Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Kelson, Daniel D."'
Autor:
Cohn, Jonathan H., Leja, Joel, Tran, Kim-Vy H., Forrest, Ben, Johnson, Benjamin D., Tillman, Megan, Alcorn, Leo, Conroy, Charlie, Glazebrook, Karl, Kacprzak, Glenn G., Kelson, Daniel D., Nanayakkara, Themiya, Papovich, Casey, van Dokkum, Pieter G., Yuan, Tiantian
Using the \prospector\ spectral energy distribution (SED) fitting code, we analyze the properties of 19 Extreme Emission Line Galaxies (EELGs) identified in the bluest composite SED in the \zfourge\ survey at $2.5 \leq z \leq 4$. \prospector\ include
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0b14617f23b977fd35a0a46d52df625
Autor:
Yang, Yujin, Zabludoff, Ann, Jahnke, Knud, Eisenstein, Daniel, Dav��, Romeel, Shectman, Stephen A., Kelson, Daniel D.
Exploring the origin of Ly-alpha nebulae (blobs) requires measurements of their gas kinematics that are impossible with only the resonant, optically-thick LyA line. To define gas motions relative to the systemic velocity of the blob, the LyA line mus
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6c8117ebfe8d9de171baafd6c7e9067
http://arxiv.org/abs/1104.3597
http://arxiv.org/abs/1104.3597
Clusters of galaxies have long been used as laboratories for the study of galaxy evolution, but despite intense, recent interest in feedback between AGNs and their hosts, the impact of environment on these relationships remains poorly constrained. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f369fe36b41c3c6c28644fb018ecd16d
http://arxiv.org/abs/1101.0812
http://arxiv.org/abs/1101.0812
Autor:
Tran, Kim-Vy H., Franx, Marijn, Illingworth, Garth D., van Dokkum, Pieter, Kelson, Daniel D., Magee, Daniel
We select E+A candidates from a spectroscopic dataset of ~800 field galaxies and measure the E+A fraction at 0.3
Accepted by ApJ
Accepted by ApJ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7114e4c832cc465a30af52633688c2cd
Autor:
Ferrarese, Laura, Ford, Holland C., Huchra, John, Kennicutt, Robert C., Mould, Jeremy R., Sakai, Shoko, Freedman, Wendy L., Stetson, Peter B., Madore, Barry F., Gibson, Brad K., Graham, John A., Hughes, Shaun M., Illingworth, Garth D., Kelson, Daniel D., Macri, Lucas, Sebo, Kim, Silbermann, N. A.
We present a compilation of Cepheid distance moduli and data for four secondary distance indicators that employ stars in the old stellar populations: the planetary nebula luminosity function (PNLF), the globular cluster luminosity function (GCLF), th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::305a015aeffd7eba2abba37f737f978e
http://arxiv.org/abs/astro-ph/9910501
http://arxiv.org/abs/astro-ph/9910501
Autor:
Ferrarese, Laura, Mould, Jeremy R., Kennicutt, Robert C., Huchra, John, Ford, Holland C., Freedman, Wendy L., Stetson, Peter B., Madore, Barry F., Sakai, Shoko, Gibson, Brad K., Graham, John A., Hughes, Shaun M., Illingworth, Garth D., Kelson, Daniel D., Macri, Lucas, Sebo, Kim, Silbermann, N. A.
A Cepheid-based calibration is derived for four distance indicators that utilize stars in the old stellar populations: the tip of the red giant branch (TRGB), the planetary nebula luminosity function (PNLF), the globular cluster luminosity function (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8a2453d70a68173538250e964396d91
http://arxiv.org/abs/astro-ph/9908192
http://arxiv.org/abs/astro-ph/9908192
Autor:
Gibson, Brad K., Stetson, Peter B., Freedman, Wendy L., Mould, Jeremy R., Kennicutt, Robert C., Huchra, John P., Sakai, Shoko, Graham, John A., Fassett, Caleb I., Kelson, Daniel D., Ferrarese, Laura, Hughes, Shaun M. G., Illingworth, Garth D., Macri, Lucas M., Madore, Barry F., Sebo, Kim M., Silbermann, Nancy A.
Cepheid-based distances to seven Type Ia supernovae (SNe)-host galaxies have been derived using the standard HST Key Project on the Extragalactic Distance Scale pipeline. For the first time, this allows for a transparent comparison of data accumulate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64298123d6c585140facda4609283b84
http://arxiv.org/abs/astro-ph/9908149
http://arxiv.org/abs/astro-ph/9908149
The cluster CL1358+62 displays a prominent red arc in WFPC2 images obtained with the Hubble Space Telescope. Keck spectra of the arc show Ly alpha emission at 7204 Angstrom, a continuum drop blueward of the line, and several absorption lines to the r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a28b04bfd224b9a59663942b2b071fde
http://arxiv.org/abs/astro-ph/9704090
http://arxiv.org/abs/astro-ph/9704090