%0 Generic %1 wiegert2015changes %A Wiegert, Theresa %A Irwin, Judith %A Miskolczi, Arpad %A Schmidt, Philip %A Mora, Silvia Carolina %A Damas-Segovia, Ancor %A Stein, Yelena %A English, Jayanne %A Rand, Richard J. %A Santistevan, Isaiah %A Walterbos, Rene %A Krause, Marita %A Beck, Rainer %A Dettmar, Ralf-Juergen %A Kepley, Amanda %A Wezgowiec, Marek %A Wang, Q. Daniel %A Heald, George %A Li, Jiangtao %A MacGregor, Stephen %A Johnson, Megan %A Strong, A. W. %A DeSouza, Amanda %A Porter, Troy A. %D 2015 %K emission fields galaxies magnetic radio spiral %R 10.1088/0004-6256/150/3/81 %T CHANG-ES IV: Radio continuum emission of 35 edge-on galaxies observed with the Karl G. Jansky Very Large Array in D-configuration, Data Release 1 %U http://arxiv.org/abs/1508.05153 %X We present the first part of the observations made for the Continuum Halos in Nearby Galaxies, an EVLA Survey (CHANG-ES) project. The aim of the CHANG-ES project is to study and characterize the nature of radio halos, their prevalence as well as their magnetic fields, and the cosmic rays illuminating these fields. This paper reports observations with the compact D configuration of the Karl G. Jansky Very Large Array (VLA) for the sample of 35 nearby edge-on galaxies of CHANG-ES. With the new wide bandwidth capabilities of the VLA, an unprecedented sensitivity was achieved for all polarization products. The beam resolution is an average of 9.6" and 36" with noise levels reaching approximately 6 and 30 microJy per beam for C- and L-bands, respectively (robust weighting). We present intensity maps in these two frequency bands (C and L), with different weightings, as well as spectral index maps, polarization maps, and new measurements of star formation rates (SFRs). The data products described herein are available to the public in the CHANG-ES data release available at www.queensu.ca/changes. We also present evidence of a trend among galaxies with larger halos having higher SFR surface density, and we show, for the first time, a radio continuum image of the median galaxy, taking advantage of the collective signal-to-noise ratio of 30 of our galaxies. This image shows clearly that a typical spiral galaxy is surrounded by a halo of magnetic fields and cosmic rays.

@misc{wiegert2015changes, abstract = {We present the first part of the observations made for the Continuum Halos in Nearby Galaxies, an EVLA Survey (CHANG-ES) project. The aim of the CHANG-ES project is to study and characterize the nature of radio halos, their prevalence as well as their magnetic fields, and the cosmic rays illuminating these fields. This paper reports observations with the compact D configuration of the Karl G. Jansky Very Large Array (VLA) for the sample of 35 nearby edge-on galaxies of CHANG-ES. With the new wide bandwidth capabilities of the VLA, an unprecedented sensitivity was achieved for all polarization products. The beam resolution is an average of 9.6" and 36" with noise levels reaching approximately 6 and 30 microJy per beam for C- and L-bands, respectively (robust weighting). We present intensity maps in these two frequency bands (C and L), with different weightings, as well as spectral index maps, polarization maps, and new measurements of star formation rates (SFRs). The data products described herein are available to the public in the CHANG-ES data release available at www.queensu.ca/changes. We also present evidence of a trend among galaxies with larger halos having higher SFR surface density, and we show, for the first time, a radio continuum image of the median galaxy, taking advantage of the collective signal-to-noise ratio of 30 of our galaxies. This image shows clearly that a typical spiral galaxy is surrounded by a halo of magnetic fields and cosmic rays.}, added-at = {2015-08-24T09:55:46.000+0200}, author = {Wiegert, Theresa and Irwin, Judith and Miskolczi, Arpad and Schmidt, Philip and Mora, Silvia Carolina and Damas-Segovia, Ancor and Stein, Yelena and English, Jayanne and Rand, Richard J. and Santistevan, Isaiah and Walterbos, Rene and Krause, Marita and Beck, Rainer and Dettmar, Ralf-Juergen and Kepley, Amanda and Wezgowiec, Marek and Wang, Q. Daniel and Heald, George and Li, Jiangtao and MacGregor, Stephen and Johnson, Megan and Strong, A. W. and DeSouza, Amanda and Porter, Troy A.}, biburl = {https://www.bibsonomy.org/bibtex/2459ffae824439328aaf74e8b38a271f8/miki}, description = {[1508.05153] CHANG-ES IV: Radio continuum emission of 35 edge-on galaxies observed with the Karl G. Jansky Very Large Array in D-configuration, Data Release 1}, doi = {10.1088/0004-6256/150/3/81}, interhash = {3e39b9ecaede95bad90c6fb7315c90dd}, intrahash = {459ffae824439328aaf74e8b38a271f8}, keywords = {emission fields galaxies magnetic radio spiral}, note = {cite arxiv:1508.05153Comment: 70 pages, of which 35 pages present the data of each galaxy}, timestamp = {2015-08-24T09:55:46.000+0200}, title = {CHANG-ES IV: Radio continuum emission of 35 edge-on galaxies observed with the Karl G. Jansky Very Large Array in D-configuration, Data Release 1}, url = {http://arxiv.org/abs/1508.05153}, year = 2015 }