Follow-on Science Instrument
Monthly Status Report No. 002
Prepared in accordance with DR 972MA-002
DPD #972
Prepared for
National Aeronautics and Space Administration
Marshall Space Flight Center, Alabama 35812
Center for Space Research
Massachusetts Institute of Technology
Cambridge,
MA 02139
1.0 Distribution List for Monthly Status Report
MIT-External Electronic:
FD03/Mike Smith, MSFC Carl.M.Smith@msfc.nasa.gov
PS41/Steve Morris, MSFC Steven.D.Morris@msfc.nasa.gov
MIT-External Hardcopy:
None specified.
MIT-Internal Electronic:
Deborah Gage dgage@space.mit.edu
Gail Monahan gmonahan@mit.edu
MIT-Internal Hardcopy:
Claude Canizares Room 37-582G (via Gail Monahan)
Please send distribution requests and other comments on this document to dd@mit.edu .
2.0 Schedule of Past and Future Events Relevant to HETG
Date |
Past Events |
Comment |
April 20-23 |
HEAD meeting, Albuquerque |
N103B poster, 4U 0142+61, EXO 0748, etc. |
April 23,24 |
Chandra Quarterly at OCC |
HETG for ~15 min. |
Date |
Future Events |
Comment |
May 24- June 3 |
4th Microquasar Workshop, Corsica, France. |
Dr. Lee attending. |
June 2-6 |
AAS meeting, Albuquerque |
|
June 18-20 |
Chandra Peer Review |
2 GTO proposals competing |
July TBD |
Chandra Quarterly at TBD |
|
Aug. 25-28 |
SPIE conference |
|
Oct. 10-12 |
34th COSPAR, Houston TX: E1.2 …clusters of galaxies and black holes E1.4 …supernova remnants and neutron stars |
|
Oct. TBD |
Chandra Quarterly at TBD |
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Oct./Nov. |
Proposers’ Observatory Guide |
HETG provide input |
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3.0 Instrument Status and Science Support
3.1 Flight Events and HETG Instrument Status
The HETG continues to function with no outstanding issues.
There were 9 targets observed in 11 observation intervals by the HETG in April 2002. One target, Capella, is an HETG Calibration observation and will be analyzed when data are available (early May.) Two of the targets are in the HETG GTO program and will be examined in detail by the HETG group.
The HRMA PSF, which is crucial to the HETG’s high resolution, continues to be stable based on occasional analyses of the width of the ACIS frame-transfer streak in bright point-source HETG observations. Observations of PKS 2155-204 and Cygnus X-1 were recently analyzed and added to the FWHM plot, shown on next page.
3.2 Science Support to CXC, SWG, etc.
E0102 images were provided to Project Science / Weisskopf for use in Structure and Evolution of Universe talk.
Participated in Chandra Quarterly review at OCC, Cambridge MA.
The HRMA PSF core width is monitored by measuring the FWHM of the ACIS
frame-transfer streak. Over two years of data show a very stable FWHM.
4.0 GTO Science Program
4.1 Observations and Data status
Progress in the GTO program observations and data analyses are noted in the Table of Appendix A.
4.2 Science theme progress
The HETG GTO science efforts span a range of “science themes” given in the list below. In each month’s report progress and plans in one of these themes will be highlighted, in addition to the terse incremental progress notes given in the Table of Appendix A. For each listed theme the date of its last progress reporting is also given for reference.
GTO Science Theme |
Date of last reporting |
Stars |
Not yet reported |
X-ray Binaries |
Not yet reported |
Supernova Remnants |
Not yet reported |
Neutron Stars |
Not yet reported |
Galaxies and Galaxy Clusters |
Not yet reported |
Active Galactic Nuclei |
Not yet reported |
ISM and IGM Absorption |
Not yet reported |
No theme is reported this month.
4.3 HETG-related Software: Development, Evaluation, and Support
In the process of carrying out the HETG GTO science program, the HETG scientist make use of existing analysis and modeling software and are engaged in helping to modify current and design future software. Notable efforts in this direction will be described here in future report issues.
4.4 Presentations (March and April)
Canizares, C.: “Instrumentation for High Resolution X-ray Spectroscopy” a talk at the Symposium honoring A. Brinkman, ESTEC, Nordwijk, The Netherlands, April 5, 2002.
Juett, A.M., “Chandra/HETGS Spectroscopy of the Anomalous X-ray Pulsar 4U 0142+61”, a talk at the 2002 HEAD meeting, Albuquerque.
Jimenez-Garate, M.A., “X-ray Spectroscopy of Her X-1 and the Detection of CNO-processed Material”, a poster at the 2002 HEAD meeting, Albuquerque.
