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 | 4U1538-522 | 235.6015 | -52.3857 | 234.665107 | -52.226494 | 246.064673 | -31.762519 | 327.42188954 | 2.16239803 | 275.2972 | 56149.0031134259 | 2012-08-10 00:04:29 | 56149.7349537037 | 2012-08-10 17:38:20 | 407068010 | 45.9554 | 40 | 45.9554 | 45.9554 | 0 | 45.9554 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 40.05 | 40.05 | 63.212 | 0 | PROCESSED | 57606.8269444444 | 2016-08-06 19:50:48 | 56640 | 2013-12-14 00:00:00 | 56272.688900463 | 2012-12-11 16:32:01 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071233 | Observations of accreting pulsars in High Mass X-ray Binaries (HMXBs) provide us with important information about the physical processes in the stellar wind of the high mass donor star, the coupling between the accreting material and the neutron star's magnetic field, and the physics of the strongly magnetized accretion column above the neutron star. In this proposal we ask for a 40 ks observation of the accreting HMXB 4U1538-522 to conduct the most sensitive study to date of the wide range of characteristics of the broad band (0.1-100 keV) spectrum over a quarter of a binary orbit and with pulse phase. When one considers the ~50% duty cycle of Suzaku observations, the proposed observation will yield coverage of a quarter of the binary orbit. | GALACTIC POINT SOURCES | 4 | A | RICHARD ROTHSCHILD | USA | 7 | AO7 | THE FIRST SUZAKU OBSERVATION OF 4U1538-522 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407068010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '407068010'
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