Zobrazeno 1 - 10
of 102
pro vyhledávání: '"Peth, Michael"'
Autor:
Müller, Helena Sophie1 (AUTHOR) helena.mueller@wiso.uni-koeln.de, Becker-Peth, Michael2 (AUTHOR), Kuntz, Ludwig1 (AUTHOR), on behalf of Neo-CamCare (AUTHOR), Scholten, Nadine (AUTHOR), Müller, Andreas (AUTHOR), Dresbach, Till (AUTHOR), Hellmich, Martin (AUTHOR), Samel, Christina (AUTHOR), Woopen, Christiane (AUTHOR), Jannes, Christiane (AUTHOR), Spiecker gen Döhmann, Indra (AUTHOR), Bretthauer, Sebastian (AUTHOR), Horenkamp-Sonntag, Dirk (AUTHOR), Wobbe-Ribinski, Stefanie (AUTHOR)
Publikováno v:
BMC Nursing. 7/2/2024, Vol. 23 Issue 1, p1-10. 10p.
Autor:
Barro, Guillermo, Perez-Gonzalez, Pablo G., Cava, Antonio, Brammer, Gabriel, Pandya, Viraj, Moral, Carmen Eliche, Esquej, Pilar, Dominguez-Sanchez, Helena, Pampliega, Belen Alcalde, Guo, Yicheng, Koekemoer, Anton M., Trump, Jonathan R., Ashby, Matthew L. N., Cardiel, Nicolas, Castellano, Marco, Conselice, Christopher J., Dickinson, Mark E., Dolch, Timothy, Donley, Jennifer L., Briones, Nestor Espino, Faber, Sandra M., Fazio, Giovanni G., Ferguson, Henry, Finkelstein, Steve, Fontana, Adriano, Galametz, Audrey, Gardner, Jonathan P., Gawiser, Eric, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Hathi, Nimish P., Hemmati, Shoubaneh, Hernan-Caballero, Antonio, Kocevski, Dale, Koo, David C., Kodra, Dritan, Lee, Kyoung-Soo, Lin, Lihwai, Lucas, Ray A., Mobasher, Bahram, McGrath, Elizabeth J., Nandra, Kirpal, Nayyeri, Hooshang, Newman, Jeffrey A., Pforr, Janine, Peth, Michael, Rafelski, Marc, Rodriguez-Munoz, Lucia, Salvato, Mara, Stefanon, Mauro, van der Wel, Arjen, Willner, Steven P., Wiklind, Tommy, Wuyts, Stijn
Publikováno v:
The Astrophysical Journal Supplement Series, Volume 243, Number 2, 2019
We present a WFC3 F160W ($H$-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts and stellar parameters derived from the analysis of the multi-wavelength
Externí odkaz:
http://arxiv.org/abs/1908.00569
Akademický článek
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Autor:
Mantha, Kameswara Bharadwaj, McIntosh, Daniel H., Brennan, Ryan, Ferguson, Henry C., Kodra, Dritan, Newman, Jeffrey A., Rafelski, Marc, Somerville, Rachel S., Conselice, Christopher J., Cook, Joshua S., Hathi, Nimish P., Koo, David C., Lotz, Jennifer M., Simmons, Brooke D., Straughn, Amber N., Synder, Gregory F., Wuyts, Stijn, Bell, Eric F., Dekel, Avishai, Kartaltepe, Jeyhan, Kocevski, Dale D., Koekemoer, Anton M., Lee, Seong-Kook, Lucas, Ray A., Pacifici, Camilla, Peth, Michael A., Barro, Guillermo, Dahlen, Tomas, Finkelstein, Steven L., Fontana, Adriano, Galametz, Audrey, Grogin, Norman A., Guo, Yicheng, Mobasher, Bahram, Nayyeri, Hooshang, Perez-Gonzalez, Pablo G., Pforr, Janine, Santini, Paola, Stefanon, Mauro, Wiklind, Tommy
The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development ($1{\leq}z{\leq}3$). We use close-pair statistics to objectively study the incidence of massive
Externí odkaz:
http://arxiv.org/abs/1712.06611
Autor:
