Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Katie Jameson"'
Publikováno v:
Bio-Protocol, Vol 12, Iss 21 (2022)
Ubiquitination is a post-translational modification conserved across eukaryotic species. It contributes to a variety of regulatory pathways, including proteasomal degradation, DNA repair, and cellular differentiation. The ubiquitination of substrate
Externí odkaz:
https://doaj.org/article/af110d8aaedd46bb9ace42bb07371454
Autor:
Katie Jameson
The Small Magellanic Cloud (SMC) provides the only laboratory to study the detailed physics of star formation and the interstellar medium relevant to the high redshift universe. Not only is the transition from warm to cold neutral gas a rate limiting
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20416f53553bacd5367ecbf6514da813
Autor:
Karl D. Gordon, Annie Hughes, C. Bot, Monica Rubio, Remy Indebetouw, Frank P. Israel, Maud Galametz, Julia Roman-Duval, Suzanne C. Madden, E. Montiel, Katie Jameson, Marc Sauvage, Akiko Kawamura, Martha L. Boyer, D. Paradis, Karin Sandstrom, Aigen Li, Frédéric Galliano, Mikako Matsuura, Brian Babler, J. Seale, Ramin A. Skibba, Pasquale Panuzzo, Marta Sewilo, Vianney Lebouteiller, Toshikazu Onishi, Yasuo Fukui, Jean-Philippe Bernard, Kirill Tchernyshyov, Karl Misselt, Sacha Hony, Margaret Meixner, K. Okumura, Alberto D. Bolatto, Geoffrey C. Clayton, Charles W. Engelbracht
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, 2017, 837 (1), pp.98. ⟨10.3847/1538-4357/aa6042⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 837 (1), pp.98. ⟨10.3847/1538-4357/aa6042⟩
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 837(1), 98
The Astrophysical journal letters, 2017, 837 (1), pp.98. ⟨10.3847/1538-4357/aa6042⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 837 (1), pp.98. ⟨10.3847/1538-4357/aa6042⟩
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 837(1), 98
International audience; Not Available
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::333e8e282d45edf16a336bc0b8c87b0d
https://hal.science/hal-02105249
https://hal.science/hal-02105249
Autor:
Mikako Matsuura, Jonathan Seale, Brian Babler, Charles W. Engelbracht, Maud Galametz, Karl D. Gordon, Kirill Tchernyshyov, Yasuo Fukui, Monica Rubio, Sacha Hony, E. Montiel, Marc Sauvage, Karl Misselt, Frédéric Galliano, Geoffrey C. Clayton, Jean-Philippe Bernard, Alberto D. Bolatto, Marta Sewilo, Remy Indebetouw, Frank P. Israel, Karin Sandstrom, Vianney Lebouteiller, Ramin A. Skibba, Annie Hughes, K. Okumura, Toshikazu Onishi, Akiko Kawamura, Pasquale Panuzzo, Katie Jameson, Martha L. Boyer, Suzanne C. Madden, Margaret Meixner, Caroline Bot, Deborah Paradis, Julia Roman-Duval, Aigen Li
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2014, 797 (2), pp.85. ⟨10.1088/0004-637X/797/2/85⟩
The Astrophysical journal letters, 2014, 797 (2), pp.85. ⟨10.1088/0004-637X/797/2/85⟩
Astronomy & Astrophysics
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
ASTROPHYSICAL JOURNAL
The Astrophysical journal letters, Bristol : IOP Publishing, 2014, 797 (2), pp.85. ⟨10.1088/0004-637X/797/2/85⟩
The Astrophysical journal letters, 2014, 797 (2), pp.85. ⟨10.1088/0004-637X/797/2/85⟩
Astronomy & Astrophysics
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
ASTROPHYSICAL JOURNAL
The dust properties in the Large and Small Magellanic Clouds are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 micron. Three simple models of dust emission were fit to the observations: a single temper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f1691e36df54581a5533bd28ba394d4
http://arxiv.org/abs/1406.6066
http://arxiv.org/abs/1406.6066
Autor:
Alberto D. Bolatto, Martha P. Haynes, Kristen B. W. McQuinn, John J. Salzer, Riccardo Giovanelli, Elizabeth A. K. Adams, John M. Cannon, Katherine L. Rhode, Edward Molter, Evan D. Skillman, Elijah Z. Bernstein-Cooper, Rodrigo Herrera-Camus, Steven R. Warren, Katie Jameson
Publikováno v:
The Astrophysical Journal. 814:30
We present sensitive CO (J = 1→ 0) emission line observations of three metalpoor dwarf irregular galaxies Leo P (Z∼3% Z ), Sextans A (Z∼7.5% Z ), and Sextans B (Z∼7.5% Z ), all obtained with the Combined Array for Millimeterwave Astronomy (CA
Autor:
Steven R. Warren, Edward Molter, John M. Cannon, Alberto D. Bolatto, Elizabeth A. K. Adams, Elijah Z. Bernstein-Cooper, Riccardo Giovanelli, Martha P. Haynes, Rodrigo Herrera-Camus, Katie Jameson, Kristen B. W. McQuinn, Katherine L. Rhode, John J. Salzer, Evan D. Skillman
Publikováno v:
Astrophysical Journal; 11/20/2015, Vol. 814 Issue 1, p1-1, 1p