Accepted Cycle 11 Observing Proposals

NORMAL GALAXIES DIFFUSE EMISSION & SURVEYS

Proposal Number	Subject Category	PI Name	Title
11610210	NORMAL GALAXIES: DIFFUSE EMISSION	Wang	Mapping out the hot gas outflow from the M31 bulge
11610278	NORMAL GALAXIES: DIFFUSE EMISSION	Swartz	X-raying Circumnuclear Star Formation and Feedback in Nearby Normal Galaxies
11610479	NORMAL GALAXIES: DIFFUSE EMISSION	Trinchieri	Seyfert's Sextet: an evolved Stephan's Quintet
11610596	NORMAL GALAXIES: DIFFUSE EMISSION	BUOTE	Snapshots of Isolated Elliptical Galaxies
11610615	NORMAL GALAXIES: DIFFUSE EMISSION	Irwin	Peering Into the Bondi Radius of the Supermassive Black Hole of NGC3115
11620024	NORMAL GALAXIES: X-RAY POPULATIONS	Murray	Black Hole X-ray Novae in M31
11620048	NORMAL GALAXIES: X-RAY POPULATIONS	Garmire	Are the Observed Submm Flares Related to the X-ray/NIR Flares in Sgr A*?
11620101	NORMAL GALAXIES: X-RAY POPULATIONS	Fabbiano	Constraining the transient LMXB population
11620107	NORMAL GALAXIES: X-RAY POPULATIONS	Kaaret	X-Rays from Blue Compact Dwarf Galaxies
11620112	NORMAL GALAXIES: X-RAY POPULATIONS	Fabbiano	The ringed galaxy NGC1291
11620243	NORMAL GALAXIES: X-RAY POPULATIONS	Maccarone	A new look at the X-ray binary richest galaxy
11620280	NORMAL GALAXIES: X-RAY POPULATIONS	Garcia	Monitoring M31 for BHXNe
11620296	NORMAL GALAXIES: X-RAY POPULATIONS	Rappaport	Search for the Most Luminous ULXs in Collisional Ring Galaxies
11620601	NORMAL GALAXIES: X-RAY POPULATIONS	Prestwich	Ultra-Luminous x-Ray Sources in the Most Metal-Poor Galaxies
11620675	NORMAL GALAXIES: X-RAY POPULATIONS	Clarkson	The Deepest Stellar X-ray/optical Census of the Bulge
11620883	NORMAL GALAXIES: X-RAY POPULATIONS	van den Berg	Studying binary evolution in the oldest open clusters: Collinder 261
11620895	NORMAL GALAXIES: X-RAY POPULATIONS	Kundu	Low Mass X-ray Binaries in Spiral Galaxies
11620915	NORMAL GALAXIES: X-RAY POPULATIONS	Gallo	Accretion onto nuclear black holes in early type galaxies: comparing field vs. clusters

Subject Category: NORMAL GALAXIES: DIFFUSE EMISSION

Proposal Number: 11610210

Title: Mapping out the hot gas outflow from the M31 bulge

PI Name: Q. Daniel Wang

The hot gas outflow from the galactic bulge of M31 was discovered recently, which is driven primarily by Type Ia SNe. To quantify the morphological, thermal, and dynamical properties of this outflow along the minor axis of the galaxy, we propose four ACIS observations to obtain X-ray data with substantially improved spatial resolution, sensitivity, and field coverage. We will map out the overall X-ray morphology and substructure of the outflow, characterize its spectral properties, and distinguish X-ray emission and/or absorption features caused by spiral arms. The results will test our understanding of the galactic bulge energy and mass feedback and will provide badly-needed insights into similar phenomena observed in the Milky Way and other galaxies.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
00:43:25.60	+41:08:21.40	M31 bulge off-field 1	ACIS-I	NONE	60
00:44:03.10	+41:01:15.90	M31 bulge off-field 2	ACIS-I	NONE	20

Subject Category: NORMAL GALAXIES: DIFFUSE EMISSION

Proposal Number: 11610278

Title: X-raying Circumnuclear Star Formation and Feedback in Nearby Normal Galaxies

