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 | A0535+026 | 84.7243 | 26.3189 | 83.946776 | 26.291426 | 85.267864 | 2.964757 | 181.44092218 | -2.64422146 | 83.608 | 53627.5694907407 | 2005-09-14 13:40:04 | 53628.0418865741 | 2005-09-15 01:00:19 | 100021010 | 21.761 | 20 | 21.761 | 21.761 | 21.761 | 21.761 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 21.2572 | 21.2572 | 40.7839 | 1 | PROCESSED | 57527.3122337963 | 2016-05-19 07:29:37 | 54247 | 2007-05-27 00:00:00 | 54035.0644444444 | 2006-10-27 01:32:48 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000021 | We propose to observe the X-ray binary pulsar A0535+26. The main objectives is measuring changes in the cyclotron resonance energy in an outburst decay.It is known from another X-ray pulsar 4U0115+63 that the cyclotron resonance energy increased from 11 keV to 16 keV, as the luminosity decreased across a threshold luminosity of 4x10^37 erg/s. The flare of A0535+26 is a chance to know whether this behavior is the RULE among binary pulsars or an EXCEPTION. A0535+26 is fading down and will reach 30mCrab (5-100keV) on September 17, which is 5x10^36 erg/s. It is better to be observed as soon as possible, before it fades out. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | TOO Observation of A0535+026 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100021010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100021010'
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