Dynamical Hypermassive Black Hole Masses
We will use STIS spectra to derive the masses of 5 hypermassive black holes (HMBHs). From the observed scaling relations defined by less massive spheroids, these objects are expected to reside at the nuclei of host galaxies with stellar velocity dispersions greater than 320 km/s. These 5 targets have confirmed regular gas distributions on the scales of the black hole sphere of influence. It is essential that the sphere of influence is resolved for accurate determinations of black hole mass (0.1"). These scales cannot be effectively observed from the ground. Only two HMBHs have had their masses modeled so far; it is impossible to draw any general conclusions about the connections between HMBH mass and their massive host galaxies. With these 5 targets we will determine whether these HMBHs deviate from the scaling relations defined by less massive spheroids. A larger sample will allow us to firmly anchor the high mass end of the correlation between black hole mass and stellar velocity dispersion, and other scaling relations. Therefore we are also conducting a SNAPSHOT program with which we expect to detect a further 24 HMBH candidates for STIS observation in future Cycles. At the completion of this project we will have populated the high mass end of the scaling relations with the sample sizes enjoyed by less massive spheroids.
The 25 orbits are split equally across 5 targets. Each target is a (giant) Elliptical galaxy with a large velocity dispersion. In each orbit we will use different slit positons to map a 2D region at the nuclear region of each target. We are targeting regular gas disks surrounding the central Black Hole and therefore will cover the H-alpha region of the spectrum.
We use 3 visits per target. At the central slit position we require maximum spatial resolution, so we will use the 52x0.1 arcsec slit and G750M grating. In the first visit for each target (3 orbits) the central 0.1 slit will be flanked by two offset 0.2 slit observations (1 orbit per slit position).
At the two off nuclear slit positions, as the line brightnesses drop off rapidly, we will use the wider 52x0.2 arcsec slit in order to provide the best compromise between resolution and throughput. The two subsequent visits will acquire the nucleus of the target and use the 0.1 slit. However, the slits will be orientated +/- ~60 degrees from the first visit. This technique ensures one slit position will be close to the disk position angle.
We will be using the longest possible exposures, so all will be CR-SPLIT. In addition, we will make one non-integer dither along the slit, by 4.5 pixels, in order to enable a proper rejection of hot pixels and to deal with the possible undulation issue due to undersampling.
To minimize the overheads per target/orbit/visit our observing strategy is as follows:
1) GS-ACQ
2) ACQ
3) Offset to slit position OFF1
4) 4 exposures with 52x0.2 (2 crsplits and 1 dither).
1 orbit used.
5) GS-ReACQ
6) Peak-up on nucleus
7) 4 exposures with 52x0.1
2 orbits used.
8) GS-RAc
9) 4 exposures with 52x0.2
3 orbits used
10) GS-ACQ
11) ACQ
12) Peak-up
13) 4 exposures with 52x0.1
4 orbits used
14) GS-ACQ
15) ACQ
16) Peak-up
17) 4 exposures with 52x0.1
5 orbits used.
UNRESOLVED STELLAR POPULATIONS AND GALAXY STRUCTURE
12
false
0.0
0.0
false
false
false
false
false
SUPPORTED
GALAXY
ELLIPTICAL
NUCLEUS
This object was generated by the targetselector and retrieved from the NED database.
J2000
12 54 35.9064
-12 34 7.54
J2000
GALAXY
ELLIPTICAL
NUCLEUS
This object was generated by the targetselector and retrieved from the NED database.
J2000
23 38 29.3056
+27 01 53.02
J2000
GALAXY
ELLIPTICAL
NUCLEUS
This object was generated by the targetselector and retrieved from the NED database.
J2000
12 43 40.0001
+11 33 8.24
J2000
GALAXY
ELLIPTICAL
NUCLEUS
This object was generated by the targetselector and retrieved from the NED database.
J2000
03 38 28.9748
-35 27 2.49
J2000
GALAXY
ELLIPTICAL
NUCLEUS
This object was generated by the targetselector and retrieved from the NED database.
J2000
02 23 11.5149
+42 59 31.25
J2000
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
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STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
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STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6581
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
STIS/CCD
Spectroscopic
No
No
G750M
6768
POS-TARG
DITHER
0.35546
LINE
false
false
3
90.0
STIS-ALONG-SLIT
1
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