PI Name: Douglas Swartz

We propose an ACIS-S imaging observation of the barred late-type spiral galaxy NGC 2903. Our primary scientific objective is to investigate the star-forming circumnuclear ring and related structures. We will investigate the effects of star formation on the distribution of gas in this ring and on accretion onto any central massive object. We will construct maps of the distribution of hot gas and compare these to the cold gas, warm gas, and stellar morphologies. We will determine whether the hot gas is confined to the disk or is being expelled in galactic outflows, determine the physical properties of the gas (and point sources), and estimate the role of star formation and associated feedback in impeding or enhancing gas accretion onto any central object.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
09:32:10.10	+21:30:03.00	NGC 2903	ACIS-S	NONE	95

Subject Category: NORMAL GALAXIES: DIFFUSE EMISSION

Proposal Number: 11610479

Title: Seyfert's Sextet: an evolved Stephan's Quintet

PI Name: Ginevra Trinchieri

In the context of galaxy structure evolution, groups are expected to become more X-ray luminous as they grow older. Seyfert's Sextet is a spectacular example of a compact group unambiguously in an advanced stage of coalescence, and as such is expected to be X-ray luminous. Although it shares many characteristics with Stephan's Quintet, it is more evolved, has twice as much light in a diffuse halo, yet its X-ray luminosity is significantly smaller. We aim at studying its X-ray properties to better understand its place in a compact group evolutionary scheme. The biggest mystery involves the low gas fraction. Is there an extended low surface brightness X-ray halo that earlier ROSAT observations could not see? How much gas has fallen into component nuclei generating AGN activity?

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
15:59:11.90	+20:45:31.00	HCG 79	ACIS-S	NONE	70

Subject Category: NORMAL GALAXIES: DIFFUSE EMISSION

Proposal Number: 11610596

Title: Snapshots of Isolated Elliptical Galaxies

PI Name: DAVID BUOTE

The properties of dark matter halos on galactic scales remain a largely untapped resource for cosmological studies. X-ray observations offer potentially the most promising means to study dark matter in isolated elliptical galaxies, but there is presently a lack of known suitable candidates for study. Therefore, we propose a snapshot survey of 12 systems to identify isolated elliptical galaxies with X-ray properties similar to the best examples currently known. Deep follow-up exposures with XMM and Chandra of promising targets will then be sought for detailed analysis of their dark matter distributions.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
02:31:09.80	+29:35:19.50	NGC 953	ACIS-S	NONE	7.5
03:01:30.40	+37:45:57.60	IC 278	ACIS-S	NONE	7.5
02:50:59.70	+37:27:59.90	UGC 02328	ACIS-S	NONE	7.5
20:56:56.60	+06:49:03.70	PGC 65766	ACIS-S	NONE	7.5
09:56:47.90	-65:37:33.30	ESO092-001	ACIS-S	NONE	7.5
01:11:35.90	+49:07:16.30	UGC 00746	ACIS-S	NONE	7.5

Subject Category: NORMAL GALAXIES: DIFFUSE EMISSION

Proposal Number: 11610615

Title: Peering Into the Bondi Radius of the Supermassive Black Hole of NGC3115

PI Name: Jimmy Irwin

We propose a 125 ksec observation of the hot gas around the supermassive black hole at the center of the S0 galaxy NGC3115 to confirm that the size of the Bondi radius is large enough to be resolved by Chandra in future deeper observations. We also seek to confirm that the temperature of the gas rises within the Bondi radius, as predicted by radiative inefficient accretion models. If confirmed, NGC3115 will represent the *only* opportunity to perform a detailed test of inefficient accretion flow theory in the Chandra era and the foreseeable future, and deeper Chandra observations will be proposed to map rho(R) and T(R) for the first time within the Bondi radius of a black hole. This observation will also provide the deepest look of the X-ray binary population of an S0 galaxy to date.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
10:05:13.90	-07:43:06.90	NGC3115	ACIS-S	NONE	125

