Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Hensley, Hagan"'
Autor:
Steinhardt, Charles L., Sneppen, Albert, Hensley, Hagan, Jermyn, Adam S., Mostafa, Basel, Weaver, John R., Brammer, Gabriel, Clark, Thomas H., Davidzon, Iary, Diaconu, Andrei C., Mobasher, Bahram, Rusakov, Vadim, Toft, Sune
The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The introduction of an additional parameter, $T_{IMF}$ , into photometric template fitting, suggest most galaxies obey an IMF
Externí odkaz:
http://arxiv.org/abs/2206.01750
Autor:
Steinhardt, Charles L., Sneppen, Albert, Mostafa, Basel, Hensley, Hagan, Jermyn, Adam S., Lopez, Adrian, Weaver, John, Brammer, Gabriel, Clark, Thomas H., Davidzon, Iary, Diaconu, Andrei C., Mobasher, Bahram, Rusakov, Vadim, Toft, Sune
The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The introduction of an additional parameter, $T_{IMF}$ , into photometric template fitting, allows galaxies to be fit with a
Externí odkaz:
http://arxiv.org/abs/2205.14161
Autor:
Sneppen, Albert, Steinhardt, Charles L., Hensley, Hagan, Jermyn, Adam S., Mostafa, Basel, Weaver, John R.
A universal stellar initial mass function (IMF) should not be expected from theoretical models of star formation, but little conclusive observational evidence for a variable IMF has been uncovered. In this paper, a parameterization of the IMF is intr
Externí odkaz:
http://arxiv.org/abs/2205.11536
Autor:
Steinhardt, Charles L., Jauzac, Mathilde, Acebron, Ana, Atek, Hakim, Capak, Peter, Davidzon, Iary, Eckert, Dominique, Harvey, David, Koekemoer, Anton M., Lagos, Claudia D. P., Mahler, Guillaume, Montes, Mireia, Niemiec, Anna, Nonino, Mario, Oesch, P. A., Richard, Johan, Rodney, Steven A., Schaller, Matthieu, Sharon, Keren, Strolger, Louis-Gregory, Allingham, Joseph, Amara, Adam, Bah'e, Yannick, Boehm, Celine, Bose, Sownak, Bouwens, Rychard J., Bradley, Larry D., Brammer, Gabriel, Broadhurst, Tom, Canas, Rodrigo, Cen, Renyue, Clement, Benjamin, Clowe, Douglas, Coe, Dan, Connor, Thomas, Darvish, Behnam, Diego, Jose M., Ebeling, Harald, Edge, A. C., Egami, Eiichi, Ettori, Stefano, Faisst, Andreas L., Frye, Brenda, Furtak, Lukas J., Gomez-Guijarro, C., Gonzalez, J. D. Remolina, Gonzalez, Anthony, Graur, Or, Gruen, Daniel, Hensley, Hagan, Hovis-Afflerbach, Beryl, Jablonka, Pascale, Jha, Saurabh W., Jullo, Eric, Kneib, Jean-Paul, Kokorev, Vasily, Lagattuta, David J., Limousin, Marceau, von der Linden, Anja, Linzer, Nora B., Lopez, Adrian, Magdis, Georgios E., Massey, Richard, Masters, Daniel C., Maturi, Matteo, McCully, Curtis, McGee, Sean L., Meneghetti, Massimo, Mobasher, Bahram, Moustakas, Leonidas A., Murphy, Eric J., Natarajan, Priyamvada, Neyrinck, Mark, O'Connor, Kyle, Oguri, Masamune, Pagul, Amanda, Rhodes, Jason, Rich, R. Michael, Robertson, Andrew, Sereno, Mauro, Shan, Huanyuan, Smith, Graham P., Sneppen, Albert, Squires, Gordon K., Tam, Sut-Ieng, Tchernin, Celine, Toft, Sune, Umetsu, Keiichi, Weaver, John R., van Weeren, R. J., Williams, Liliya L. R., Wilson, Tom J., Yan, Lin, Zitrin, Adi
The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. BUFFALO will expand existing coverage of the Hubble Frontier Fields (HF
Externí odkaz:
http://arxiv.org/abs/2001.09999