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 SU AUR 73.9934 30.5715 73.195309 30.492884 76.133121 7.898373 172.51103259 -7.93275707 85.9197 54339.1713541667 2007-08-27 04:06:45 54340.7502199074 2007-08-28 18:00:19 402090010 57.3034 55 57.3114 57.3034 0 57.3114 2 2 0 2 1 0 0 54.3848 54.3848 136.4018 1 PROCESSED 57539.9114699074 2016-05-31 21:52:31 54723 2008-09-14 00:00:00 54350.6381597222 2007-09-07 15:18:57 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 022007 We propose to observe the cTTS TW~Hya, SU~Aur and XZ~Tau with the Suzaku XIS in order to search for soft X-ray "excesses", indicating the presence of accretion induced X-rays in cTTS. We plan to utilize the sensitivity and capability of the Suzaku XIS to resolve the OVIII/OVII lines.With grating observations the absence of the forbidden line in the latter was found to provide strong evidence for the presence of accretion in the X-ray spectra of a few cTTS. With the increased sensitivity of Suzaku the presence of soft X-ray excesses can be demonstrated in a far larger sample of stars, and we want to demonstrate the existence of a soft X-ray, probably accretion induced component in cTTS with extremely hot coronae exhibiting the presence of the 6.7 keV iron line complex in their spectra. GALACTIC POINT SOURCES 4 A JURGEN SCHMITT EUR 2 AO2 ACCRETION RELATED SOFT X-RAY EMISSION IN CLASSICAL T TAURI STARS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402090010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402090010'

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