Canizares, C.: “Probing the Violent Universe with the Chandra X-ray Observatory” a talk at the Symposium in memory of Herbert Friedman, Philosophical Society, Philadelphia. April 25, 2002.
Migliazzo, J. et al., “A New Look at N103B with the Chandra HETGS”, a poster at the 2002 HEAD meeting, Albuquerque.
4.5 Publications (March and April), see also: http://space.mit.edu/csr_pubs.html
Canizares, C., “Recent X-Ray Observations of Supernova Remnants”, to appear in Phil. Trans. Roy. Soc., submitted.
Marshall, H.L. and Schulz, N.S., “Using the High Resolution X-ray Spectrum of PSR B0656+14 to Constrain the Chemical Composition of the Neutron Star Atmosphere”, Ap. J., in press, 2002. [CSR-02-12]
Lee, J.C. et al., “Confirmation of the Relativistic Iron K-alpha Emission and Limits on the Narrow Core with Chandra HETGS-RXTE Observations of MCG-6-30-15, Ap. J. Letters, in press, 2002. [CSR-02-15]
Juett, A.M., et al., “Chandra High Resolution Spectrum of the Anomalous X-ray Pulsar 4U 0142+61”, Ap. J. Letters, 568, L31, 2002. [CSR-02-16]
Fang, T. et al., “A Chandra HETG Observation of the Quasar H 1821+643 and Its Surrounding Cluster”, Ap. J., 565, 86, 2002. [CSR-02-16.5]
Fang, T. et al., “Chandra Detection of OVIII Ly$\alpha$ Absorption from an Overdense Region in the Intergalactic Medium”, accepted to ApJ. [CSR-02-??]
5.0 Systems and Engineering Support
5.1 Documentation and “Knowledge Capture”
Attended Dan Shropshire’s demo of Chandra “document” database during the Chandra Quarterly review.
5.2 Spares Retest and Test Instrumentation
1. Vacuum Storage Gratings are due for re-test. The test is delayed because of failure of the Vacuum Gauge Controller. The controller was returned to the manufacturer for repair. The manufacturer has not yet given an estimate of the repair schedule, but the MIT estimate is two weeks or less.
2. The four computers which are part of the X-GEF and LR test instruments will no longer be supported long before the end of the planned Chandra mission. We have begun a low level effort to identify spares as other computers in CSR are replaced with more powerful versions. We anticipate minimal hardware costs.
3. The primary archival machine, named "caliber", operates on the Sun OS4 operating system, which is no longer supported. We are still operating on Sun OS4 because the software is configuration controlled. We have to perform additional manual steps to manage data storage because the volume of data accumulated is a challenge for OS4. We anticipate operating another computer on Solaris in parallel, so that when "caliber" fails, we will have confidence in the replacement hardware and software.
4. The Labview software for the MAC's was written by a now defunct outside vendor. We are working on upgrading the documentation.
5.3 Anomalies, Insert/retract, etc. Support
No actions this month.
6.0 Management
6.1 Program Office & NASA Support
Supported monthly Chandra telecon and 9th Chandra Quarterly Review at OCC, Cambridge.
Responded to question about GFE equipment list, contract attachment D – will finalize modifications to
Attachment D soon.
6.2 MIT-internal management activities
Just the usual.
7.0 Open Issues, Problems, etc.
There are no known critical open issues or problems regarding the HETG.
There are no outstanding requests for travel or equipment.
Thanks to MSFC for timely approval of the recent request for Dr.Lee’s foreign travel.
Appendix A. GTO Observation Status Tables
Notes:
1. Entries indicating progress during this period are shown in this font.
2. For CSR Publication references (CSR-YY-NN) see http://space.mit.edu/csr_pubs.html
3. Up-to-date observation information can be obtained from http://cxc.harvard.edu/cda/ using the WebChaSeR link.
4. Due to time limitations all previous work has not been indicated in the 3 right-most columns – subsequent reports will be more complete.