Stefanon, Mauro, Yan, Haojing, Mobasher, Bahram, Barro, Guillermo, Donley, Jennifer L., Fontana, Adriano, Hemmati, Shoubaneh, Koekemoer, Anton M., Lee, BoMee, Lee, Seong-Kook, Nayyeri, Hooshang, Peth, Michael, Pforr, Janine, Salvato, Mara, Wiklind, Tommy, Wuyts, Stijn, Ashby, Matthew L. N., Castellano, Marco, Conselice, Christopher J., Cooper, Michael C., Cooray, Asantha R., Dolch, Timothy, Ferguson, Henry, Galametz, Audrey, Giavalisco, Mauro, Guo, Yicheng, Willner, Steven P., Dickinson, Mark E., Faber, Sandra M., Fazio, Giovanni G., Gardner, Jonathan P., Gawiser, Eric, Grazian, Andrea, Grogin, Norman A., Kocevski, Dale, Koo, David C., Lee, Kyoung-Soo, Lucas, Ray A., McGrath, Elizabeth J., Nandra, Kirpal, Newman, Jeffrey A., van der Wel, Arjen
We present a 0.4-8$\mu$m multi-wavelength photometric catalog in the Extended Groth Strip (EGS) field. This catalog is built on the Hubble Space Telescope (HST) WFC3 and ACS data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
Externí odkaz:
http://arxiv.org/abs/1703.05768
Autor:
Simmons, B. D., Lintott, Chris, Willett, Kyle W., Masters, Karen L., Kartaltepe, Jeyhan S., Häußler, Boris, Kaviraj, Sugata, Krawczyk, Coleman, Kruk, S. J., McIntosh, Daniel H., Smethurst, R. J., Nichol, Robert C., Scarlata, Claudia, Schawinski, Kevin, Conselice, Christopher J., Almaini, Omar, Ferguson, Henry C., Fortson, Lucy, Hartley, William, Kocevski, Dale, Koekemoer, Anton M., Mortlock, Alice, Newman, Jeffrey A., Bamford, Steven P., Grogin, N. A., Lucas, Ray A., Hathi, Nimish P., McGrath, Elizabeth, Peth, Michael, Pforr, Janine, Rizer, Zachary, Wuyts, Stijn, Barro, Guillermo, Bell, Eric F., Castellano, Marco, Dahlen, Tomas, Ownsworth, Avishai Dekel Jamie, Faber, Sandra M., Finkelstein, Steven L., Fontana, Adriano, Galametz, Audrey, Grützbauch, Ruth, Koo, David, Lotz, Jennifer, Mobasher, Bahram, Mozena, Mark, Salvato, Mara, Wiklind, Tommy
We present quantified visual morphologies of approximately 48,000 galaxies observed in three Hubble Space Telescope legacy fields by the Cosmic And Near-infrared Deep Extragalactic Legacy Survey (CANDELS) and classified by participants in the Galaxy
Externí odkaz:
http://arxiv.org/abs/1610.03070
Autor:
Lee, Seong-Kook, Im, Myungshin, Kim, Jae-Woo, Lotz, Jennifer, McPartland, Conor, Peth, Michael, Koekemoer, Anton
Using a stellar mass limited sample of $\sim 46,600$ galaxies ($M_* > 10^{9.1}\,M_{\odot}$) at $0.5 < z < 2$, we show that the tellar mass, rather than the environment, is the main parameter controlling quenching of star formation in galaxies with $M
Externí odkaz:
http://arxiv.org/abs/1508.01294
Autor:
Simons, Raymond C., Kassin, Susan A., Weiner, Benjamin J., Heckman, Timothy M., Lee, Janice C., Lotz, Jennifer M., Peth, Michael, Tchernyshyov, Kirill
We study the stellar mass Tully-Fisher relation (TFR, stellar mass versus rotation velocity) for a morphologically blind selection of emission line galaxies in the field at redshifts 0.1 $<$ z $<$ 0.375. Kinematics ($\sigma_g$, V$_{rot}$) are measure
Externí odkaz:
http://arxiv.org/abs/1506.04144
Autor:
Peth, Michael A., Lotz, Jennifer M., Freeman, Peter E., McPartland, Conor, Mortazavi, S. Alireza, Snyder, Gregory F., Barro, Guillermo, Grogin, Norman A., Guo, Yicheng, Hemmati, Shoubaneh, Kartaltepe, Jeyhan S., Kocevski, Dale D., Koekemoer, Anton M., McIntosh, Daniel H., Nayyeri, Hooshang, Papovich, Casey, Primack, Joel R., Simons, Raymond C.
Important but rare and subtle processes driving galaxy morphology and star-formation may be missed by traditional spiral, elliptical, irregular or S\'ersic bulge/disk classifications. To overcome this limitation, we use a principal component analysis
Externí odkaz:
http://arxiv.org/abs/1504.01751