Adriano Fontana, Yicheng Guo, Boris Haeussler, Shoubaneh Hemmati, Marziye Jafariyazani, Susan A. Kassin, Rebecca L. Larson, Bomee Lee, Kameswara Bharadwaj Mantha, Francesca Marchi, Hooshang Nayyeri, Jeffrey A. Newman, Viraj Pandya, Janine Pforr, Naveen Reddy, Ryan Sanders, Ekta Shah, Abtin Shahidi, Matthew L. Stevans, Dian Puspita Triani, Krystal D. Tyler, Brittany N. Vanderhoof, Alexander de la Vega, Weichen Wang, Madalyn E. Weston
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 2, p 141 (2023)
The study of galaxy evolution hinges on our ability to interpret multiwavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy distribution (SED) models, which allow us to infer physical parameters
Externí odkaz:
https://doaj.org/article/e3f8aeb7ca42439d83db6ac21b54304c
Autor:
Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher, Elisabete da Cunha, Viviana Acquaviva, Denis Burgarella, Gabriela Calistro Rivera, Adam C. Carnall, Yu-Yen Chang, Nima Chartab, Kevin C. Cooke, Ciaran Fairhurst, Jeyhan Kartaltepe, Joel Leja, Katarzyna Małek, Brett Salmon, Marianna Torelli, Alba Vidal-García, Médéric Boquien, Gabriel G. Brammer, Michael J. I. Brown, Peter L. Capak, Jacopo Chevallard, Chiara Circosta, Darren Croton, Iary Davidzon, Mark Dickinson, Kenneth J. Duncan, Sandra M. Faber, Harry C. Ferguson, Adriano Fontana, Yicheng Guo, Boris Haeussler, Shoubaneh Hemmati, Marziye Jafariyazani, Susan A. Kassin, Rebecca L. Larson, Bomee Lee, Kameswara Bharadwaj Mantha, Francesca Marchi, Hooshang Nayyeri, Jeffrey A. Newman, Viraj Pandya, Janine Pforr, Naveen Reddy, Ryan Sanders, Ekta Shah, Abtin Shahidi, Matthew L. Stevans, Dian Puspita Triani, Krystal D. Tyler, Brittany N. Vanderhoof, Alexander de la Vega, Weichen Wang, Madalyn E. Weston
Publikováno v:
Pacifici, C, Iyer, K G, Mobasher, B, da Cunha, E, Acquaviva, V, Burgarella, D, Rivera, G C, Carnall, A C, Chang, Y-Y, Chartab, N, Cooke, K C, Fairhurst, C, Kartaltepe, J, Leja, J, Malek, K, Salmon, B, Torelli, M, Vidal-Garcia, A, Boquien, M, Brammer, G G, Brown, M J I, Capak, P L, Chevallard, J, Circosta, C, Croton, D, Davidzon, I, Dickinson, M, Duncan, K J, Faber, S M, Ferguson, H C, Fontana, A, Guo, Y, Haeussler, B, Hemmati, S, Jafariyazani, M, Kassin, S A, Larson, R L, Lee, B, Mantha, K B, Marchi, F, Nayyeri, H, Newman, J A, Pandya, V, Pforr, J, Reddy, N, Sanders, R, Shah, E, Shahidi, A, Stevans, M L, Triani, D P, Tyler, K D, Vanderhoof, B N, de la Vega, A, Wang, W & Weston, M E 2023, ' The Art of Measuring Physical Parameters in Galaxies : A Critical Assessment of Spectral Energy Distribution Fitting Techniques ', Astrophysical Journal, vol. 944, no. 2, 141 . https://doi.org/10.3847/1538-4357/acacff
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy distribution (SED) models which allow us to infer physical parameters
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df92440c48a98ef48152b90d914453d0
http://arxiv.org/abs/2212.01915
http://arxiv.org/abs/2212.01915
Autor:
Matthew L. Stevans, Sydney Sherman, Steven L. Finkelstein, Casey Papovich, Robin Ciardullo, Jonathan Florez, Lalitwadee Kawinwanichakij, Shardha Jogee, Caryl Gronwall, Isak Wold
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 505:947-962
We present the main sequence for all galaxies and star-forming galaxies for a sample of 28,469 massive ($M_\star \ge 10^{11}$M$_\odot$) galaxies at cosmic noon ($1.5 < z < 3.0$), uniformly selected from a 17.5 deg$^2$ area (0.33 Gpc$^3$ comoving volu
Autor:
Steven L. Finkelstein, Robin Ciardullo, Isak Wold, Allison Kirkpatrick, Shardha Jogee, Sydney Sherman, Casey Papovich, Caryl Gronwall, Lalitwadee Kawinwanichakij, Jonathan Florez, C. Megan Urry, Stephanie M. LaMassa, Matthew L. Stevans, Tonima Tasnim Ananna
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 497:3273-3296
We investigate the relation between AGN and star formation (SF) activity at $0.5 < z < 3$ by analyzing 898 galaxies with X-ray luminous AGN ($L_X > 10^{44}$ erg s$^{-1}$) and a large comparison sample of $\sim 320,000$ galaxies without X-ray luminous
Autor:
Caryl Gronwall, Lalitwadee Kawinwanichakij, Robin Ciardullo, Shardha Jogee, Viviana Acquaviva, Casey Papovich, Steven L. Finkelstein, Sydney Sherman, Zacharias E. Escalante, Matthew L. Stevans, Jonathan Florez, Isak Wold
