Zobrazeno 1 - 10
of 336
pro vyhledávání: '"Rich, Jeffrey A."'
Autor:
Linden, Sean T., Lai, Thomas, Evans, Aaron S., Armus, Lee, Larson, Kirsten L., Rich, Jeffrey A., U, Vivian, Privon, George C., Inami, Hanae, Song, Yiqing, Bianchin, Marina, Bohn, Thomas, Buiten, Victorine A., Sanchez-Garcia, Maria, Kader, Justin, Lenkic, Laura, Medling, Anne M., Boeker, Torsten, Diaz-Santos, Tanio, Charmandaris, Vassilis, Barcos-Munoz, Loreto, van der Werf, Paul, Stierwalt, Sabrina, Aalto, Susanne, Appleton, Philip, Hayward, Christopher C., Howell, Justin H., Malkan, Matthew A., Mazzarella, Joseph M., Murphy, Eric J., Surace, Jason
We present the results of a James Webb Space Telescope (JWST) NIRCam and NIRSpec investigation into the young massive star cluster (YMC) population of NGC 3256, the most cluster-rich luminous infrared galaxy (LIRG) in the Great Observatories All Sky
Externí odkaz:
http://arxiv.org/abs/2409.16503
Autor:
Buiten, Victorine A., van der Werf, Paul P., Viti, Serena, Armus, Lee, Barr, Andrew G., Barcos-Muñoz, Loreto, Evans, Aaron S., Inami, Hanae, Linden, Sean T., Privon, George C., Song, Yiqing, Rich, Jeffrey A., Aalto, Susanne, Appleton, Philip N., Böker, Torsten, Charmandaris, Vassilis, Diaz-Santos, Tanio, Hayward, Christopher C., Lai, Thomas S. -Y., Medling, Anne M., Ricci, Claudio, U, Vivian
The enormous increase in mid-IR sensitivity and spatial and spectral resolution provided by the JWST spectrographs enables, for the first time, detailed extragalactic studies of molecular vibrational bands. This opens an entirely new window for the s
Externí odkaz:
http://arxiv.org/abs/2312.01945
Autor:
Sextl, Eva, Kudritzki, Rolf-Peter, Burkert, Andreas, Ho, I-Ting, Zahid, H. Jabran, Seibert, Mark, Battisti, Andrew J., Madore, Barry F., Rich, Jeffrey A.
We analyze TYPHOON long slit absorption line spectra of the starburst barred spiral galaxy NGC 1365 obtained with the Progressive Integral Step Method covering an area of 15 square kpc. Applying a population synthesis technique, we determine the spat
Externí odkaz:
http://arxiv.org/abs/2311.01140
Autor:
Spilker, Justin S., Phadke, Kedar A., Aravena, Manuel, Archipley, Melanie, Bayliss, Matthew B., Birkin, Jack E., Bethermin, Matthieu, Burgoyne, James, Cathey, Jared, Chapman, Scott C., Dahle, Hakon, Gonzalez, Anthony H., Gururajan, Gayathri, Hayward, Christopher C., Hezaveh, Yashar D., Hill, Ryley, Hutchison, Taylor A., Kim, Keunho J., Kim, Seonwoo, Law, David, Legin, Ronan, Malkan, Matthew A., Marrone, Daniel P., Murphy, Eric J., Narayanan, Desika, Navarre, Alex, Olivier, Grace M., Rich, Jeffrey A., Rigby, Jane R., Reuter, Cassie, Rhoads, James E., Sharon, Keren, Smith, J. D. T., Solimano, Manuel, Sulzenauer, Nikolaus, Vieira, Joaquin D., Weiss, Axel, Whitaker, Katherine E.
Dust grains absorb half of the radiation emitted by stars throughout the history of the universe, re-emitting this energy at infrared wavelengths. Polycyclic aromatic hydrocarbons (PAHs) are large organic molecules that trace millimeter-size dust gra
Externí odkaz:
http://arxiv.org/abs/2306.03152
Autor:
Alatalo, Katherine, Bitsakis, Theodoros, Lanz, Lauranne, Lacy, Mark, Brown, Michael J. I., French, K. Decker, Ciesla, Laure, Appleton, Philip N., Beaton, Rachael L., Cales, Sabrina L., Crossett, Jacob, Falcón-Barroso, Jesús, Kelson, Daniel D., Kewley, Lisa J., Kriek, Mariska, Medling, Anne M., Mulchaey, John S., Nyland, Kristina, Rich, Jeffrey A., Urry, C. Meg
We investigate the optical and Wide-field Survey Explorer (WISE) colors of "E+A" identified post-starburst galaxies, including a deep analysis of 190 post-starbursts detected in the 2 mu m All Sky Survey Extended Source Catalog. The post-starburst ga
Externí odkaz:
http://hdl.handle.net/10150/624929
http://arizona.openrepository.com/arizona/handle/10150/624929
http://arizona.openrepository.com/arizona/handle/10150/624929
Autor:
Linden, Sean T., Evans, Aaron S., Armus, Lee, Rich, Jeffrey A., Larson, Kirsten L., Lai, Thomas, Privon, George C., U, Vivian, Inami, Hanae, Bohn, Thomas, Song, Yiqing, Barcos-Muñoz, Loreto, Charmandaris, Vassilis, Medling, Anne M., Stierwalt, Sabrina, Diaz-Santos, Tanio, Böker, Torsten, van der Werf, Paul, Aalto, Susanne, Appleton, Philip, Brown, Michael J. I., Hayward, Christopher C., Howell, Justin H., Iwasawa, Kazushi, Kemper, Francisca, Frayer, David T., Law, David, Malkan, Matthew A., Marshall, Jason, Mazzarella, Joseph M., Murphy, Eric J., Sanders, David, Surace, Jason
