0
Assigned ID: 1534
----- Attempting Submission 1 (Wed Apr 07 09:43:33 GMT 2021) -----
HST Phase I Proposal 1534 successfully submitted.
Receipt: # 1534-1
----- Attempting Submission 2 (Wed Apr 07 13:46:37 GMT 2021) -----
HST Phase I Proposal 1534 successfully submitted.
Receipt: # 1534-2
----- Attempting Submission 3 (Wed Apr 07 14:23:09 GMT 2021) -----
HST Phase I Proposal 1534 successfully submitted.
Receipt: # 1534-3
----- Attempting Submission 4 (Thu Apr 08 08:51:21 GMT 2021) -----
0
----- Attempting Submission 1 (Fri Jul 23 06:34:05 GMT 2021) -----
----- Attempting Submission 2 (Wed Sep 08 15:35:41 GMT 2021) -----
----- Attempting Submission 3 (Tue Sep 28 20:02:42 GMT 2021) -----
Globular cluster systems of ultra-diffuse galaxies in low density environments
As part of a systematic deep imaging survey with CFHT+MegaCam, 96 ultra-diffuse galaxies (UDGs) in low to medium density fields have been identified. This UDG dataset is among the largest sample of this type of galaxy outside of galaxy clusters. Thanks to the high image quality of MegaCam, part of their globular clusters (GCs) population can already be detected and two populations of UDGs have been identified: one with an excess number and the other with a similar number of GCs compared to normal dwarfs. This GC candidate selection method was proven reliable for a UDG in the NGC 5846 group, using HST data that sampled most of the GCLF. This most extreme UDG hosts 40 GCs and a vast dark matter (DM) halo as massive as the Large Magellanic Cloud, but is less luminous by a factor of 50, i.e., is too massive for its stellar mass. However, VLT+MUSE spectroscopy suggests that based on the stellar velocity dispersion, this UDG hosts a rather small DM halo. Many of these properties are similar to those of the UDGs NGC1052-DF2 and -DF4 which, however, appear to have over-luminous GCs. This reveals a tension between the two different paths to measure the DM mass of a dwarf. We propose a SNAPSHOT program of 70 UDGs in non-cluster environments, employing two-band ACS imaging to trace the full population of GCs 3 magnitudes below the peak of the GCLF and give us an accurate estimate of the total number of GCs. We will characterize their GC systems and test whether some UDGs host an exceptionally large number of GCs, but with a regular GCLF, or contain a population consisting of only over-luminous GCs. Both cases pose a conundrum for our undertanding of GC and galaxy formation.
SNAPSHOT program for F606W/F814W imaging of ultra-diffuse galaxies. Limited to 4 exposures of equal length for a single orbit requested/allocated per galaxy. Use of small DITHER LINE as we do not require filling in the chip gap, but we do need two exposures in each filter to facilitate CR and hot pixel removal. We have created a DITHER-LINE of 7.5 pixels x 6.5 pixels, or spacing 0.504" at an angle of 42.11 degrees.
Data to be used to obtain magnitudes and colors of most (marginally-resolved) globular cluster candidates in sample galaxies.
We have centered each galaxy on aperture WFC1 in order to avoid chip gap running through each galaxy. As this is a SNAP program, ORIENT values are not specified. No bright objects have been found to be a danger for the health and safety of the detector.
Reduced Gyro mode: We do not expect any significant complications if less than 3 gyros are available for the observations, reducing the effective time available for observations.
Schedulability: We have adopted a 46 minute visit length to optimize exposure times and schedulability.
The team consists of several junior and senior members of the MATLAS collaboration who have ample experience with:
- HST imaging data (e.g., Francine Marleau, Sungsoon Lim, Patrick Durrell, Oliver Mueller)
- dwarf galaxies (e.g., Pierre-Alain Duc, Oliver Mueller, Sanjaya Paudel, Ruben Sanchez-Janssen, Rebecca Habas)
- PSF and aperture photometry (e.g. Oliver Mueller, Sungsoon Lim, Patrick Durrell)
- globular clusters (e.g., Patrick Durrell, Ruben Sanchez-Janssen, Sungsoon Lim)
and have proven to have an excellent publication track on the topic of dwarf/ultra-diffuse galaxies (e.g., van der Burg et al. 2015, 2016, Mueller et al. 2018, Lim et al. 2018, 2020, Emsellem et al. 2019, Fensch et al. 2019, Habas et al. 2020, Mueller et al. 2020, Mueller et al. 2021). The project will be led by Prof. Francine Marleau who is based at the Institute of Astro- and Particle Physics, at the University of Innsbruck. The data reduction will be accomplished in a timely manner and the results will be published in a renowned journal like ApJ.
Galaxies
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "27"
:si-bright-earth-limb-angle 20.0
:data-volume 1136896
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16711
:visit-id "70"
:obset-id "70"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16711
:visit-id "70"
:orbit-number 1
:pcs-time 383
:si-vis-utilization 2397
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3200
:pcs-gap 0
)
true
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