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 | 1RXS J070407.9+26250 | 106.0341 | 26.4126 | 105.260164 | 26.487679 | 104.355942 | 3.767203 | 190.27497025 | 14.29877104 | 282.0717 | 54548.4868865741 | 2008-03-23 11:41:07 | 54549.9862384259 | 2008-03-24 23:40:11 | 402008010 | 58.3157 | 50 | 58.3237 | 58.3157 | 0 | 58.3237 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 49.4766 | 49.4766 | 129.5278 | 0 | PROCESSED | 57541.9808912037 | 2016-06-02 23:32:29 | 54933 | 2009-04-12 00:00:00 | 54566.326712963 | 2008-04-10 07:50:28 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020029 | Soft Intermediate Polar (IP) is a small group of IPs whose X-ray spectrum is extremely soft compared with general IPs. Recent observations reveal that some soft IPs harbor a soft blackbody component like polars, yet its nature is not fully understood. Systematic study of the soft IP blackbody emission is important in the sense that it may provide a clue to understand possible evolutionary link from IPs to polars, the origin of the soft excess in polars, etc. We propose to observe five soft IPs, each for 50ksec, in order to search for the blackbody component and to measure their temperature and flux systematically. | GALACTIC POINT SOURCES | 4 | C | MANABU ISHIDA | JAP | 2 | AO2 | OBSERVATIONS OF SOFT INTERMEDIATE POLARS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402008010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402008010'
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