Object |
AO |
Obs ID |
Seq. No. |
Expos. (ks) |
Observer / Analyst |
Start Date |
Comments & Analysis |
Talks and Publications |
4U 1626-67 |
4 |
--- |
--- |
[100.0] |
N. Schulz |
|
Prop. No.: 04400027 |
|
Sco X-1 |
4 |
--- |
--- |
[15.0] |
N. Schulz |
|
Prop. No.: 04400046 |
|
H1426+428 |
4 |
--- |
--- |
[102.0] |
T. Fang |
|
Prop. No.: 04700987 |
|
Mrk 290 |
4 |
--- |
--- |
[250.0] |
J. Lee |
|
Prop. No.: 04700988 |
|
TV Crit |
4 |
--- |
--- |
[100.0] |
D. Huenemoerder |
|
Prop. No.: 04200007, Competitive w/GOs |
|
E0102 |
4 |
--- |
--- |
[140.0] |
K. Flanagan |
|
Prop. No.: 04500008, Competitive w/GOs |
|
Cycle 3
Object |
AO |
Obs ID |
Seq. No. |
Expos. (ks) |
Observer / Analyst |
Start Date |
Comments & Analysis |
Talks and Publications |
MRC 2251-178 |
3 |
2977 |
700416 |
[150.0] |
J. Lee/ H. Marshall |
--- |
Scheduled: 9/10/02 |
|
NGC 7469 |
3 |
3147 |
700586 |
[70.0] |
J. Lee/ H. Marshall |
--- |
Scheduled: 9/4/02 |
|
1H 0414+009 |
3 |
2969 |
700408 |
[93.0] |
T. Fang |
--- |
Scheduled: 8/1/02 |
|
GX 349+2 |
3 |
3354 |
900193 |
35.2 |
N. Schulz |
4/9/02 |
Observed on 4/9; data available 5/2 |
|
NGC 2362 |
3 |
2525, 2526 |
200133, 200134 |
44.5, 43.8 |
N. Schulz |
3/28/02, 4/23/02 |
Data are in-house. Observed 4/23. |
|
1ES 1028+511 |
3 |
2970, 3472 |
700409 |
21.8, 69.6 |
T. Fang |
3/27/02, 3/28/02 |
Both data sets are in-house. |
|
3C 279 |
3 |
2971 |
700410 |
108.2 |
T. Fang |
3/21/02 |
Data are in-house [3/02]. |
|
IRAS 18325-5926 |
3 |
3148, 3452 |
700587 |
56.9, 51.1 |
J. Lee |
3/19/02, 3/23/02 |
Data are in-house [3/02]. |
|
Cycle 2
Object |
AO |
Obs ID |
Seq. No. |
Expos. (ks) |
Observer / Analyst |
Start Date |
Comments & Analysis |
Talks and Publications |
Cyg X-2 |
2 |
1016 |
400094 |
15.1 |
N. Schulz |
8/12/01 |
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|
Cas A |
2 |
1046 |
500112 |
69.9 |
K. Flanagan, D.Dewey |
5/25/01 |
Si knot analysis started [3/02]. |
|
4U 0142+61 |
2 |
1018 |
400096 |
25.4 |
N. Schulz, A. Juett |
5/23/01 |
Finishing additional analysis [3/02] |
HEAD-2002, CSR-02-16[3/02] |
Mrk 766 |
2 |
1597 |
700213 |
90.5 |
P. Ogle, J. Lee |
5/7/01 |
Paper in preparation. |
|
NGC 4696 |
2 |
1560 |
600117 |
85.8 |
M. Wise |
4/18/01 |
|
|
EXO 0748-676 |
2 |
1017 |
400095 |
49.0 |
N. Schulz |
4/14/01 |
|
|
SS 433 |
2 |
1019, 1020 |
400097, 400098 |
23.7, 23.0 |
H. Marshall |
3/16/01, 11/28/00 |
|
CSR-02-01 |
H 1821+643 |
2 |
1599 |
700215 |
101.3 |
P. Ogle, T. Fang |
2/9/01 |
|
CSR-02-16.5 |
Iota Orionis |
2 |
599, 2420 |
200075 |
37.6, 12.9 |
N. Schulz |
2/7/01, 2/8/01 |
|
|
TY Pyx (HD77137) |
2 |
601 |
200076 |
49.8 |
D. Huenemoerder |
1/3/01 |
|
|
N103B |
2 |
1045, 2410, 2416 |
500111 |
74.0, 25.7, 17.6 |
K. Flanagan, J. Migliazzo, D. Dewey |
1/1/01, 1/3/01, 1/2/01 |
NEI, vshock, and Si 2-D analyses. 1-D and 2-D analyses started [3/02] |
HEAD-2002 |
NGC 5506 |
2 |
1598 |
700214 |
90.0 |
P. Ogle, J. Lee |
12/31/00 |
