CROMOS: A cryogenic near-infrared, multi-object spectrometer for the VLT by Genzel, R, Hofmann, R, Tomono, D, Thatte, N, Eisenhauer, F, Lehnert, M, Tecza, M, Bender, R

An atlas of Hubble space telescope spectra and images of nearby spiral galaxies by Hughes, M, Alonso-Herrero, A, Axon, D, Scarlata, C, Atkinson, J, Batcheldor, D, Binney, J, Capetti, A, Carollo, C, Dressel, L, Gerssen, J, Macchetto, D, Maciejewski, W, Marconi, A, Merrifield, M, Ruiz, M, Sparks, W, Stiavelli, M, Tsvetanov, Z, Van der Marel, R

“…Dust obscuration can be significant at optical wavelengths, and so we also combine the STIS images with archival Near-Infrared Camera and Multi-Object Spectrometer H-band images to produce color maps to investigate the morphology of gas and dust in the central regions. …”

Near-infrared properties of i-drop galaxies in the Hubble Ultra Deep Field by Stanway, E, McMahon, R, Bunker, A

“…We analyse near-infrared Hubble Space Telescope (HST)/Near-Infrared Camera and Multi-Object Spectrometer F110W (J) and F160W (H) band photometry of a sample of 27 i′-drop candidate z ≃ 6 galaxies in the central region of the HST/Advanced Camera for Surveys Ultra Deep Field. …”

Nuclear properties of nearby spiral galaxies from Hubble Space Telescope NICMOS imaging and STIS spectroscopy by Hughes, M, Axon, D, Atkinson, J, Alonso-Herrero, A, Scarlata, C, Marconi, A, Batcheldor, D, Binney, J, Capetti, A, Carollo, C, Dressel, L, Gerssen, J, Macchetto, D, Maciejewski, W, Merrifield, M, Ruiz, M, Sparks, W, Stiavelli, M, Tsvetanov, Z

“…We investigate the central regions of 23 spiral galaxies using Space Telescope Imaging Spectrograph (STIS) spectroscopy and archival Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) imaging. The sample is taken from our program to determine the masses of central massive black holes (MBHs) in 54 nearby spiral galaxies. …”

ALMA observations of Ly α BLOB 1: halo substructure illuminated from within by Geach, J, Narayanan, D, Matsuda, Y, Hayes, M, Mas-Ribas, L, Dijkstra, M, Steidel, C, Chapman, S, Feldmann, R, Avison, A, Agertz, O, Ao, Y, Birkinshaw, M, Bremer, M, Clements, D, Dannerbauer, H, Farrah, D, Harrison, C, Kubo, M, Michałowski, M, Scott, D, Smith, D, Spaans, M, Simpson, J, Swinbank, A, Taniguchi, Y, Werf, P, Verma, A, Yamada, T

“…One of these companions is spectroscopically confirmed with the Keck Multi-Object Spectrometer For Infra-Red Exploration to lie within 20 projected kpc and 250 km s -1 of one of the ALMA components. …”

NEAR-INFRARED TRANSIT PHOTOMETRY OF THE EXOPLANET HD 149026b by Carter, Joshua Adam, Winn, Joshua Nathan, Gilliland, Ronald L., Holman, Matthew J.

“…We present observations of four transits with the Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) on the Hubble Space Telescope within a wavelength range of 1.1-2.0 μm. …”
Get full text
Get full text

Herschel observations of a z∼ 2 stellar mass selected galaxy sample drawn from the GOODS NICMOS Survey by Hilton, M, Conselice, C, Roseboom, I, Burgarella, D, Buat, V, Berta, S, Béthermin, M, Bock, J, Chapman, S, Clements, D, Conley, A, Conversi, L, Cooray, A, Farrah, D, Ibar, E, Magdis, G, Magnelli, B, Marsden, G, Nordon, R, Oliver, S, Page, M, Popesso, P, Pozzi, F, Schulz, B, Scott, D

“…We present a study of the far-infrared (IR) properties of a stellar mass selected sample of 1.5 < z < 3 galaxies with log(M */M ⊙) > 9.5 drawn from the Great Observatories Origins Deep Survey (GOODS) Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Survey (GNS), the deepest H-band Hubble Space Telescope survey of its type prior to the installation of Wide Field Camera 3 (WFC3). …”

PREDICTING FUTURE SPACE NEAR-IR GRISM SURVEYS USING THE WFC3 INFRARED SPECTROSCOPIC PARALLELS SURVEY by Colbert, J, Teplitz, H, Atek, H, Bunker, A, Rafelski, M, Ross, N, Scarlata, C, Bedregal, A, Dominguez, A, Dressler, A, Henry, A, Malkan, M, Martin, C, Masters, D, McCarthy, P, Siana, B

“…Our Hα luminosity function contains a comparable number density of faint line emitters to that found by the Near IR Camera and Multi-Object Spectrometer near-infrared grism surveys, but significantly fewer (factors of 3-4 less) high-luminosity emitters. …”