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
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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