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 491:3318-3335
We present the high-mass end of the galaxy stellar mass function using the largest sample to date (5,352) of star-forming galaxies with $M_{\star} > 10^{11} M_{\odot}$ at cosmic noon, $1.5 < z < 3.5$. This sample is uniformly selected across 17.2 deg
Autor:
Lalitwadee Kawinwanichakij, Gene C. K. Leung, Rainer Weinberger, Yuchen Guo, Sofía A. Cora, Robin Ciardullo, Casey Papovich, Steven L. Finkelstein, Mark Vogelsberger, Lars Hernquist, Isak Wold, Matthew L. Stevans, Stephanie M. LaMassa, Romeel Davé, Shardha Jogee, Jonathan Florez, Caryl Gronwall
Publikováno v:
Florez, J, Jogee, S, Guo, Y, Cora, S A, Weinberger, R, Davé, R, Hernquist, L, Vogelsberger, M, Ciardullo, R, Finkelstein, S L, Gronwall, C, Kawinwanichakij, L, Leung, G C K, LaMassa, S, Papovich, C, Stevans, M L & Wold, I 2021, ' AGN and star formation at cosmic noon: comparison of data to theoretical models ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 1, pp. 762-780 . https://doi.org/10.1093/mnras/stab2593
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In theoretical models of galaxy evolution, AGN and star formation (SF) activity are closely linked and AGN feedback is routinely invoked to regulate galaxy growth. In order to constrain such models, we compare the hydrodynamical simulations Illustris
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2bcdae166312e23f23b62de423367f2
Autor:
Sofía A. Cora, Isak Wold, Caryl Gronwall, Sydney Sherman, Robin Ciardullo, Casey Papovich, Jonathan Florez, Tomás Hough, Cristian A. Vega-Martínez, Matthew L. Stevans, Steven L. Finkelstein, Lalitwadee Kawinwanichakij, Shardha Jogee
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We explore the buildup of quiescent galaxies using a sample of 28,469 massive (𝑀★ ≥ 1011M ) galaxies at redshifts 1.5 < 𝑧 < 3.0, drawn from a 17.5 deg2 area (0.33 Gpc3 comoving volume at these redshifts). This allows for a robust study of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47526e42eaae6dc1165cf5c5d176050a
https://academic.oup.com/mnras/article/499/3/4239/5924472
https://academic.oup.com/mnras/article/499/3/4239/5924472
Autor:
Steven L. Finkelstein, Isak Wold, A. Coughlin, Johnnes Zabl, R. A. Swaters, Vithal Tilvi, Bhavin Joshi, John Pharo, Huan Yang, Tianxing Jiang, Sylvain Veilleux, Ali Ahmad Khostovan, Zhen-Ya Zheng, James E. Rhoads, Pascale Hibon, Lucia A. Perez, Sangeeta Malhotra, Matthew L. Stevans, Bahram Mobasher, Junxian Wang, R. Probst, Santosh Harish
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2020, 892, ⟨10.3847/1538-4357/ab7015⟩
The Astrophysical Journal, 2020, 892, ⟨10.3847/1538-4357/ab7015⟩
We present new estimates of the luminosity function (LF) and star formation rate density (SFRD) for an H$\alpha$ selected sample at $z\sim0.62$ from the Deep And Wide Narrow-band (DAWN) survey. Our results are based on a new H$\alpha$ sample in the e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92ee31746cc1ddf01bcc2de34d72bf42
https://hal-insu.archives-ouvertes.fr/insu-03711477
https://hal-insu.archives-ouvertes.fr/insu-03711477
Autor:
Keely D. Finkelstein, Sofía Rojas-Ruiz, M. Mechtley, Micaela Bagley, Steven L. Finkelstein, Rebecca L. Larson, Matthew L. Stevans, James Diekmann
Looking for bright galaxies born in the early universe is fundamental to investigating the Epoch of Reionization, the era when the first stars and galaxies ionized the intergalactic medium. We utilize Hubble Space Telescope pure parallel imaging to s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9dc5460a883f4fec12d1eefcda8832d0
Autor:
L. Y. Aaron Yung, Romeel Davé, Robin Ciardullo, Isak Wold, Jonathan Florez, Lalitwadee Kawinwanichakij, Matthew L. Stevans, Rachel S. Somerville, Sydney Sherman, Steven L. Finkelstein, Casey Papovich, Caryl Gronwall, Shardha Jogee
Publikováno v:
The Astrophysical Journal. 921:58
We present the results of a deep K_s-band (2.1 um) imaging survey of the Spitzer/HETDEX Exploratory Large Area (SHELA) field using the NEWFIRM near-infrared (NIR) camera on the KPNO Mayall 4-m telescope. This NEWFIRM HETDEX Survey (NHS) reaches a 5-s