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 1210-64 | 183.3036 | -64.8719 | 182.632422 | -64.593786 | 222.057216 | -55.171704 | 298.88624165 | -2.30082607 | 98.4956 | 55553.1591550926 | 2010-12-23 03:49:11 | 55555.1488194444 | 2010-12-25 03:34:18 | 405045010 | 79.3476 | 80 | 79.3476 | 79.3476 | 0 | 79.3561 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 70.7512 | 70.7512 | 171.8799 | 0 | PROCESSED | 57554.5554398148 | 2016-06-15 13:19:50 | 55961 | 2012-02-04 00:00:00 | 55595.085474537 | 2011-02-03 02:03:05 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051236 | 4U 1210-64 is a high mass X-ray binary with a stable 6.7 day period when the long-term (RXTE ASM) light curve is analyzed. However, we observed strong aperiodic variability in a series of pointed observations with the RXTE PCA, to the point of masking this 6.7 day period. Moreover, we have not detected a spin period, even though the accretor is most likely a neutron star. The strong variability is suggestive of accretion from a clumpy wind. We propose a 2-day Suzaku observation of this object (1) to search for unequivocal evidence for a neutron star, such as the spin period and cyclotron features; and (2) to measure the spectral shapes at different flux levels, to investigate the cause of the strong aperiodic variability. | GALACTIC POINT SOURCES | 4 | C | KOJI MUKAI | USA | 5 | AO5 | 4U 1210-64: A HIGHLY VARIABLE X-RAY BINARY | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405045010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '405045010'
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