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620024

Title: Black Hole X-ray Novae in M31

PI Name: Steve Murray

During A01-10 we found sufficient numbers of Black Hole X-ray Novae (BHXN) in M31 in order to estimate orbital periods for 10, and make the first comparison to the MW BHXN orbital period distribution. We propose to continue this Chandra/HST program, concentrating our scarce HST resources on a single transient which exceeds the NS Eddington limit. Only uninterrupted monitoring can yield the duty cycles and long-term lightcurves of BHXN (and other variables) in M31. Our GO+GTO programs have accumulated over 600ks (ACIS+HRC) near the M31 bulge. By continuing our monitoring program we will reach >750ks on the bulge and >1Msec total Chandra M31 exposure.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
00:42:44.40	+41:16:08.30	M31	ACIS-I	NONE	25

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620048

Title: Are the Observed Submm Flares Related to the X-ray/NIR Flares in Sgr A*?

PI Name: Gordon Garmire

We propose three 40-ks ACIS-I observations of the Galactic SMBH, SgrA*, with simultaneous NIR, submm, and mm monitoring. Our last two campaigns observed two flares simultaneously in the X-ray, NIR, and submm. We found a possible correlation between the X-ray to NIR flux ratio and the time lag of the submm peak in the two flares that can be explained with an adiabatically expanding relativistic plasma model. This project will test the proposed correlation and the expansion model for flare evolution; test the apparent overabundance of X-ray transients in the central pc; extend our survey of X-ray point sources to fainter fluxes; and measure the proper motion of variable Fe fluorescent features near SgrA* to test whether the SMBH was the irradiator, and hence more luminous in the recent past.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
17:45:40.00	-29:00:28.00	Sgr A*	ACIS-I	NONE	39.9
17:45:40.00	-29:00:28.00	Sgr A*	ACIS-I	NONE	39.9

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620101

Title: Constraining the transient LMXB population

PI Name: Giuseppina Fabbiano

We propose a single 110 ks ACIS-S observation of the well-studied nearby elliptical galaxy NGC 4278, to constrain the transient LMXB population, which is of compelling interest for binary evolution models. We expect that this observation will more than triple the size of the transient sample, and will result in a five-fold increase, if followed by another observation in a few years time. This is a unique opportunity for verifying widely discussed theories on the nature and evolution of LMXB populations that cannot be addressed with Galactic data.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
12:20:06.80	+29:16:50.70	NGC 4278	ACIS-S	NONE	110

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620107

Title: X-Rays from Blue Compact Dwarf Galaxies

PI Name: Philip Kaaret

Blue compact dwarf galaxies (BCDs) provide a local analog to the heavy element deficient conditions under which early galaxy formation occurred. All of the low metallicity BCDs observed with Chandra or XMM-Newton show strong X-ray emission. We propose a survey of nearby, low metallicity BCDs which will enable us to determine if the ratio of X-ray luminosity to star formation rate in BCDs is different from that in normal galaxies. Calibrating this relation for conditions similar to early galaxy formation is essential to using X-ray luminosity as a star formation indicator at high redshift.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
11:51:33.30	-02:22:22.00	UM 461	ACIS-S	NONE	38
09:56:46.00	+28:49:33.80	DDO 68	ACIS-S	NONE	10

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620112

Title: The ringed galaxy NGC1291

PI Name: Giuseppina Fabbiano

We propose to observe the nearby ring galaxy NGC1291, with two ACIS-S exposures to cover the northern and southern sides of the UV-bright ring for a total of 120 ks. Together with the ~80 ks archival ACIS-S data these observations will give us the unique opportunity to observe and study in detail the X-ray binary (XRB) population of a galactic ring, which includes two ULXs.These observations will also provide the means to study the LMXB population of the bulge down to the limiting sensitivity of deep studies of LMXB elliptical populations, and establish if the 5 1037 erg s-1 break observed in these XLFsis a general feature of LMXB populations. Finally, we will be able to set a stringent constraint to the gaseous fuel available to the faint nuclear supermassive black hole.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
03:17:20.40	-41:04:41.70	NGC 1291	ACIS-S	NONE	70
03:17:40.20	-41:08:41.30	NGC 1291	ACIS-S	NONE	50

