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 | 4U 0115+63 | 19.6139 | 63.7554 | 18.78861 | 63.492562 | 49.805717 | 49.807631 | 125.91367385 | 1.04017806 | 82.1235 | 55750.053587963 | 2011-07-08 01:17:10 | 55751.0210763889 | 2011-07-09 00:30:21 | 406049010 | 42.2748 | 45 | 42.2748 | 42.3548 | 0 | 42.3548 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 42.1432 | 42.1432 | 83.5779 | 1 | PROCESSED | 57602.5577662037 | 2016-08-02 13:23:11 | 56163 | 2012-08-24 00:00:00 | 55778.4311226852 | 2011-08-05 10:20:49 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061234 | We propose to perform Target of Opportunity observations of one accreting neutron star that is a known cyclotron line source, out of a sample of five, in outburst. The aim is to observe the source for 50 ks at a level of >~40 mCrab and for another 45 ks at >~200 mCrab, in order to determine the properties of the cyclotron line(s) and constrain the broad band spectrum at different luminosities. These measurements have implications for the B-field strength and geometry as well as the properties of the accreted plasma. | GALACTIC POINT SOURCES | 4 | A | KATJA POTTSCHMIDT | USA | 6 | AO6-TOO | CYCLOTRON LINES IN TRANSIENT PULSARS I: PROBING THE B-FIELD | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406049010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '406049010'
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