Zobrazeno 1 - 10
of 393
pro vyhledávání: '"Kollmeier, J."'
Autor:
Kreckel, K., Egorov, O. V., Egorova, E., Blanc, G. A., Drory, N., Kounkel, M., Mendez-Delgado, J. E., Roman-Zuniga, C. G., Sanchez, S. F., Stringfellow, G. S., Stutz, A. M., Zari, E., Barrera-Ballesteros, J. K., Bizyaev, D., Brownstein, J. R., Congiu, E., Fernandez-Trincado, J. G., Garcia, P., Hillenbrand, L., Ibarra-Medel, H. J., Jin, Y., Johnston, E. J., Jones, A. M., Kim, J. Serena, Kollmeier, J. A., Kong, S., Krishnarao, D., Kumari, N., Li, J., Long, K., Mata-Sanchez, A., Mejia-Narvaez, A., Popa, S. A., Rix, H-W, Sattler, N., Serna, J., Singh, A., Sanchez-Gallego, J. R., Wofford, A., Wong, T.
Publikováno v:
A&A 689, A352 (2024)
The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedback, but its ~12 deg diameter on the sky requires a dedicated approach
Externí odkaz:
http://arxiv.org/abs/2405.14943
Autor:
Zasowski, G., Cohen, R. E., Chojnowski, S. D., Santana, F., Oelkers, R. J., Andrews, B., Beaton, R. L., Bender, C., Bird, J. C., Bovy, J., Carlberg, J. K., Covey, K., Cunha, K., Dell’Agli, F., Fleming, Scott W., Frinchaboy, P. M., García-Hernández, D. A., Harding, P., Holtzman, J., Johnson, J. A., Kollmeier, J. A., Majewski, S. R., Mészáros, Sz., Munn, J., Muñoz, R. R., Ness, M. K., Nidever, D. L., Poleski, R., Román-Zúñiga, C., Shetrone, M., Simon, J. D., Smith, V. V., Sobeck, J. S., Stringfellow, G. S., Szigetiáros, L., Tayar, J., Troup, N.
APOGEE-2 is a high-resolution, near-infrared spectroscopic survey observing similar to 3. x. 10(5) stars across the entire sky. It is the successor to APOGEE and is part of the Sloan Digital Sky Survey IV (SDSS-IV). APOGEE-2 is expanding on APOGEE's
Externí odkaz:
http://hdl.handle.net/10150/626051
http://arizona.openrepository.com/arizona/handle/10150/626051
http://arizona.openrepository.com/arizona/handle/10150/626051
Autor:
Elias-Rosa, N., Chen, P., Benetti, S., Dong, Subo, Prieto, J. L., Cappellaro, E., Kollmeier, J. A., Morrell, N., Piro, A. L., Phillips, M. M.
Publikováno v:
A&A 652, A115 (2021)
There is a wide consensus that type Ia supernovae (SN Ia) originate from the thermonuclear explosion of CO white dwarfs (WD), with the lack of hydrogen in the observed spectra as a distinctive feature. Here, we present SN 2016jae, which was classifie
Externí odkaz:
http://arxiv.org/abs/2106.15340
Autor:
Gutiérrez, C. P., Sullivan, M., Martinez, L., Bersten, M. C., Inserra, C., Smith, M., Anderson, J. P., Pan, Y. -C., Pastorello, A., Galbany, L., Nugent, P., Angus, C. R., Barbarino, C., Chen, T. -W., Davis, T. M., Della Valle, M., Foley, R. J., Fraser, M., Frohmaier, C., González-Gaitán, S., Lewis, G. F., Gromadzki, M., Kankare, E., Kokotanekova, R., Kollmeier, J., Magee, M. R., Maguire, K., Möller, A., Morrell, N., Nicholl, M., Pursiainen, M., Sollerman, J., Sommer, N. E., Swann, E., Tucker, B. E., Wiseman, P., Aguena, M., Allam, S., Avila, S., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Eifler, T. F., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Morganson, E., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Varga, T. N., Walker, A. R., Wilkinson, R.
We present DES16C3cje, a low-luminosity, long-lived type II supernova (SN II) at redshift 0.0618, detected by the Dark Energy Survey (DES). DES16C3cje is a unique SN. The spectra are characterized by extremely narrow photospheric lines corresponding
Externí odkaz:
http://arxiv.org/abs/2001.11559
Autor:
Prieto, Jose L., Chen, Ping, Dong, Subo, Bose, S., Gal-Yam, A., Holoien, T. W. -S., Kollmeier, J. A., Phillips, M. M., Shappee, B. J.