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620243

Title: A new look at the X-ray binary richest galaxy

PI Name: Thomas Maccarone

We propose a 40 ksec observation of NGC 4472, the optically brightest galaxy in the Virgo Cluster, which remains one of the few bright nearby galaxies which has been the subject of only a single observation of more than 10 ksec. Previous observations showed many sources in the range between 4E+38 and 1E+39 ergs/sec, while other galaxies have not. These objects represent the best candidates for being transient black hole X-ray binaries with outburst durations much shorter than the 9 years since the previous deep observations. If found to be persistent, they would suggest a large ultracompact black hole X-ray binary population. These data will also present the first deep look at the globular cluster black hole in NGC 4472 since the XMM data which demonstrated its existence.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
12:29:46.80	+07:59:59.90	NGC 4472	ACIS-S	NONE	40

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620280

Title: Monitoring M31 for BHXNe

PI Name: Michael Garcia

During A01-9 we found ~25 Black Hole X-ray Novae (BHXNe) in M31 using Chandra, and with HST follow-up have estimated orbital periods for 9 of these. Observations are under way with HST to attempt to estimate additional periods. We propose to continue this program concentrating our scarce HST resources on a single transient which exceeds 1e38 erg/s. Only uninterrupted monitoring can yield the duty cycles and long-term light curves of BHXNe (and other variables) in M31. Our GO+GTO programs will have accumulated over 800ks (ACIS+HRC) near the M31 bulge by the end of A10, and total Chandra exposure on M31 is now almost 1Msec. By continuing our monitoring program through AO12 we will reach ~950ks on the bulge and >1Msec total Chandra M31 exposure.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
00:42:44.40	+41:16:08.30	M31	ACIS-I	NONE	25

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620296

Title: Search for the Most Luminous ULXs in Collisional Ring Galaxies

PI Name: Saul Rappaport

We propose to observe nine prominent collisional ring galaxies in order to explore the upper end of the luminosity function of ultraluminous X-ray sources (``ULXs''), i.e., with Lx > 10^{40} ergs/sec, and to investigate a possible cutoff at high luminosities. The significant numbers of ULXs in collisional ring galaxies, as well as their relatively simple geometry, make these galaxies good targets for such a study. The results may help determine the typical masses of the accretors in ULXs, and thereby bear on whether stellar mass black holes with M < 30 M_sun can radiate in a way that seems to violate the Eddington limit or, alternatively, on how intermediate mass black holes with masses of order 1000 M_sun can form and acquire massive companion stars.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
03:11:18.90	+01:18:53.00	Arp 147	ACIS-S	NONE	45

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620601

Title: Ultra-Luminous x-Ray Sources in the Most Metal-Poor Galaxies

PI Name: Andrea Prestwich

There is growing observational and theoretical evidence to suggest that Ultra-Luminous X-ray sources (ULX) form preferentially in low metallicity environments. Here we propose a survey of 27 nearby (< 30Mpc) star-forming Extremely Metal Poor Galaxies (Z<5% solar). There are almost no X-ray observations of such low abundance galaxies (3 in the Chandra archive). These are the most metal-deficient galaxies known, and a logical place to find ULX if they favor metal-poor systems. We plan to test recent population synthesis models which predict that ULX should be very numerous in metal-poor galaxies. We will also test the hypothesis that ULX form in massive young star clusters, and ask for HST time to obtain the necessay imaging data.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
01:13:39.40	+00:52:27.80	UGC 772	ACIS-S	NONE	5
21:04:55.30	-00:35:22.00	SDSS J210455.31-003522.2	ACIS-S	NONE	5
11:32:02.50	+57:22:45.70	SBS 1129+576	ACIS-S	NONE	15.03
08:25:55.50	+35:32:32.00	HS 0822+3542	ACIS-S	NONE	5
11:05:53.70	+60:22:28.70	SBS 1102+606	ACIS-S	NONE	10.261
12:01:22.30	+02:11:08.30	SDSS J120122.32+021108.5	ACIS-S	NONE	8.072
11:19:34.40	+51:30:12.10	[RC2] A1116+51	ACIS-S	NONE	10.901
09:44:16.60	+54:11:34.30	SBS 0940+544	ACIS-S	NONE	16.93
10:16:24.50	+37:54:46.00	KUG 1013+381	ACIS-S	NONE	9.411
12:30:48.50	+12:02:42.10	[RC2] A1228+12	ACIS-S	NONE	12.124
14:17:01.40	+43:30:05.50	SBS 1415+437	ACIS-S	NONE	5
04:05:20.40	-36:49:00.70	6dF J0405204-364859	ACIS-S	NONE	5
14:14:54.20	-02:08:22.90	SDSS J141454.13-020822.9	ACIS-S	NONE	16.75
22:30:36.80	-00:06:37.00	SDSS J223036.79-000636.9	ACIS-S	NONE	7.657
12:38:40.10	+32:46:00.50	UGCA 292	ACIS-S	NONE	5
14:44:12.80	+42:37:44.00	HS 1442+4250	ACIS-S	NONE	5
02:04:25.60	-10:09:35.00	KUG 0201-103	ACIS-S	NONE	13.596
08:12:39.50	+48:36:45.40	SDSS J081239.52+483645.3	ACIS-S	NONE	5
08:59:46.90	+39:23:05.60	SDSS J085946.92+392305.6	ACIS-S	NONE	5
07:47:32.10	+51:11:28.20	KUG 0743+513	ACIS-S	NONE	5
09:40:12.80	+29:35:30.30	KUG 0937+298	ACIS-S	NONE	5
09:46:22.80	+54:52:08.30	KUG 0942+551	ACIS-S	NONE	16.395

