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 | CENTAURUS X-3 | 170.3244 | -60.5721 | 169.768632 | -60.297812 | 209.195093 | -56.294338 | 292.07802241 | 0.38603209 | 97.3521 | 54808.2886111111 | 2008-12-08 06:55:36 | 54810.2085532407 | 2008-12-10 05:00:19 | 403046010 | 97.5871 | 90 | 97.5871 | 97.5871 | 0 | 97.5871 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 79.6562 | 79.6562 | 165.8537 | 0 | PROCESSED | 57544.7036805556 | 2016-06-05 16:53:18 | 55188 | 2009-12-23 00:00:00 | 54822.6243634259 | 2008-12-22 14:59:05 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031154 | We ask for a 90 ks observation (which will be performed within typically 180 ks taking Suzaku's duty cycle into account) of the accreting HMXB Centaurus X-3 to conduct the most sensitive study to date of the wide range of changes of its broad band spectrum over one 2.1 binary orbit and with pulse phase. Especially we will determine the evolution of the hydrogen absorption column over the orbit and test whether signatures of the tidal wake observed with RXTE can be confirmed. The variable Fe line complex will be studied. The cyclotron resonance scattering feature of Cen X-3 at ~30 keV is especially well suited to test new physical models describing phase-resolved line profiles, since it is very variable over the pulse, with the line centroid spanning an energy range from 28 to 39 keV. | GALACTIC POINT SOURCES | 4 | A | KATJA POTTSCHMIDT | USA | 3 | AO3 | THE BROAD BAND SPECTRUM OF CEN X-3 OVER ORBIT AND PULSE PHASE | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403046010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403046010'
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