We present the results of a {\it James Webb Space Telescope} NIRCam investigation into the young massive star cluster (YMC) population in the luminous infrared galaxy VV 114. We identify 374 compact YMC candidates with a $S/N \geq 3$, 5, and 5 at F15
Externí odkaz:
http://arxiv.org/abs/2210.05763
Autor:
Bohn, Thomas, Inami, Hanae, Diaz-Santos, Tanio, Armus, Lee, Linden, Sean T., U, Vivian, Surace, Jason, Larson, Kirsten L., Evans, Aaron S., Hoshioka, Shunshi, Lai, Thomas, Song, Yiqing, Mazzarella, Joseph M., Barcos-Munoz, Loreto, Charmandaris, Vassilis, Howell, Justin H., Medling, Anne M., Privon, George C., Rich, Jeffrey A., Stierwalt, Sabrina, Aalto, Susanne, Boker, Torsten, Brown, Michael J. I., Iwasawa, Kazushi, Malkan, Matthew A., van der Werf, Paul P., Appleton, Philip, Hayward, Christopher C., Kemper, Francisca, Law, David, Marshall, Jason, Murphy, Eric J., Sanders, David
We present James Webb Space Telescope (JWST) imaging of NGC 7469 with the Near-Infrared Camera (NIRCam) and the Mid-InfraRed Instrument (MIRI). NGC 7469 is a nearby, $z=0.01627$, luminous infrared galaxy (LIRG) that hosts both a Seyfert Type-1.5 nucl
Externí odkaz:
http://arxiv.org/abs/2209.04466
Autor:
Evans, Aaron S., Frayer, David, Charmandaris, Vassilis, Armus, Lee, Inami, Hanae, Surace, Jason, Linden, Sean, Soifer, Baruch, Diaz-Santos, Tanio, Larson, Kirsten, Rich, Jeffrey, Song, Yiqing, Barcos-Munoz, Loreto, Mazzarella, Joseph, Privon, George, U, Vivian, Medling, Anne, Boeker, Torsten, Aalto, Susanne, Iwasawa, Kazushi, Howell, Justin, van der Werf, Paul, Appleton, Philip N., Bohn, Thomas, Brown, Michael, Hayward, Christopher, Hoshioka, Shunshi, Kemper, Francisca, Lai, Thomas, Law, David, Malkan, Matthew, Marshall, Jason, Murphy, Eric, Sanders, David, Stierwalt, Sabrina
James Webb Space Telescope (JWST) Mid-InfraRed Instrument (MIRI) images of the luminous infrared (IR) galaxy VV 114 are presented. This redshift ~ 0.020 merger has a western component (VV 114W) rich in optical star clusters and an eastern component (
Externí odkaz:
http://arxiv.org/abs/2208.14507
Autor:
Inami, Hanae, Surace, Jason, Armus, Lee, Evans, Aaron S., Larson, Kirsten L., Barcos-Munoz, Loreto, Stierwalt, Sabrina, Mazzarella, Joseph M., Privon, George C., Song, Yiqing, Linden, Sean, Hayward, Christopher C., Boker, Torsten, U, Vivian, Bohn, Thomas, Charmandaris, Vassilis, Diaz-Santos, Tanio, Howell, Justin H., Lai, Thomas, Medling, Anne M., Rich, Jeffrey A., Aalto, Susanne, Appleton, Philip, Brown, Michael J. I., Hoshioka, Shunshi, Iwasawa, Kazushi, Kemper, Francisca, Law, David, Malkan, Matthew A., Marshall, Jason, Murphy, Eric J., Sanders, David, van der Werf, Paul
We have used the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) to obtain the first spatially resolved, mid-infrared (mid-IR) images of IIZw096, a merging luminous infrared galaxy (LIRG) at $z = 0.036$. Previous observations
Externí odkaz:
http://arxiv.org/abs/2208.10647
Autor:
Ni, Yuan Qi, Moon, Dae-Sik, Drout, Maria R., Polin, Abigail, Sand, David J., GonzÁlez-GaitÁn, Santiago, Kim, Sang Chul, Lee, Youngdae, Park, Hong Soo, Howell, D. Andrew, Nugent, Peter E., Piro, Anthony L., Brown, Peter J., Galbany, LluÍs, Burke, Jamison, Hiramatsu, Daichi, Hosseinzadeh, Griffin, Valenti, Stefano, Afsariardchi, Niloufar, Andrews, Jennifer E., Antoniadis, John, Beaton, Rachael L., Bostroem, K. Azalee, Carlberg, Raymond G., Cenko, S. Bradley, Cha, Sang-Mok, Dong, Yize, Gal-Yam, Avishay, Haislip, Joshua, Holoien, Thomas W. -S., Johnson, Sean D., Kouprianov, Vladimir, Lee, Yongseok, Matzner, Christopher D., Morrell, Nidia, Mccully, Curtis, Pignata, Giuliano, Reichart, Daniel E., Rich, Jeffrey, Ryder, Stuart D., Smith, Nathan, Wyatt, Samuel, Yang, Sheng
SN~2018aoz is a Type Ia SN with a $B$-band plateau and excess emission in the infant-phase light curves $\lesssim$ 1 day after first light, evidencing an over-density of surface iron-peak elements as shown in our previous study. Here, we advance the
Externí odkaz:
http://arxiv.org/abs/2206.12437