Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Nedkova, Kalina V"'
Autor:
Mehta, Vihang, Rafelski, Marc, Sunnquist, Ben, Teplitz, Harry I., Scarlata, Claudia, Wang, Xin, Fontana, Adriano, Hathi, Nimish P., Iyer, Kartheik G., Alavi, Anahita, Colbert, James, Grogin, Norman, Koekemoer, Anton, Nedkova, Kalina V., Hayes, Matthew, Prichard, Laura, Siana, Brian, Smith, Brent M., Windhorst, Rogier, Ashcraft, Teresa, Bagley, Micaela, Baronchelli, Ivano, Barro, Guillermo, Blanche, Alex, Broussard, Adam, Carleton, Timothy, Chartab, Nima, Codoreanu, Alex, Cohen, Seth, Conselice, Christopher, Dai, Y. Sophia, Darvish, Behnam, Dave, Romeel, DeGroot, Laura, De Mello, Duilia, Dickinson, Mark, Emami, Najmeh, Ferguson, Henry, Ferreira, Leonardo, Finkelstein, Keely, Finkelstein, Steven, Gardner, Jonathan P., Gawiser, Eric, Gburek, Timothy, Giavalisco, Mauro, Grazian, Andrea, Gronwall, Caryl, Guo, Yicheng, Haro, Pablo Arrabal, Hemmati, Shoubaneh, Howell, Justin, Jansen, Rolf A., Ji, Zhiyuan, Kaviraj, Sugata, Kim, Keunho J., Kurczynski, Peter, Lazar, Ilin, Lucas, Ray A., MacKenty, John, Mantha, Kameswara Bharadwaj, Martin, Alec, Martin, Garreth, McCabe, Tyler, Mobasher, Bahram, Morales, Alexa M., O'Connell, Robert, Olsen, Charlotte, Otteson, Lillian, Ravindranath, Swara, Redshaw, Caleb, Rutkowski, Michael, Robertson, Brant, Sattari, Zahra, Soto, Emmaris, Sun, Lei, Taamoli, Sina, Vanzella, Eros, Yung, L. Y. Aaron, Zabelle, Bonnabelle
The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS fields (GOODS-N, GOODS-S, COSMOS, and EGS). We combine this newly acq
Externí odkaz:
http://arxiv.org/abs/2410.16404
Autor:
Nedkova, Kalina V., Häußler, Boris, Marchesini, Danilo, Brammer, Gabriel B., Feinstein, Adina D., Johnston, Evelyn J., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Martis, Nicholas S., Muzzin, Adam, Rafelski, Marc, Shipley, Heath V., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E.
Using deep imaging from the CANDELS and HFF surveys, we present bulge+disc decompositions with GalfitM for $\sim$17,000 galaxies over $0.2 \leq z\leq 1.5$. We use various model parameters to select reliable samples of discs and bulges, and derive the
Externí odkaz:
http://arxiv.org/abs/2406.14613
Autor:
Nedkova, Kalina V., Rafelski, Marc, Teplitz, Harry I., Mehta, Vihang, DeGroot, Laura, Ravindranath, Swara, Alavi, Anahita, Beckett, Alexander, Grogin, Norman A., Häußler, Boris, Koekemoer, Anton M., Oyarzún, Grecco A., Prichard, Laura, Revalski, Mitchell, Snyder, Gregory F., Sunnquist, Ben, Wang, Xin, Windhorst, Rogier A., Chartab, Nima, Conselice, Christopher J., Guo, Yicheng, Hathi, Nimish, Hayes, Matthew J., Ji, Zhiyuan, Kim, Keunho J., Lucas, Ray A., Mobasher, Bahram, O'Connell, Robert W., Sattari, Zahra, Smith, Brent M., Taamoli, Sina, Yung, L. Y. Aaron, Team, the UVCANDELS
We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest-frame far-UV for $\sim$16,000 disk-like galaxies over $0.5\leq z \leq 3$. We compare these
Externí odkaz:
http://arxiv.org/abs/2405.10908
Autor:
Revalski, Mitchell, Rafelski, Marc, Henry, Alaina, Fossati, Matteo, Fumagalli, Michele, Dutta, Rajeshwari, Pirzkal, Norbert, Beckett, Alexander, Battaia, Fabrizio Arrigoni, Dayal, Pratika, D'Odorico, Valentina, Lusso, Elisabeta, Nedkova, Kalina V., Prichard, Laura J., Papovich, Casey, Peroux, Celine
Using more than 100 galaxies in the MUSE Ultra Deep Field with spectroscopy from the Hubble Space Telescope's Wide Field Camera 3 and the Very Large Telescope's Multi Unit Spectroscopic Explorer, we extend the gas-phase mass-metallicity relation (MZR
Externí odkaz:
http://arxiv.org/abs/2403.17047
The many unique properties of galaxies are shaped by physical processes that affect different components of the galaxy - like the bulges and discs - in different ways, and leave characteristic imprints on the light and spectra of these components. Di
Externí odkaz:
http://arxiv.org/abs/2402.00959
Autor:
