Data

HI absorption associated to Norma's brightest cluster galaxy

Commonwealth Scientific and Industrial Research Organisation
Saraf, Manasvee ; Wong, Ivy ; Cortese, Luca ; Koribalski, Baerbel
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.25919/1842-k647&rft.title=HI absorption associated to Norma's brightest cluster galaxy&rft.identifier=https://doi.org/10.25919/1842-k647&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Continuum and HI spectral cubes and multi-frequency synthesis continuum map towards the Norma cluster's brightest cluster galaxy, ESO137-G006. Cubes contain HI flux as a function of position and velocity. HI absorption has been detected to be associated to ESO137-G006.Telescope: The Australian Telescope Compact Array (ATCA)Centre RA: 16:15:04Centre Dec: -60:54:26Radius of cubes: 1 arcminRadius of continuum map: 0.5 degSynthesised Beam: 9 arcsec by 7 arcsec at 31 degreesPixel Size: 2 arcsecRMS noise: 9 mJy/beamFrequency: 1396 MHzVelocity Resolution: 6.6 km/sDetection centre: 5460 km/sDetection width: 192 km/sSpectral noise: 9 mJyFor more detailed information refer to Saraf, M et al 2022 (submitted to MNRAS)Lineage: The data has been obtained from the ATOA, from ATCA Project C2891. Data is observed in the ATCA 6A configuration using a 64-MHz bandwidth. We only processed pointings 12, 13, 14, 17, 18, 19 and 23 to make the cubes and maps.&rft.creator=Saraf, Manasvee &rft.creator=Wong, Ivy &rft.creator=Cortese, Luca &rft.creator=Koribalski, Baerbel &rft.date=2022&rft.edition=v2&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO, International Centre for Radio Astronomy Research, University of Western Australia 2022.&rft_subject=radio lines: galaxies -- galaxies: elliptical and lenticular&rft_subject=cD -- galaxies: individual: ESO137-G006 -- galaxies: clusters: individual: Norma cluster (ACO 3627)&rft_subject=Cosmology and extragalactic astronomy&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft_subject=Astronomical sciences not elsewhere classified&rft.type=dataset&rft.language=English Access the data

Licence & Rights:

Open Licence view details
CC-BY

Creative Commons Attribution 4.0 International Licence
https://creativecommons.org/licenses/by/4.0/

Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO, International Centre for Radio Astronomy Research, University of Western Australia 2022.

Access:

Open view details

Accessible for free

Contact Information



Full description

Continuum and HI spectral cubes and multi-frequency synthesis continuum map towards the Norma cluster's brightest cluster galaxy, ESO137-G006. Cubes contain HI flux as a function of position and velocity. HI absorption has been detected to be associated to ESO137-G006.

Telescope: The Australian Telescope Compact Array (ATCA)
Centre RA: 16:15:04
Centre Dec: -60:54:26
Radius of cubes: 1 arcmin
Radius of continuum map: 0.5 deg
Synthesised Beam: 9 arcsec by 7 arcsec at 31 degrees
Pixel Size: 2 arcsec
RMS noise: 9 mJy/beam
Frequency: 1396 MHz
Velocity Resolution: 6.6 km/s
Detection centre: 5460 km/s
Detection width: 192 km/s
Spectral noise: 9 mJy

For more detailed information refer to Saraf, M et al 2022 (submitted to MNRAS)
Lineage: The data has been obtained from the ATOA, from ATCA Project C2891. Data is observed in the ATCA 6A configuration using a 64-MHz bandwidth. We only processed pointings 12, 13, 14, 17, 18, 19 and 23 to make the cubes and maps.

Available: 2022-12-13

Data time period: 2013-10-22 to 2022-04-29

This dataset is part of a larger collection

Click to explore relationships graph
Identifiers
ACN 633 798 857