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620675

Title: The Deepest Stellar X-ray/optical Census of the Bulge

PI Name: William Clarkson

We have obtained the deepest optical dataset ever taken or planned towards the bulge, allowing bulge/disk decomposition down to F606W=23 and variability monitoring over seven days, diagnostics not available for any bulge field observed by Chandra. We propose ACIS-I imaging to identify X-ray point sources in this field. This will directly trace a number of fundamental yet poorly-constrained parameters of the inner Milky Way, for example the spin-down timescale of stars along the disk and bulge; the formation history of the bulge and, for the first time, direct constraints on the gravitational potential of the inner milky way through AGN-enabled absolute proper motions. Our proposed survey will be an essential calibrator for other X-ray/optical surveys of the bulge both past and planned.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
17:59:08.00	-29:14:05.00	SWEEPS_FIELD	ACIS-I	NONE	100

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620883

Title: Studying binary evolution in the oldest open clusters: Collinder 261

PI Name: Maureen van den Berg

We propose to extend our study of close interacting binaries in old open clusters by obtaining the first X-ray observation (55 ks) of the rich cluster Collinder 261 (7 Gyr). Based on our previous work we expect to detect a variety of binaries: active binaries, cataclysmic variables, and also anomalous binaries that formed in dynamical encounters. The latter are key to constraining the complex interaction between binary evolution and open-cluster dynamics that models are now trying to understand; X-ray observations are an efficient way to discover these rare and otherwise difficult-to-find systems. Since their age and distance are accurately known, the X-ray sources in Collinder 261 will be important benchmarks for the study of binary evolution and coronal activity.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
12:37:59.00	-68:22:40.00	Collinder 261	ACIS-I	NONE	55

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620895

Title: Low Mass X-ray Binaries in Spiral Galaxies

PI Name: Arunav Kundu

We propose to study the low mass X-ray binary (LMXB) populations of a sample of 7 edge-on spiral galaxies and their connection with globular clusters (GCs). Chandra studies have established that roughly half of the LMXBs in elliptical galaxies are associated with GCs. This systematic study of 7 edge-on spirals will establish the corresponding rate in GCs. This analysis will allow us to test whether the small correlation between the scatter in L_LMXB/L_Opt and morphological type is due to differences in the properties of LMXBs in GCs or the field, and the implications of such observations. We will combine the requested Chandra observations of 3 spiral galaxies with archival analysis of another 4, and our extant large field of view optical study of the GC systems.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
00:03:14.90	+16:08:44.00	NGC 7814	ACIS-S	NONE	60
12:11:04.40	+50:29:05.00	NGC 4157	ACIS-S	NONE	60
08:52:41.30	+33:25:19.00	NGC 2683	ACIS-S	NONE	40