Sun, Lei, Wang, Xin, Teplitz, Harry I., Mehta, Vihang, Alavi, Anahita, Rafelski, Marc, Windhorst, Rogier A., Scarlata, Claudia, Gardner, Jonathan P., Smith, Brent M., Sunnquist, Ben, Prichard, Laura, Cheng, Yingjie, Grogin, Norman, Hathi, Nimish P., Hayes, Matthew, Koekemoer, Anton M., Mobasher, Bahram, Nedkova, Kalina V., O'Connell, Robert, Robertson, Brant, Taamoli, Sina, Yung, L. Y. Aaron, Brammer, Gabriel, Colbert, James, Conselice, Christopher, Gawiser, Eric, Guo, Yicheng, Jansen, Rolf A., Ji, Zhiyuan, Lucas, Ray A., Rutkowski, Michael, Siana, Brian, Vanzella, Eros, Ashcraft, Teresa, Bagley, Micaela, Baronchelli, Ivano, Barro, Guillermo, Blanche, Alex, Broussard, Adam, Carleton, Timothy, Chartab, Nima, Codoreanu, Alex, Cohen, Seth, Dai, Y. Sophia, Darvish, Behnam, Davé, Romeel, DeGroot, Laura, De Mello, Duilia, Dickinson, Mark, Emami, Najmeh, Ferguson, Henry, Ferreira, Leonardo, Finkelstein, Keely, Finkelstein, Steven, Gburek, Timothy, Giavalisco, Mauro, Grazian, Andrea, Gronwall, Caryl, Hemmati, Shoubaneh, Howell, Justin, Iyer, Kartheik, Kaviraj, Sugata, Kurczynski, Peter, Lazar, Ilin, MacKenty, John, Mantha, Kameswara Bharadwaj, Martin, Alec, Martin, Garreth, McCabe, Tyler, Olsen, Charlotte, Otteson, Lillian, Ravindranath, Swara, Redshaw, Caleb, Sattari, Zahra, Soto, Emmaris, Zabelle, Bonnabelle, team, the UVCANDELS
UVCANDELS is a HST Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields: GOODS-N, GOODS-S, EGS, and COSMOS, covering a total area of $\sim426$ arc
Externí odkaz:
http://arxiv.org/abs/2311.15664
Autor:
Martin, Alec, Guo, Yicheng, Wang, Xin, Koekemoer, Anton M., Rafelski, Marc, Teplitz, Harry I., Windhorst, Rogier A., Alavi, Anahita, Grogin, Norman A., Prichard, Laura, Sunnquist, Ben, Ceverino, Daniel, Chartab, Nima, Conselice, Christopher J., Dai, Y. Sophia, Dekel, Avishai, Gardner, Johnathan P., Gawiser, Eric, Hathi, Nimish P., Hayes, Matthew J., Jansen, Rolf A., Ji, Zhiyuan, Koo, David C., Lucas, Ray A., Mandelker, Nir, Mehta, Vihang, Mobasher, Bahram, Nedkova, Kalina V., Primack, Joel, Ravindranath, Swara, Robertson, Brant E., Rutkowski, Michael J., Sattari, Zahra, Soto, Emmaris, Yung, L. Y. Aaron
Publikováno v:
ApJ 955 106 (2023)
Giant star-forming clumps are a prominent feature of star-forming galaxies (SFGs) and contain important clues on galaxy formation and evolution. However, basic demographics of clumps and their host galaxies remain uncertain. Using the HST/WFC3 F275W
Externí odkaz:
http://arxiv.org/abs/2308.00041
Autor:
van der Wel, Arjen, Martorano, Marco, Haussler, Boris, Nedkova, Kalina V., Miller, Tim B., Brammer, Gabriel B., van de Ven, Glenn, Leja, Joel, Bezanson, Rachel S., Muzzin, Adam, Marchesini, Danilo, de Graaff, Anna, Kriek, Mariska, Bell, Eric F., Franx, Marijn
We use CEERS JWST/NIRCam imaging to measure rest-frame near-IR light profiles of $>$500 $M_\star>10^{10}~M_\odot$ galaxies in the redshift range $0.5
Externí odkaz:
http://arxiv.org/abs/2307.03264
Autor:
Revalski, Mitchell, Rafelski, Marc, Fumagalli, Michele, Fossati, Matteo, Pirzkal, Norbert, Sunnquist, Ben, Prichard, Laura J., Henry, Alaina, Bagley, Micaela, Dutta, Rajeshwari, Papini, Giulia, Battaia, Fabrizio Arrigoni, D'Odorico, Valentina, Dayal, Pratika, Estrada-Carpenter, Vicente, Lofthouse, Emma K., Lusso, Elisabeta, Morris, Simon L., Nedkova, Kalina V., Papovich, Casey, Peroux, Celine
We present extremely deep Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) observations of the MUSE Ultra Deep Field (MUDF). This unique region of the sky contains two quasars at $z \approx$ 3.22 that are separated by only $\sim$500 kpc, provi
Externí odkaz:
http://arxiv.org/abs/2302.01345
Autor:
Tan, Vivian Yun Yan, Muzzin, Adam, Marsan, Z. Cemile, Sok, Visal, Alcorn, Leo Y., Matharu, Jasleen, Shipley, Heath, Marchesini, Danilo, Nedkova, Kalina V., Martis, Nicholas, van der Wel, Arjen, Whitaker, Katherine E.
One of the challenges in understanding the quenching processes for galaxies is connecting progenitor star-forming populations to their descendant quiescent populations over cosmic time. Here we attempt a novel approach to this challenge by assuming t
Externí odkaz:
http://arxiv.org/abs/2205.07913