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.
observation_id
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
exposure
awarded_exposure
xtend_exposure
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
xtend_data_mode1
xtend_data_mode2
1 201108010 WR140 305.11507 43.85461 304.69305 43.69532 327.36841 60.49261 80.92972 4.17805 283.34756 60587.46255 2024-10-04 11:06:04 60588.95560 2024-10-05 22:56:04 104.066 45.000 59.588 2 31100010 320000A0 63.738 59.588 0.000 0.000 11110 11310 PROCESSED 2024-10-18 00:19:49 2025-10-19 00:00:00 2024-10-15 16:28:10 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012182 Cosmic dust is a primary building block of the Earth, and its formation is a fundamental question. The massive colliding wind binary system, WR140, produces massive dust near periastron of its 7.9-year-long orbit. During the dust emission rise in previous binary cycles, the CIII line excess enhanced, and the X-ray emission declined oppositely, suggesting strong cooling of the WWC plasma produced a condition for dust formation. The star experiences another periastron passage on November 22nd, 2024. We propose 3 XRISM observations around that time to study the location and motion of the WWC plasma using the Fe XXV emission line. We also expect to detect the fluorescent Fe line, which strongly constrains the distance of the WWC apex from the stellar surface. STELLAR CORONAE, WINDS, AND YOUNG STARS 2 A KENJI HAMAGUCHI USA 1 NOR DYNAMICS OF THE EXPLOSIVE DUST FORMATION NEAR PERIASTRON IN WR140 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201108010/ Quick Look 304.49026 43.56877 305.34759 43.42312 305.55539 44.04666 304.68843 44.19395 304.0677 43.41198 304.92168 43.26292 305.13364 43.88562 304.27016 44.03636 326.28796 60.44693 327.26673 60.03223 328.11988 60.51429 327.13606 60.93572 80.43836 4.39157 80.66821 3.79538 81.26831 4.02536 81.03851 4.62245 WINDOW2 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '201108010'

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