Subject Category: NORMAL GALAXIES: X-RAY POPULATIONS

Proposal Number: 11620915

Title: Accretion onto nuclear black holes in early type galaxies: comparing field vs. clusters

PI Name: Elena Gallo

IF black holes are indeed ubiquitous in galactic nuclei, little is known about the frequency and intensity of their activity, the more so at the low-mass/low-luminosity end. Our cycle 8 observations of the Virgo clusters have delivered the most comprehensive measurement of the duty cycle, showing that although black holes are present even in low mass spheroids, activity is a strong function of mass. However, nuclear activity is also expected to be a strong function of environment, which regulates the gas supply through processes such as ram pressure stripping and merging. We propose the first systematic study of the effects of the environment on low level accretion, by combining our Virgo study with new observations and archival data of a volume limited sample of 100 field spheroids.

R.A.	Dec.	Target Name	Det.	Grating	Exp.Time
14:21:03.60	+03:16:15.71	NGC5576	ACIS-S	NONE	8.5
14:29:40.56	+03:14:00.67	NGC5638	ACIS-S	NONE	10.2
15:04:06.96	+01:13:11.68	NGC5831	ACIS-S	NONE	10.3
12:51:48.00	-10:27:17.21	NGC4742	ACIS-S	NONE	5.3
13:30:42.96	-22:25:15.92	ESO576-076	ACIS-S	NONE	8.8
12:51:06.72	+10:54:43.49	NGC4733	ACIS-S	NONE	3.5
12:42:56.40	+03:40:35.54	PGC042748	ACIS-S	NONE	3.5
13:21:19.44	-13:02:31.56	NGC5099	ACIS-S	NONE	5.7
12:37:48.24	-01:20:41.35	PGC042173	ACIS-S	NONE	8.2
15:03:50.40	+01:07:36.62	PGC1185375	ACIS-S	NONE	9.2
12:42:50.88	+12:18:31.50	PGC042737	ACIS-S	NONE	11
12:43:51.12	+11:28:01.31	PGC042846	ACIS-S	NONE	3.5
15:00:33.12	+02:13:49.30	SDSSJ150033.02+021349.1	ACIS-S	NONE	6.3
14:58:28.56	+01:32:34.91	SDSSJ145828.64+013234.6	ACIS-S	NONE	8.4
12:45:15.36	+07:36:56.45	PGC042982	ACIS-S	NONE	6.4
15:01:00.96	+01:00:49.68	SDSSJ150100.85+010049.8	ACIS-S	NONE	11.4
12:54:05.28	-00:06:04.54	PGC135814	ACIS-S	NONE	4.5
15:02:33.12	+01:56:08.95	SDSSJ150233.03+015608.3	ACIS-S	NONE	10.1
15:04:24.00	+00:55:06.20	PGC1179083	ACIS-S	NONE	10.2
12:42:45.36	+03:25:50.12	PGC042724	ACIS-S	NONE	1.7
15:01:16.08	+01:46:24.49	PGC1205406	ACIS-S	NONE	8.5
13:31:33.84	+02:11:17.16	PGC135829	ACIS-S	NONE	6.7
13:03:44.16	+02:02:23.86	PGC135818	ACIS-S	NONE	3.5
12:41:45.12	+04:00:23.62	PGC042596	ACIS-S	NONE	2.5
14:59:44.88	+02:07:51.82	SDSSJ145944.77+020752.1	ACIS-S	NONE	8
14:58:41.04	+02:20:23.50	PGC1223766	ACIS-S	NONE	9.5
12:50:07.44	+02:14:52.87	PGC043421	ACIS-S	NONE	4.2
