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 J062518.2+73343 | 96.3307 | 73.5671 | 94.750009 | 73.593987 | 92.79758 | 50.188181 | 140.86801575 | 24.12512545 | 262.0383 | 54570.0388310185 | 2008-04-14 00:55:55 | 54571.1252777778 | 2008-04-15 03:00:24 | 403004010 | 50.3267 | 50 | 50.3267 | 50.3267 | 0 | 50.3267 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 50.1253 | 50.1253 | 93.8488 | 0 | PROCESSED | 57542.3202430556 | 2016-06-03 07:41:09 | 54953 | 2009-05-02 00:00:00 | 54581.2328472222 | 2008-04-25 05:35:18 | 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/ver3.0/403004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403004010'
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