We present optical photometry and spectroscopy of the Type Ia supernova SN2018cqj/ATLAS18qtd. The supernova exploded in an isolated region at $\sim 65$~kpc from the S0 galaxy IC~550 at $z=0.0165$ ($D\approx 74$~Mpc) and has a redshift consistent with
Externí odkaz:
http://arxiv.org/abs/1909.05267
Autor:
Pellegrini, E. W., Drory, N., B., Guillermo A., Kollmeier, J. A., Tuttle, S. E., Lopez, L. A., Simon, Josh, Jones, A. M., Avila-Reese, V., Kreckel, K., Yan, R.
Crucial progress in our understanding of star formation and feedback will depend on the ability to obtain spatially resolved spectroscopic observations of \ion{H}{ii} regions, from which reliable instantaneous measurements of their physical condition
Externí odkaz:
http://arxiv.org/abs/1905.00311
Autor:
Zasowski, G., Finkbeiner, D. P., Green, G. M., Kollmeier, J. A., Nataf, D. M., Peek, J. E. G., Schlafly, E. F., Aguirre, V. Silva, Speagle, J. S., Tchernyshyov, K., Trujillo, J. D., Zucker, C.
Galactic interstellar dust has a profound impact not only on our observations of objects throughout the Universe, but also on the morphology, star formation, and chemical evolution of the Galaxy. The advent of massive imaging and spectroscopic survey
Externí odkaz:
http://arxiv.org/abs/1903.05150
Autor:
Drout, M. R., Piro, A. L., Shappee, B. J., Kilpatrick, C. D., Simon, J. D., Contreras, C., Coulter, D. A., Foley, R. J., Siebert, M. R., Morrell, N., Boutsia, K., Di Mille, F., Holoien, T. W. -S., Kasen, D., Kollmeier, J. A., Madore, B. F., Monson, A. J., Murguia-Berthier, A., Pan, Y. -C., Prochaska, J. X., Ramirez-Ruiz, E., Rest, A., Adams, C., Alatalo, K., Bañados, E., Baughman, J., Beers, T. C., Bernstein, R. A., Bitsakis, T., Campillay, A., Hansen, T. T., Higgs, C. R., Ji, A. P., Maravelias, G., Marshall, J. L., Bidin, C. Moni, Prieto, J. L., Rasmussen, K. C., Rojas-Bravo, C., Strom, A. L., Ulloa, N., Vargas-González, J., Wan, Z., Whitten, D. D.
On 2017 August 17, gravitational waves were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB170817A. An optical transient source, Swope Supernova Survey 17a (SSS17a), was subsequently identified
Externí odkaz:
http://arxiv.org/abs/1710.05443
Autor:
Shappee, B. J., Simon, J. D., Drout, M. R., Piro, A. L., Morrell, N., Prieto, J. L., Kasen, D., Holoien, T. W. -S., Kollmeier, J. A., Kelson, D. D., Coulter, D. A., Foley, R. J., Kilpatrick, C. D., Siebert, M. R., Madore, B. F., Murguia-Berthier, A., Pan, Y. -C., Prochaska, J. X., Ramirez-Ruiz, E., Rest, A., Adams, C., Alatalo, K., Banados, E., Baughman, J., Bernstein, R. A., Bitsakis, T., Boutsia, K., Bravo, J. R., Di Mille, F., Higgs, C. R., Ji, A. P., Maravelias, G., Marshall, J. L., Placco, V. M., Prieto, G., Wan, Z.
On 2017 August 17, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event GW170817. We report time-series spectroscopy of SSS17a from 11.75 hours until 8.5 days after merger
Externí odkaz:
http://arxiv.org/abs/1710.05432
Autor:
Wessolly M, Stephan-Falkenau S, Streubel A, Werner R, Borchert S, Griff S, Mairinger E, Walter RFH, Bauer T, Eberhardt WEE, Blum TG, Schmid KW, Kollmeier J, Mairinger T, Mairinger FD
Publikováno v:
Cancer Management and Research, Vol Volume 12, Pp 7881-7890 (2020)
Michael Wessolly,1,2,* Susann Stephan-Falkenau,3,* Anna Streubel,3 Robert Werner,3 Sabrina Borchert,1,2 Sergej Griff,3 Elena Mairinger,1 Robert FH Walter,1,4 Torsten Bauer,5 Wilfried EE Eberhardt,4,6 Torsten G Blum,5 Kurt W Schmid,1 Jens Kollmeier,5
Externí odkaz:
https://doaj.org/article/b8824cd3fb03410eba09eeb0be75bde2