15:02:28.32	+01:21:51.19	PGC1192611	ACIS-S	NONE	8.6
12:40:25.92	+04:03:01.01	PGC042454	ACIS-S	NONE	2.4
22:32:13.44	-41:10:09.52	PGC085239	ACIS-S	NONE	6.8
20:27:34.08	-55:05:23.82	PGC064718	ACIS-S	NONE	2
02:08:21.12	+10:59:47.04	NGC0821	ACIS-S	NONE	10.4
23:12:07.44	-28:32:26.20	NGC7507	ACIS-S	NONE	7.3
03:28:19.63	-31:04:05.09	NGC1340	ACIS-S	NONE	3.2
03:44:49.99	-21:55:15.60	NGC1439	ACIS-S	NONE	7.5
03:42:49.10	-22:06:30.10	NGC1426	ACIS-S	NONE	5.4
03:01:36.05	-14:50:11.80	NGC1172	ACIS-S	NONE	6.5
01:47:55.30	-26:53:31.88	IC1729	ACIS-S	NONE	6
03:35:14.62	-20:22:25.28	NGC1370	ACIS-S	NONE	2.6
02:26:28.30	+01:09:37.73	IC0225	ACIS-S	NONE	7.4
00:41:11.76	-21:07:53.11	ESO540-014	ACIS-S	NONE	7.9
23:37:39.60	+30:07:45.88	PGC071938	ACIS-S	NONE	7.8
00:23:04.20	-27:55:37.31	PGC132768	ACIS-S	NONE	6.5
02:41:25.51	-08:07:36.88	PGC3097911	ACIS-S	NONE	5.7
23:11:46.80	-28:31:45.12	PGC740586	ACIS-S	NONE	5.7
20:49:40.08	-32:41:53.02	6dFJ2049400-324154	ACIS-S	NONE	9
02:43:10.61	-00:15:45.72	PGC135659	ACIS-S	NONE	2.7
12:20:17.76	+75:22:15.38	NGC4291	ACIS-S	NONE	13.7
10:18:24.96	+21:53:38.29	NGC3193	ACIS-S	NONE	7.2
14:20:43.20	+39:41:36.89	NGC5582	ACIS-S	NONE	9.5
12:41:44.40	+74:25:15.10	NGC4648	ACIS-S	NONE	11
15:57:15.60	+05:59:54.10	NGC6017	ACIS-S	NONE	12.3
10:54:48.72	+17:37:13.40	NGC3457	ACIS-S	NONE	5.2
11:51:47.76	+48:40:59.20	NGC3457	ACIS-S	NONE	4.5
12:07:56.64	+65:06:50.40	NGC4121	ACIS-S	NONE	9.5
12:35:32.64	+73:40:29.39	UGC07767	ACIS-S	NONE	8.9
10:31:06.72	+28:47:47.65	NGC3265	ACIS-S	NONE	8.3
09:43:31.20	+31:58:36.84	NGC2970	ACIS-S	NONE	10.6
10:52:04.32	+71:46:22.91	UGC05955	ACIS-S	NONE	7.8
11:06:40.56	+20:05:08.38	NGC3522	ACIS-S	NONE	5.9
12:41:60.00	+32:34:25.00	NGC4627	ACIS-S	NONE	2
16:02:47.52	+19:47:14.75	PGC056821	ACIS-S	NONE	11.4
15:06:34.32	+01:33:31.79	PGC3119319	ACIS-S	NONE	8.7
14:58:46.08	+02:58:08.36	PGC1242097	ACIS-S	NONE	11.9
09:50:10.80	+28:00:47.59	PGC028305	ACIS-S	NONE	8.2
15:09:14.88	+01:55:17.08	PGC1210284	ACIS-S	NONE	11.3
10:19:01.44	+21:17:01.57	PGC030133	ACIS-S	NONE	4.6
15:05:50.64	+01:54:30.10	PGC1209872	ACIS-S	NONE	11.2
15:11:01.44	+01:40:50.20	PGC1202458	ACIS-S	NONE	11
15:04:24.72	+02:06:52.67	PGC1216386	ACIS-S	NONE	11.5
15:03:44.16	+02:33:08.68	PGC1230503	ACIS-S	NONE	11.7
15:09:07.92	+00:43:29.17	SDSSJ150907.83+004329.7	ACIS-S	NONE	10.4
15:08:12.48	+01:29:59.24	r	ACIS-S	NONE	9.9
15:08:22.80	+01:47:54.31	PGC1206166	ACIS-S	NONE	10.5
15:08:01.44	+02:09:03.67	PGC1217593	ACIS-S	NONE	4.5

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