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We present 21 cm observations of Arp 158. We have performed a study of the neutral hydrogen (HI) to help us understand the overall formation and evolution of this system. This is a disturbed system with distinct optical knots connected by a…

We present HI 21 cm spectroscopy from the GBT for the host galaxies of 31 nearby AGNs with direct M$_{\textrm{BH}}$ measurements from reverberation mapping. These are the first published HI detections for 12 galaxies, and the spectral…

Astrophysics of Galaxies · Physics 2019-07-31 Justin H. Robinson , Misty C. Bentz , Megan C. Johnson , Hélène M. Courtois , Benjamin Ou-Yang

We have carried out CCD photometry in the Cousins B and R bands of 21 dwarf galaxies in and around the M101 group. Eleven are members and suspected members of the group and ten are field galaxies in the projected vicinity of the group. We…

Astrophysics · Physics 2009-10-31 T. Bremnes , B. Binggeli , P. Prugniel

We have used dedicated 0.7m telescopes in California and Israel to image the halos of ~200 galaxies in the Local Volume to 29 mag/sq arcsec, the sample mainly drawn from the 2MASS Large Galaxy Atlas (LGA). We supplement the LGA sample with…

SN2017egm is the closest (z=0.03) H-poor superluminous supernova (SLSN-I) detected to date, and a rare example of an SLSN-I in a massive and metal-rich galaxy. Here we present the HST UV & optical spectra covering (1000 - 5500)A taken at +3…

High Energy Astrophysical Phenomena · Physics 2018-05-23 Lin Yan , D. A. Perley , A. De Cia , R. Quimby , R. Lunnan , Kate H. R. Rubin , P. J. Brown

We are undertaking a large, wide-field survey of nearby groups and poor clusters. The main goals are identifying and characterizing the properties of low-surface-brightness dwarf galaxies and determining the galaxy luminosity function for…

Astrophysics · Physics 2007-05-23 C. Mendes de Oliveira , E. R. Carrasco , L. Infante , M. Bolte

Giant low surface brightness galaxies (gLSBs) are galaxies with extremely extended, faint, optical disks over 50 kpc in radius and have high total masses which can reach 10^12 solar masses. The existence of such galaxies is problematic for…

We present the design and methods of the COS-Halos survey, a systematic investigation of the gaseous halos of 44 z = 0.15-0.35 galaxies using background QSOs observed with the Cosmic Origins Spectrograph aboard the Hubble Space Telescope.…

We present near infrared ISAAC VLT observations of nine (0.01<z<0.06) Active Galactic Nuclei selected from the Hamburg/ESO Survey and the Veron-Cetty & Veron catalog. Hydrogen recombination lines Pa$\alpha$ and Br$\gamma$ are observed in…

Astrophysics · Physics 2009-11-11 S. Fischer , C. Iserlohe , J. Zuther , T. Bertram , C. Straubmeier , R. Schoedel , A. Eckart

We use Hyper Suprime-Cam on the Subaru Telescope to investigate the structural and photometric properties of early-type dwarf galaxies and young stellar systems at the center of the M81 Group. We have mapped resolved stars to $\sim2$…

Astrophysics of Galaxies · Physics 2019-11-06 Sakurako Okamoto , Nobuo Arimoto , Annette M. N. Ferguson , Mike J. Irwin , Edouard J. Bernard , Yousuke Utsumi

[abridged] We present observations of the dust and atomic gas phase in seven dwarf irregular galaxies of the M81 group from the SINGS and THINGS surveys. The Spitzer observations provide a first glimpse of the nature of the non-atomic ISM…

The Arecibo Galaxy Environment Survey (AGES) is one of several HI surveys utilising the new Arecibo L-band Feed Array (ALFA) fitted to the 305m radio telescope at Arecibo. The survey is specifically designed to investigate various galactic…

The recently published GALFA-HI Compact Cloud Catalogue lists 20 neutral hydrogen clouds that might pinpoint previously undiscovered high-latitude dwarf galaxies. Detection of an associated gamma-ray dark matter signal could provide a route…

High Energy Astrophysical Phenomena · Physics 2015-06-15 N. Mirabal

From the first published z > 3 survey of 21-cm absorption within the hosts of radio galaxies and quasars, we found an apparent dearth of cool neutral gas at high redshift. From a detailed analysis of the photometry, each object is found to…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 S. J. Curran , M. T. Whiting

We have obtained deep multi-object optical spectra of 49 HII regions in the outer disk of the spiral galaxy M83 (=NGC 5236) with the FORS2 spectrograph at the Very Large Telescope. The targets span the range in galactocentric distance…

Astrophysics of Galaxies · Physics 2011-02-11 Fabio Bresolin , Emma Ryan-Weber , Robert C. Kennicutt , Quinton Goddard

We have combined observations of Galactic high-velocity HI from two surveys: a very sensitive survey from the Green Bank 140ft Telescope with limited sky coverage, and the less sensitive but complete Galactic All Sky Survey from the 64m…

Astrophysics of Galaxies · Physics 2017-01-18 Vanessa A. Moss , Felix J. Lockman , Naomi M. McClure-Griffiths

We report results from a study of the HI content and stellar properties of nearby galaxies detected by the Arecibo Legacy Fast ALFA blind 21-cm line survey and the Sloan Digital Sky Survey in two declination strips covering a total area of…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 M. C. Toribio , J. M. Solanes , R. Giovanelli , M. P. Haynes , K. L. Masters

Neutral hydrogen (HI) has been detected in the Local Group dwarf spheroidal galaxy Sculptor with the 64 m Parkes single dish and mapped with the Australia Telescope synthesis array. Most of the detected HI is in two clouds \sim 15'-20' away…

Astrophysics · Physics 2009-10-30 Claude Carignan , Sylvie Beaulieu , Stephanie Cote , Serge Demers , Mario Mateo

We present the photometric and spectroscopic results of a survey done in a wide-field area of nearby groups and poor clusters. The main goals are identifying and characterizing the properties of low-surface-brightness dwarf galaxies and…

Astrophysics · Physics 2007-05-23 E. R. Carrasco , C. Mendes de Oliveira , L. Infante

We have carried out a blind HI survey using the Westerbork Synthesis Radio Telescope to make an inventory of objects with small HI masses (between 10^6 and 10^8 Msol) and to constrain the low-mass end of the HI mass function. The survey has…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 K. Kovac , T. A. Oosterloo , J. M. van der Hulst
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