DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | 4U1700-37 | 255.9894 | -37.8441 | 255.139416 | -37.774677 | 258.577099 | -14.956185 | 347.75582102 | 2.17172645 | 269.6945 | 53991.447662037 | 2006-09-13 10:44:38 | 53992.918912037 | 2006-09-14 22:03:14 | 401058010 | 81.4425 | 80 | 81.4569 | 81.4704 | 81.4425 | 81.4544 | 3 | 3 | 3 | 3 | 1 | 0 | 0 | 82.1093 | 82.1093 | 127.109 | 1 | PROCESSED | 57535.6097916667 | 2016-05-27 14:38:06 | 54526 | 2008-03-01 00:00:00 | 54053.5428240741 | 2006-11-14 13:01:40 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011135 | The compact object in the massive X-ray binary 4U1700-37/HD153919 has been inferred to be a neutron star based on its spectral shape, but no pulsations have been observed. One possible explanation for the absence of observed pulsations is that the pulsed signal is beamed in directions other than our line of sight. This can be tested using Suzaku by searching for pulsations in the iron K line. This line is formed efficiently under almost all conditions of ionization and temperature, and so represents an X-ray bolometer which should respond to pulsed X-rays no matter where they are pointed. We plan to make such a search, and to probe the other properties of the wind and compact object in this system by observing with Suzaku for 80 ks away from eclipse. | GALACTIC POINT SOURCES | 4 | A | TIMOTHY KALLMAN | USA | 1 | AO1 | IRON LINE VARIABILITY IN 4U1700-37 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401058010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '401058010'
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