Paper in preparation. |
|
ZW 3146 |
2 |
1651 |
800119 |
167.8 |
M. Wise |
12/25/00 |
|
|
Cycle 1
Object |
AO |
Obs ID |
Seq. No. |
Expos. (ks) |
Observer / Analyst |
Start Date |
Comments & Analysis |
Talks and Publications |
NGC 1068 |
1 |
332 |
700004 |
46.3 |
H. Marshall, P. Ogle |
12/4/00 |
Paper in preparation. |
|
4U 1626-67 |
1 |
104 |
400017 |
40.0 |
N. Schulz |
9/16/00 |
|
|
AR Lac |
1 |
6,7,8, 9,10,11 |
20000N: 4,5,6,7,8,9 |
32.5,7.5, 7.5,32.6, 7.3,7.3 |
D. Huenemoerder |
9/11/00- 9/19/00 |
|
Internal draft circulated. Paper started [3/02] |
Abell 1835 |
1 |
49896 511 |
800019 |
9.8 127.0 |
M. Wise |
8/25/00 8/26/00 |
|
|
N132D |
1 |
121, 1828 |
500008 |
22.3 77.6 |
K. Flanagan, D. Dewey |
7/19/00 7/20/00 |
|
|
TW Hydra |
1 |
5 |
200003 |
48.3 |
D. Huenemoerder |
7/18/00 |
|
CSR-02-02 |
NGC 4486 |
1 |
241 |
600001 |
38.5 |
M. Wise |
7/17/00 |
|
|
GX 301-2 |
1 |
103 |
400016 |
40.0 |
N. Schulz |
6/19/00 |
Re-analysis initiated [3/02] |
Draft paper begun [3/02] |
NGC 1399 |
1 |
49898, 240, 2389 |
600214 600000 |
13.2 44.1 14.8 |
M. Wise |
5/8/01 6/15/00 5/8/01 |
|
|
Vela X-1 |
1 |
102 |
400015 |
28.4 |
N. Schulz |
4/13/00 |
|
|
MCG –6-30-15 (w/Fabian) |
1 |
433 |
700105 |
128.2 |
H. Marshall, J. Lee |
4/5/00 |
|
Lee et al 2002, CSR-02-15 [3/02] |
NGC 4151 |
1 |
335 |
700007 |
48.0 |
H. Marshall |
3/5/00 |
|
|
PSR B0656+14 |
1 |
130 |
500017 |
38.1 |
H. Marshall |
11/28/99 |
LETG/HRC |
Paper accepted, CSR-02-12[3/02] |
PKS 2149-306 |
1 |
336, 1481 |
700008 |
36.0 54.8 |
H. Marshall |
11/18/99 11/20/99 |
|
|
Trapezium |
1 |
3, 4 |
200001 200002 |
50.1 31.3 |
N. Schulz |
10/31/99 11/24/99 |
|
Detailed modeling paper started [3/02] |
4U 1636-53 |
1 |
105 |
400018 |
29.8 |
N. Schulz |
10/20/99 |
|
|
PKS 2155-304 |
1 |
337, 1703, 1705 |
700009 700261 700263 |
39.1 26.2 25.8 |
H. Marshall |
10/20/99 5/31/00 5/31/00 |
HETG and LETG w/ACIS-S |
Paper accepted. Responded to referee [3/02] |
Cyg X-1 |
1 |
107, 1511 |
400020 |
2.5 12.6 |
N. Schulz, H. Marshall |
10/19/99 1/12/00 |
Second paper started. Paper in process [3/02] |
|
II Peg (HD 224085) |
1 |
1451 |
200010 |
43.3 |
D. Huenemoerder |
10/17/99 |
|
|
Q0836+7104 |
1 |
1450, 1802 |
700006 |
61.0 14.1 |
H. Marshall |
10/17/99 8/25/00 |
|
|
PKS 0745-191 |
1 |
510, 1509, 1509 |
800018 |
45.3, 40.4, 39.9 |
M. Wise |
10/14/99 4/25/00 3/4/00 |
|
ApJ submitted, Hicks et al. [3/02] |
PSR B0833-45 |
1 |
131 |
500018 |
36.1 |
H. Marshall |
10/12/99 |
|
|
NGC 1275 |
1 |
333, 428 |
700005 700201 |
53.2 25.0 |
H. Marshall |
10/10/99 8/25/00 |
|
|
E0102 |
1 |
120, 968 |
500007 |
88.2, 49.0 |
K. Flanagan, A. Fredricks |
9/28/99 10/8/99 |
Fluxes and ratios in “arc”. Initial calc O mass. |
More progress on ApJ paper [3/02] |
SS 433 |
1 |
106 |
400019 |
28.9 |
N. Schulz, H. Marshall |
9/23/99 |
|
|
Object |
AO |
Obs ID |
Seq. No. |
Expos. (ks) |
Observer / Analyst |
Start Date |
Comments & Analysis |
Talks and Publications |
Cycle 1