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 106.0316 26.4199 105.25762 26.494968 104.352906 3.774212 190.26714041 14.29962915 96.1437 54749.1266319444 2008-10-10 03:02:21 54750.3682175926 2008-10-11 08:50:14 403003010 53.5519 50 53.5519 53.5519 0 53.5519 2 2 0 2 1 0 0 41.1405 41.1405 107.2319 0 PROCESSED 57544.1456944445 2016-06-05 03:29:48 55148 2009-11-13 00:00:00 54780.5445949074 2008-11-10 13:04:13 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030009 Soft Intermediate Polar (IP) is a group of IPs whose X-ray spectra are extremely soft compared with general IPs. Recent observations reveal that some soft IPs have a soft blackbody emission 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 comprehensively the emission characteristics of polars and IPs in the soft X-ray band, and to follow possible evolutionary link from IPs to polars, etc. We propose to observe five soft IPs, each for 50ksec, in order to search for the blackbody component and to measure its temperature and flux systematically. GALACTIC POINT SOURCES 4 B MANABU ISHIDA JAP 3 AO3 OBSERVATIONS OF SOFT INTERMEDIATE POLARS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403003010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